xmatch_obsxmatch_obs.allwiselamost_decTarget observation datepos.eq.decdoublelamost_ra_obsLocal modified Julian daydoublelamost_dec_obsModified Julian daydouble"__id__"Plan nameintdesignationSpectrograph IDcharlamost_ra_2Fiber IDdoublelamost_dec_2Fiber pointing right ascension (degree)doublesigdecS/N of u filterdoublesigradecS/N of g filterdoubleglonS/N of r filterdoubleelonS/N of z filterdoublewyRedshiftdoublecntrRedshift uncertaintylongsource_idThe objID in the Pan-STARRS catalogcharsrcPan-STARRS r band magnitudeintw1rchi2The "source_id" field of Gaia DR3 catalogdoublew2snrWhether there is a fiber offset during observationdoublew3snrSpectral sub-types of white dwarf starsdoublew4rchi2Metallicity uncertainty obtained by the LASPdoublenbUncertainty of heliocentric radial velocity obtained by the LASPintw1satThe uncertainty of alpha_mdoublew2satProjected rotation velocity given by the LASPdoublew3satOptical depth at the Balmer edge of 3646 ÅdoublesatnumThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingintdec_pmContinuum luminosity in common logarithm at rest-frame 1350 Ådoublesigdec_pmContinuum luminosity in common logarithm at rest-frame 5100 Ådoublesigradec_pmThe name of the first group of spectral linesdoublepmdecReduced chi-square in the fitting of the first group linesintw1rchi2_pmThe name of the second group of spectral linesdoublew3rchi2_pmMinimal chi-square in the fitting of the second group linesdoublew4rchi2_pmReduced chi-square in the fitting of the second group linesdoublerchi2_pmDegree of freedom in the fitting of the second group linesdoublepmcodeThe name of the first group of spectral linescharrelMinimal chi-square in the fitting of the third group linescharext_flgReduced chi-square in the fitting of the third group linesintph_qualThe name of the fourth group of spectral lineschardet_bitThe fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intmoon_levMinimal chi-square in the fitting of the fourth group linesintw2nmThe name of the fifth group of spectral linesintw3nmMinimal chi-square in the fitting of the fifth group linesintw4nmDegree of freedom in the fitting of the fifth group linesintw3covReduced chi-square in the fitting of the sixth group linesdoublew4covDegree of freedom in the fitting of the sixth group linesdoublew1cc_mapPeak flux of Lya broad componentintw1cc_map_strPeak wavelength in natural logarithm of Lya broad componentcharw2cc_mapLine dispersion in natural logarithm of Lya broad componentintw2cc_map_strPeak flux of Lya narrow componentcharw4cc_mapPeak flux of CIV broad componentintw4cc_map_strPeak wavelength in natural logarithm of C IV broad componentcharbest_use_cntrLine dispersion in natural logarithm of C IV broad componentlongngrpPeak flux of C IV narrow componentintw1fluxPeak wavelength in natural logarithm of C IV narrow componentdoublew1sigfluxLine dispersion in natural logarithm of CIV narrow componentdoublew1sigskPeak wavelength in natural logarithm of the first C III broad componentdoublew1confLine dispersion in natural logarithm of the first C III broad componentdoublew2fluxPeak flux of the second C III broad componentdoublew2sigfluxPeak wavelength in natural logarithm of the second C III broad componentdoublew2skyPeak flux of the first C III narrow componentdoublew2sigskPeak wavelength in natural logarithm of the first C III narrow componentdoublew2confLine dispersion in natural logarithm of the first C III narrow componentdoublew3fluxPeak flux of the second C III narrow componentdoublew3sigfluxPeak wavelength in natural logarithm of the second C III narrow componentdoublew3sigskPeak flux of Mg II broad componentdoublew3confPeak wavelength in natural logarithm of Mg II broad componentdoublew4sigfluxPeak flux of the first Mg II narrow componentdoublew4skyPeak wavelength in natural logarithm of the first Mg II narrow componentdoublew4sigskLine dispersion in natural logarithm of the first Mg II narrow componentdoublew4confPeak flux of the second Mg II narrow componentdoublew1magPeak wavelength in natural logarithm of the second Mg II narrow componentdoublew1sigmLine dispersion in natural logarithm of the second Mg II narrow componentdoublew1flgPeak flux of Hbeta broad componentintw1mcorPeak wavelength in natural logarithm of Hbeta broad componentdoublew2sigmPeak flux of Hbeta narrow componentdoublew2flgPeak wavelength in natural logarithm of Hbeta narrow componentintw2mcorLine dispersion in natural logarithm of Hbeta narrow componentdoublew3magPeak flux of [O III] 4959doublew3sigmPeak wavelength in natural logarithm of [O III] 4959doublew3flgLine dispersion in natural logarithm of [O III] 4959intw4magPeak wavelength in natural logarithm of [O III] 5007doublew4flgPeak flux of the first Halpha broad componentintw4mcorPeak wavelength in natural logarithm of the first Halpha broad componentdoublew2mag_1Line dispersion in natural logarithm of the second Halpha broad componentdoublew2sigm_1Peak flux of Halpha broad componentdoublew2flg_1Peak wavelength in natural logarithm of the third Halpha broad componentintw3mag_1Line dispersion in natural logarithm of the third Halpha broad componentdoublew3sigm_1Peak flux of Halpha narrow componentdoublew3flg_1Peak wavelength in natural logarithm of Halpha narrow componentintw4flg_1Peak wavelength in natural logarithm of [N II] 6549intw2sigm_2Peak flux of [S II] 6718doublew2flg_2Peak wavelength in natural logarithm of [S II] 6718intw3mag_2Line dispersion in natural logarithm of [S II] 6718doublew3flg_2Peak wavelength in natural logarithm of [S II] 6732intw4mag_2Line dispersion in natural logarithm of [S II] 6732doublew4flg_2Line dispersion of entire Lyaintw1mag_3EW of entire Lyadoublew1flg_3Integrated Flux of entire Lyaintw3sigm_3Integrated Flux of entire C IVdoublew3flg_3FWHM of entire C IIIintw4sigm_3EW of entire C IIIdoublew4flg_3Peak wavelenth of entire C IIIintw1sigm_4FWHM of entire Mg IIdoublew1flg_4Line dispersion of entire Mg IIintw2sigm_4Peak wavelenth of entire Mg IIdoublew2flg_4Integrated Flux of entire Mg IIintw3mag_4FWHM of entire Hbetadoublew3sigm_4Line dispersion of entire Hbetadoublew3flg_4EW of entire Hbetaintw4sigm_4Integrated Flux of entire Hbetadoublew4flg_4FWHM of entire Halphaintw1flg_5Peak wavelenth of entire Halphaintw2sigm_5Minimal chi-square in the fitting of the first group linesdoublew2flg_5Peak flux of [O III] 5007intw3sigm_5Peak flux of [S II] 6732doublew3flg_5Line dispersion in natural logarithm of [O III] 4959intw1mag_6Peak flux of the first Halpha broad componentdoublew1sigm_6Line dispersion of entire Lyadoublew1flg_6Slope of AGN power lawintw2sigm_6Wavelength shift of Fe II spectrum in optical banddoublew3mag_6Line dispersion in natural logarithm of Mg II broad componentdoublew3sigm_6Peak flux of the second Halpha broad componentdoublew4mag_6The name of the fifth group of spectral linesdoublew4sigm_6Reduced chi-square in the fitting of the fifth group linesdoublew4flg_6Peak wavelength in natural logarithm of the first C III narrow componentintw1mag_7Line dispersion of entire Mg IIdoublew1sigm_7FWHM of entire Lyadoublew1flg_7Peak wavelenth of entire C IIIintw2sigm_7Peak flux of [N II] 6549doublew2flg_7The name of the first group of spectral linesintw3mag_7Minimal chi-square in the fitting of the fifth group linesdoublew3sigm_7Peak wavelength in natural logarithm of [N II] 6585doublew4flg_7Line dispersion in natural logarithm of the first C III broad componentintw1mag_8Peak wavelenth of entire Hbetadoublew2mag_8Line dispersion in natural logarithm of the first Halpha broad componentdoublew2sigm_8Continuum luminosity in common logarithm at rest-frame 1350 Ådoublew2flg_8Degree of freedom in the fitting of the third group linesintw3mag_8The coefficient of the first term of the third-order polynomial in the continuum fittingdoublew3sigm_8Peak flux of the second C III narrow componentdoublew3flg_8FWHM of entire Halphaintw4sigm_8Minimal chi-square in the fitting of the second group linesdoublew1mlqReduced chi-square in the fitting of the first group linesdoublew1mjdminThe fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublew2magpLine dispersion in natural logarithm of [O III] 5007doublew2sigp1Peak wavelength in natural logarithm of Halpha narrow componentdoublew2kPeak flux of C IV narrow componentdoublew2mlqLine dispersion in natural logarithm of the second Halpha broad componentdoublew2mjdminFWHM of entire C IVdoublew3magpPeak flux of the first C III broad componentdoublew3sigp2Minimal chi-square in the fitting of the fourth group linesdoublew3kPeak flux of [N II] 6585doublew3ndfPeak wavelength in natural logarithm of [O III] 5007intw3mlqPeak flux of the first Mg II narrow componentdoublew3mjdminFWHM of entire C IIIdoublew3mjdmaxLine dispersion in natural logarithm of the third Halpha broad componentdoublew4sigp1EW of entire Halphadoublew4sigp2Integrated Flux of entire C IVdoublew4kFWHM of entire Hbetadoublew4ndfLine dispersion in natural logarithm of Hbeta broad componentintw4mjdminPeak wavelength in natural logarithm of [S II] 6732doublew4mjdmaxWavelength shift of Fe II spectrum in UV banddoublew4mjdmeanRest-frame FWHM of Fe II spectrum in optical banddoublerho12Peak wavelength in natural logarithm of Lya narrow componentintrho23Integrated Flux of entire Halphaintrho34Reduced chi-square in the fitting of the third group linesintq23Peak wavelength in natural logarithm of [N II] 6549intq34Peak flux of Lya broad componentintxscproxEW of entire Lyadoublew1rsemiDegree of freedom in the fitting of the first group linesdoublew1baPeak flux of the first C III narrow componentdoublew1paPeak wavelength in natural logarithm of the second Mg II narrow componentdoublew1gmagLine dispersion in natural logarithm of Lya narrow componentdoublew1gerrPeak flux of [O III] 4959doublew1gflgDegree of freedom in the fitting of the fifth group linesintw2rsemidoublew2badoublew2pafile save pathdoublew2gmagFITS filenamedoublew2gerrdoublew2gflgintw3rsemidoublew3badoublew3padoublew3gmagdoublew3gerrdoublew3gflgintw4rsemidoublew4badoublew4padoublew4gmagdoublew4gerrdoublew4gflginttmass_keyintr_2massdoublepa_2massdoublen_2massintj_m_2massdoublej_msig_2massdoubleh_m_2massdoubleh_msig_2massdoublek_m_2massdoublek_msig_2massdoublexdoubleydoublezdoublespt_indinthtm20longxxchardistance_degreedoublew2mproThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublesigpmdecDegree of freedom in the fitting of the first group linesintra_pmThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublerchi2Heliocentric radial velocity obtained by the LASPdoublenaAlpha element abundance estimated by the LASPintw2rchi2_pmThe fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublesigpmraMinimal chi-square in the fitting of the first group linesintw3mproRight ascension from input catalog (degree)doubleglatS/N of i filterdoublewxStellar spectral typedoublesigraFiber pointing declination (degree)doublelamost_drUnique spectrum ID for each observation of each targetintw3mcorPeak flux of [O III] 5007doublew2mag_2Line dispersion in natural logarithm of [N II] 6585doublew1sigp2Integrated Flux of entire C IIIdoublew4sigm_7Peak wavelength in natural logarithm of the first C III broad componentdoublew3mag_3Peak wavelenth of entire C IVdoublew2mag_6Peak wavelength in natural logarithm of the second C III broad componentdoublew2mjdmaxLine dispersion in natural logarithm of the first C III narrow componentdoublew1sigm_1Peak flux of the second Halpha broad componentdoublew4mag_7Line dispersion of entire C IIIdoublew2mag_3FWHM of entire C IVdoublew1sigp1Line dispersion in natural logarithm of CIV narrow componentdoublew2sigm_3Line dispersion of entire C IVdoublew4satThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublew1sigm_5EW of entire Halphadoublew3mjdmeanNormalization parameter of Fe II spectrum in UV banddoublew1magpThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prodoublew1mag_1Line dispersion in natural logarithm of the first Halpha broad componentdoublew2ndfThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intw2flg_6The fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intvar_flgDegree of freedom in the fitting of the third group linescharw1sigm_8Peak wavelength in natural logarithm of the first Halpha broad componentdoublew2mjdmeanPeak wavelength in natural logarithm of the second Halpha broad componentdoublew1mag_5Line dispersion of entire Halphadoublew1kPeak wavelength in natural logarithm of the third Halpha broad componentdoubleq12Peak flux of Halpha narrow componentintw4mag_8Line dispersion in natural logarithm of Halpha narrow componentdoublew1sigm_2Peak flux of [N II] 6585doublew1flg_1Peak wavelength in natural logarithm of the second Halpha broad componentintw4sigm_1Peak flux of [N II] 6549doublew3flg_6Line dispersion in natural logarithm of Hbeta narrow componentintw2flg_3EW of entire C IVintw2sigp2Continuum luminosity in common logarithm at rest-frame 5100 Ådoublew1sigm_3Peak wavelenth of entire Lyadoublew1mag_2Line dispersion in natural logarithm of [N II] 6549doublew4sigm_5Line dispersion in natural logarithm of Lya broad componentdoublew3sigm_2Peak flux of [S II] 6732doublew3sigp1Peak wavelenth of entire Lyadoublew4magpFWHM of entire Mg IIdoublew4sigm_2FWHM of entire Lyadoublew1mjdmeanLine dispersion in natural logarithm of the first Mg II narrow componentdoublew2mag_4EW of entire Mg IIdoublew2covMinimal chi-square in the fitting of the sixth group linesdoublew2mag_7Minimal chi-square in the fitting of the third group linesdoublew4flg_5Minimal chi-square in the fitting of the sixth group linesintw1mjdmaxDegree of freedom in the fitting of the sixth group linesdoublew4mag_5Line dispersion in natural logarithm of [N II] 6549doublew4sigmLine dispersion in natural logarithm of [O III] 5007doublew4mlqLine dispersion in natural logarithm of [N II] 6585doublew2mag_5Integrated Flux of entire Halphadoublew2magLine dispersion in natural logarithm of Hbeta broad componentdoublew4flg_8Normalization parameter of AGN power lawintw1ndfThe coefficient of the cubic term of the third-order polynomial in the continuum fittingintw3flg_7Reduced chi-square in the fitting of the second group linesintw1flg_2Peak wavelength in natural logarithm of [N II] 6585intw1flg_8Peak wavelength in natural logarithm of [S II] 6718intw1mag_4Integrated Flux of entire C IIIdoublew4mag_4Peak wavelenth of entire Hbetadoublew3mag_5Continuum S/Ndoublew1skyPeak flux of the first C III broad componentdoublew3cc_mapPeak wavelength in natural logarithm of Lya narrow componentintw4snrSurface gravity uncertainty obtained by the LASPdoublew3skyLine dispersion in natural logarithm of the second CIII narrow componentdoublew3rchi2Effective temperature obtained by the LASPdoublecoadd_idPan-STARRS g band magnitudecharlamost_raTarget designationpos.eq.radoubleelatSpectral typedoublepmraThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prointw1covThe fitting status of the sixth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublew4mag_3Line dispersion of entire C IIIdoublecc_flagsThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.charw1mproPan-STARRS i band magnitudedoublew1snrPan-STARRS y band magnitudedoublew4mThe name of the sixth group of spectral linesintw2mThe fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intw1mDegree of freedom in the fitting of the fourth group linesintsigra_pmContinuum luminosity in common logarithm at rest-frame 3000 Ådoublelamost_versionUnique source identifier calculated with the "ura" and "udec" in table 9doublew1sigmproPan-STARRS z band magnitudedoublew4sigmproSurface gravity obtained by the LASPdoublew1nmReduced chi-square in the fitting of the fourth group linesintw3sigmproDeclination from input catalog (degree)doublelamost_obsidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.meta.idintw4mag_1Line dispersion in natural logarithm of Halpha narrow componentdoublew3cc_map_strLine dispersion in natural logarithm of Lya narrow componentcharw4fluxLine dispersion in natural logarithm of Mg II broad componentdoublew3mReduced chi-square in the fitting of the fifth group linesintw2rchi2If the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublew2sigmproFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]doublew4mproEffective temperature uncertainty obtained by the LASPdoublexmatch_obs.gaiadr3lamost_ra_obsLocal modified Julian daydoublelamost_dec_obsModified Julian daydoublesolution_idPlan namelongdesignationSpectrograph IDcharsource_idFiber IDlongcxFiber pointing right ascension (degree)doublecyFiber pointing declination (degree)doublehtmidS/N of g filterlongra_j2000S/N of r filterdoubledec_j2000S/N of i filterdoublepmra_j2000S/N of z filterdoublepx_j2000Stellar spectral typedoublerv_j2000Redshiftdoublecy_j2000The objID in the Pan-STARRS catalogdoublecz_j2000Pan-STARRS g band magnitudedoublera_j2015Pan-STARRS i band magnitudedoubledec_j2015Pan-STARRS z band magnitudedoublepmra_j2015Pan-STARRS y band magnitudedoublepmdec_j2015The "source_id" field of Gaia DR3 catalogdoublepx_j2015The "phot_g_mean_mag" field of Gaia DR3 catalogdoublecx_j2015Whether there is a fiber offset during observationdoublera_j2015_5Spectral sub-types of white dwarf starsdoublepmdec_j2015_5Surface gravity obtained by the LASPdoublepx_j2015_5Surface gravity uncertainty obtained by the LASPdoublecx_j2015_5Heliocentric radial velocity obtained by the LASPdoublecz_j2015_5Alpha element abundance estimated by the LASPdoublehtmid_j2015_5The uncertainty of alpha_mlongref_epochOptical depth at the Balmer edge of 3646 Åintra_errorThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublelamost_dec_2The coefficient of the cubic term of the third-order polynomial in the continuum fittingdoubledec_errorContinuum luminosity in common logarithm at rest-frame 1350 ÅdoublepmThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prodoublepmra_errorReduced chi-square in the fitting of the first group linesdoublepmdecDegree of freedom in the fitting of the first group linesdoublera_dec_corrThe fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublera_parallax_corrMinimal chi-square in the fitting of the second group linesdoublera_pmra_corrReduced chi-square in the fitting of the second group linesdoublera_pmdec_corrDegree of freedom in the fitting of the second group linesdoubledec_pmra_corrThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleastrometric_n_obs_acMinimal chi-square in the fitting of the fourth group linesintastrometric_gof_alThe name of the fifth group of spectral linesdoublenu_eff_used_in_astrometryThe fitting status of the sixth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublepseudocolourMinimal chi-square in the fitting of the sixth group linesdoublepseudocolour_errorReduced chi-square in the fitting of the sixth group linesdoublera_pseudocolour_corrDegree of freedom in the fitting of the sixth group linesdoubledec_pseudocolour_corrPeak flux of Lya broad componentdoubleastrometric_matched_transitsPeak wavelength in natural logarithm of Lya narrow componentintvisibility_periods_usedLine dispersion in natural logarithm of Lya narrow componentintastrometric_sigma5d_maxPeak flux of CIV broad componentdoublematched_transitsPeak wavelength in natural logarithm of C IV broad componentintipd_gof_harmonic_amplitudePeak wavelength in natural logarithm of C IV narrow componentdoubleipd_gof_harmonic_phaseLine dispersion in natural logarithm of CIV narrow componentdoubleipd_frac_multi_peakPeak flux of the first C III broad componentintipd_frac_odd_winPeak wavelength in natural logarithm of the first C III broad componentintruweLine dispersion in natural logarithm of the first C III broad componentdoublescan_direction_strength_k1Peak flux of the second C III broad componentdoublescan_direction_strength_k2Peak wavelength in natural logarithm of the second C III broad componentdoublescan_direction_strength_k3Peak flux of the first C III narrow componentdoublescan_direction_strength_k4Peak wavelength in natural logarithm of the first C III narrow componentdoublescan_direction_mean_k2Peak flux of the second C III narrow componentdoublescan_direction_mean_k3Peak wavelength in natural logarithm of the second C III narrow componentdoubleduplicated_sourcePeak flux of Mg II broad componentbooleanphot_g_n_obsPeak wavelength in natural logarithm of Mg II broad componentintphot_g_mean_flux_errorPeak flux of the first Mg II narrow componentdoublephot_g_mean_flux_over_errorPeak wavelength in natural logarithm of the first Mg II narrow componentdoublephot_g_mean_magLine dispersion in natural logarithm of the first Mg II narrow componentdoublephot_bp_mean_fluxPeak wavelength in natural logarithm of the second Mg II narrow componentdoublephot_bp_mean_flux_errorLine dispersion in natural logarithm of the second Mg II narrow componentdoublephot_bp_mean_magPeak wavelength in natural logarithm of Hbeta broad componentdoublephot_rp_n_obsLine dispersion in natural logarithm of Hbeta broad componentintphot_rp_mean_fluxPeak flux of Hbeta narrow componentdoublephot_rp_mean_magPeak flux of [O III] 4959doublephot_bp_rp_excess_factorPeak wavelength in natural logarithm of [O III] 4959doublephot_bp_n_contaminated_transitsLine dispersion in natural logarithm of [O III] 4959intphot_rp_n_contaminated_transitsPeak wavelength in natural logarithm of [O III] 5007intphot_proc_modePeak flux of the first Halpha broad componentintg_rpPeak flux of the second Halpha broad componentdoubleradial_velocityPeak wavelength in natural logarithm of the second Halpha broad componentdoubleradial_velocity_errorLine dispersion in natural logarithm of the second Halpha broad componentdoublerv_method_usedPeak flux of Halpha broad componentintrv_nb_deblended_transitsLine dispersion in natural logarithm of the third Halpha broad componentintrv_visibility_periods_usedPeak flux of Halpha narrow componentintrv_expected_sig_to_noisePeak wavelength in natural logarithm of Halpha narrow componentdoublerv_chisq_pvaluePeak flux of [N II] 6549doublerv_template_teffPeak flux of [N II] 6585intrv_template_loggPeak wavelength in natural logarithm of [N II] 6585doublerv_template_fe_hLine dispersion in natural logarithm of [N II] 6585doublerv_atm_param_originPeak flux of [S II] 6718intvbroadPeak wavelength in natural logarithm of [S II] 6718doublevbroad_nb_transitsPeak flux of [S II] 6732intgrvs_mag_errorLine dispersion in natural logarithm of [S II] 6732doublervs_spec_sig_to_noiseLine dispersion of entire LyadoublebIntegrated Flux of entire Lyadoubleecl_latLine dispersion of entire C IVdoublein_qso_candidatesEW of entire C IVbooleanin_galaxy_candidatesPeak wavelenth of entire C IVbooleannon_single_starIntegrated Flux of entire C IVinthas_xp_continuousFWHM of entire C IIIbooleanhas_xp_sampledLine dispersion of entire C IIIbooleanhas_rvsEW of entire C IIIbooleanhas_epoch_rvIntegrated Flux of entire C IIIbooleanhas_mcmc_mscLine dispersion of entire Mg IIbooleanclassprob_dsc_combmod_quasarPeak wavelenth of entire Mg IIdoubleclassprob_dsc_combmod_galaxyIntegrated Flux of entire Mg IIdoubleclassprob_dsc_combmod_starFWHM of entire Hbetadoubleteff_gspphotLine dispersion of entire Hbetadoubleteff_gspphot_lowerEW of entire Hbetadoubleteff_gspphot_upperPeak wavelenth of entire Hbetadoublelogg_gspphotIntegrated Flux of entire Hbetadoublelogg_gspphot_upperLine dispersion of entire Halphadoublemh_gspphotEW of entire Halphadoublemh_gspphot_lowerPeak wavelenth of entire Halphadoublemh_gspphot_upperIntegrated Flux of entire Halphadoubledistance_gspphotMinimal chi-square in the fitting of the first group linesdoubledistance_gspphot_lowerPeak flux of [O III] 5007doubledistance_gspphot_upperContinuum S/Ndoubleazero_gspphot_upperLine dispersion in natural logarithm of [N II] 6549doubleag_gspphotLine dispersion in natural logarithm of Lya broad componentdoubleag_gspphot_lowerMinimal chi-square in the fitting of the sixth group linesdoubleag_gspphot_upperPeak flux of the first Halpha broad componentdoubleebpminrp_gspphotLine dispersion of entire Lyadoubleebpminrp_gspphot_lowerSlope of AGN power lawdoubleebpminrp_gspphot_upperPeak wavelength in natural logarithm of the second C III broad componentdoublelibname_gspphotWavelength shift of Fe II spectrum in optical bandcharhtmid_j2015Declination from input catalog (degree)longrv_j2015Fiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]doublerv_j2015_5Metallicity uncertainty obtained by the LASPdoubleparallax_over_errorThe name of the first group of spectral linesdoublelamost_ra_2The coefficient of the first term of the third-order polynomial in the continuum fittingdoublepmdec_errorThe name of the second group of spectral linesdoublecy_j2015_5Uncertainty of heliocentric radial velocity obtained by the LASPdoublerandom_indexProjected rotation velocity given by the LASPintpmra_j2015_5Effective temperature uncertainty obtained by the LASPdoublehtmid_j2000Pan-STARRS r band magnitudelongpmraMinimal chi-square in the fitting of the first group linesdoublecz_j2015Right ascension from input catalog (degree)doublelamost_decTarget observation datepos.eq.decdoubleczS/N of u filterdoublephot_bp_n_blended_transitsPeak flux of [O III] 5007intbp_rpPeak wavelength in natural logarithm of the first Halpha broad componentdoubleastrometric_excess_noiseMinimal chi-square in the fitting of the fifth group linesdoublepmdec_pseudocolour_corrPeak flux of Lya narrow componentdoublevbroad_errorLine dispersion in natural logarithm of [S II] 6718doubleecl_lonFWHM of entire C IVdoublerv_time_durationPeak wavelength in natural logarithm of [N II] 6549doublebp_gLine dispersion in natural logarithm of the first Halpha broad componentdoubleparallax_pmdec_corrDegree of freedom in the fitting of the third group linesdoubledistance_degreeThe fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublerv_nb_transitsPeak wavelength in natural logarithm of the third Halpha broad componentintlogg_gspphot_lowerFWHM of entire Halphadoublephot_rp_mean_flux_errorPeak wavelength in natural logarithm of Hbeta narrow componentdoublehas_epoch_photometryPeak wavelenth of entire C IIIbooleanastrometric_n_obs_alThe fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intastrometric_n_bad_obs_alDegree of freedom in the fitting of the fourth group linesintlPeak wavelenth of entire Lyadoublehas_mcmc_gspphotFWHM of entire Mg IIbooleanphot_variable_flagEW of entire Lyachargrvs_mag_nb_transitsFWHM of entire Lyaintin_andromeda_surveyEW of entire Mg IIbooleanpmra_pseudocolour_corrLine dispersion in natural logarithm of Lya broad componentdoublerv_renormalised_gofLine dispersion in natural logarithm of Halpha narrow componentdoublephot_rp_n_blended_transitsLine dispersion in natural logarithm of [O III] 5007intazero_gspphot_lowerLine dispersion in natural logarithm of [O III] 4959doublephot_g_mean_fluxLine dispersion in natural logarithm of Mg II broad componentdoubleastrometric_n_good_obs_alReduced chi-square in the fitting of the fourth group linesintgrvs_magPeak wavelength in natural logarithm of [S II] 6732doublephot_bp_mean_flux_over_errorPeak flux of Hbeta broad componentdoubleazero_gspphotPeak flux of [S II] 6732doubleastrometric_params_solvedDegree of freedom in the fitting of the fifth group linesintmatched_transits_removedPeak flux of C IV narrow componentintparallax_pseudocolour_corrPeak wavelength in natural logarithm of Lya broad componentdoubledec_j2015_5Effective temperature obtained by the LASPdoublenew_matched_transitsLine dispersion in natural logarithm of C IV broad componentintpmdec_j2000Spectral typedoublecy_j2015If the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublelamost_versionUnique source identifier calculated with the "ura" and "udec" in table 9doublelamost_drUnique spectrum ID for each observation of each targetintscan_direction_mean_k1Line dispersion in natural logarithm of the first C III narrow componentdoublescan_direction_mean_k4Line dispersion in natural logarithm of the second CIII narrow componentdoubleastrometric_chi2_alThe fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublecx_j2000Redshift uncertaintydoubleparallax_errorContinuum luminosity in common logarithm at rest-frame 5100 Ådoubleastrometric_primary_flagThe name of the sixth group of spectral linesbooleandec_pmdec_corrMinimal chi-square in the fitting of the third group linesdoubledec_parallax_corrThe name of the first group of spectral linesdoubleparallaxContinuum luminosity in common logarithm at rest-frame 3000 Ådoublepmra_pmdec_corrThe name of the fourth group of spectral linesdoubleparallax_pmra_corrReduced chi-square in the fitting of the third group linesdoublelamost_obsidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.meta.idintlamost_raTarget designationpos.eq.radoubleastrometric_excess_noise_sigReduced chi-square in the fitting of the fifth group linesdoublephot_rp_mean_flux_over_errorLine dispersion in natural logarithm of Hbeta narrow componentdoublephot_bp_n_obsPeak flux of the second Mg II narrow componentintrv_amplitude_robustLine dispersion in natural logarithm of [N II] 6549doublexmatch_obs.panstarrsdr1lamost_drUnique spectrum ID for each observation of each targetintlamost_versionUnique source identifier calculated with the "ura" and "udec" in table 9doublelamost_decTarget observation datepos.eq.decdoublelamost_ra_obsLocal modified Julian daydoublelamost_dec_obsModified Julian daydoubleobjidPlan namelongippobjidFiber IDlongsurveyidFiber pointing right ascension (degree)inttessidFiber pointing declination (degree)intprojectionidS/N of u filterintskycellidS/N of g filterintprimarydetectionS/N of i filterintbestdetectionS/N of z filterintprocessingversionStellar spectral typeintgstackdetectidRedshift uncertaintylonggstackimageidThe objID in the Pan-STARRS catalogintrstackdetectidSurface gravity uncertainty obtained by the LASPlongrstackimageidMetallicity uncertainty obtained by the LASPintrraHeliocentric radial velocity obtained by the LASPdoublerdecUncertainty of heliocentric radial velocity obtained by the LASPdoublerdecerrThe uncertainty of alpha_mdoublerpsfmagOptical depth at the Balmer edge of 3646 ÅdoublerapmagThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublerapmagerrThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublerinfoflagContinuum luminosity in common logarithm at rest-frame 5100 Åintrinfoflag2The name of the first group of spectral linesintrinfoflag3The fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prointrnframesMinimal chi-square in the fitting of the first group linesintistackdetectidDegree of freedom in the fitting of the first group lineslongiraThe fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleiraerrReduced chi-square in the fitting of the second group linesdoubleidecerrDegree of freedom in the fitting of the second group linesdoubleiepochThe name of the first group of spectral linesdoubleiapmagReduced chi-square in the fitting of the third group linesdoubleiapmagerrDegree of freedom in the fitting of the third group linesdoubleikronmagThe name of the fourth group of spectral linesdoubleiinfoflag3Degree of freedom in the fitting of the fourth group linesintinframesThe name of the fifth group of spectral linesintzippdetectidThe fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intzstackdetectidMinimal chi-square in the fitting of the fifth group lineslongzraDegree of freedom in the fitting of the fifth group linesdoublezdecThe name of the sixth group of spectral linesdoublezdecerrMinimal chi-square in the fitting of the sixth group linesdoublezepochReduced chi-square in the fitting of the sixth group linesdoublezpsfmagDegree of freedom in the fitting of the sixth group linesdoublezpsfmagerrPeak flux of Lya broad componentdoublezapmagPeak wavelength in natural logarithm of Lya broad componentdoublezkronmagPeak flux of Lya narrow componentdoublezinfoflag2Peak flux of CIV broad componentintzinfoflag3Peak wavelength in natural logarithm of C IV broad componentintystackimageidLine dispersion in natural logarithm of CIV narrow componentintyraPeak flux of the first C III broad componentdoubleydecPeak wavelength in natural logarithm of the first C III broad componentdoubleyraerrLine dispersion in natural logarithm of the first C III broad componentdoubleydecerrPeak flux of the second C III broad componentdoubleyepochPeak wavelength in natural logarithm of the second C III broad componentdoubleypsfmagPeak flux of the first C III narrow componentdoubleypsfmagerrPeak wavelength in natural logarithm of the first C III narrow componentdoubleyapmagLine dispersion in natural logarithm of the first C III narrow componentdoubleyapmagerrPeak flux of the second C III narrow componentdoubleykronmagerrLine dispersion in natural logarithm of the second CIII narrow componentdoubleyinfoflag2Peak wavelength in natural logarithm of Mg II broad componentintynframesPeak flux of the first Mg II narrow componentintrownumPeak wavelength in natural logarithm of the first Mg II narrow componentlongginfoflagDeclination from input catalog (degree)intgapmagFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]doublegpsfmagerrThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublerpsfmagerrThe coefficient of the first term of the third-order polynomial in the continuum fittingdoubleistackimageidThe name of the second group of spectral linesintidecMinimal chi-square in the fitting of the second group linesdoublerepochProjected rotation velocity given by the LASPdoublegnframesEffective temperature uncertainty obtained by the LASPintiippdetectidReduced chi-square in the fitting of the first group linesintgkronmagerrRight ascension from input catalog (degree)doublegippdetectidRedshiftintgpsfmagThe "source_id" field of Gaia DR3 catalogdoublegraPan-STARRS g band magnitudedoublegraerrPan-STARRS i band magnitudedoublegepochPan-STARRS y band magnitudedoubleuniquepspsstidSpectrograph IDlongzinfoflagLine dispersion in natural logarithm of Lya narrow componentintzstackimageidReduced chi-square in the fitting of the fifth group linesintyinfoflagPeak flux of Mg II broad componentintdistance_degreeLine dispersion in natural logarithm of the first Mg II narrow componentdoubleiinfoflagMinimal chi-square in the fitting of the fourth group linesintipsfmagerrMinimal chi-square in the fitting of the third group linesdoublezapmagerrLine dispersion in natural logarithm of Lya broad componentdoubleyinfoflag3Line dispersion in natural logarithm of Mg II broad componentintiinfoflag2Reduced chi-square in the fitting of the fourth group linesintystackdetectidPeak wavelength in natural logarithm of C IV narrow componentlongzkronmagerrPeak wavelength in natural logarithm of Lya narrow componentdoubleginfoflag3Effective temperature obtained by the LASPintznframesLine dispersion in natural logarithm of C IV broad componentintgdecPan-STARRS r band magnitudedoublegkronmagIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubledvoregionidSpectral typeintzraerrThe fitting status of the sixth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleykronmagPeak wavelength in natural logarithm of the second C III narrow componentdoubleyippdetectidPeak flux of C IV narrow componentintikronmagerrThe fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublerandomstackobjidS/N of r filterdoublelamost_raTarget designationpos.eq.radoublegdecerrPan-STARRS z band magnitudedoublerippdetectidSurface gravity obtained by the LASPintrraerrAlpha element abundance estimated by the LASPdoublerkronmagContinuum luminosity in common logarithm at rest-frame 1350 ÅdoublerkronmagerrContinuum luminosity in common logarithm at rest-frame 3000 ÅdoublegapmagerrWhether there is a fiber offset during observationdoubleipsfmagThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleginfoflag2Spectral sub-types of white dwarf starsintlamost_obsidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.meta.idintxmatch_obs.sdssdr14lamost_drUnique spectrum ID for each observation of each targetintlamost_decTarget observation datepos.eq.decdoublelamost_ra_obsLocal modified Julian daydouble"__id__"Plan nameintobjidSpectrograph IDlongfieldS/N of g filterintobjS/N of r filterintflagsThe objID in the Pan-STARRS cataloglongrowcerrPan-STARRS r band magnitudedoublecolcerrPan-STARRS z band magnitudedoublerowcerr_iSurface gravity uncertainty obtained by the LASPdoublerowcerr_zMetallicity uncertainty obtained by the LASPdoublecolc_uHeliocentric radial velocity obtained by the LASPdoublecolc_gUncertainty of heliocentric radial velocity obtained by the LASPdoublecolc_rAlpha element abundance estimated by the LASPdoublecolc_zProjected rotation velocity given by the LASPdoublecolcerr_uOptical depth at the Balmer edge of 3646 Ådoublecolcerr_gThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublesky_gContinuum luminosity in common logarithm at rest-frame 5100 Ådoubleskyivar_uReduced chi-square in the fitting of the first group linesdoublepsfmag_gDegree of freedom in the fitting of the second group linesdoublepsfmag_rThe name of the first group of spectral linesdoublepsfmagerr_uReduced chi-square in the fitting of the third group linesdoublepsfmagerr_gDegree of freedom in the fitting of the third group linesdoublepsfmagerr_zMinimal chi-square in the fitting of the fourth group linesdoublefibermag_uReduced chi-square in the fitting of the fourth group linesdoublefibermag_gDegree of freedom in the fitting of the fourth group linesdoublefibermag_rThe name of the fifth group of spectral linesdoublefibermag_iThe fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublefibermag_zMinimal chi-square in the fitting of the fifth group linesdoublefibermagerr_gDegree of freedom in the fitting of the fifth group linesdoublefibermagerr_rThe name of the sixth group of spectral linesdoublefibermagerr_zMinimal chi-square in the fitting of the sixth group linesdoublefiber2mag_uReduced chi-square in the fitting of the sixth group linesdoublefiber2mag_rPeak flux of Lya broad componentdoublefiber2mag_iPeak wavelength in natural logarithm of Lya broad componentdoublefiber2magerr_uPeak flux of Lya narrow componentdoublefiber2magerr_gPeak wavelength in natural logarithm of Lya narrow componentdoublefiber2magerr_zPeak wavelength in natural logarithm of C IV broad componentdoublepetromag_uLine dispersion in natural logarithm of C IV broad componentdoublepetromag_rPeak wavelength in natural logarithm of C IV narrow componentdoublepetromag_iLine dispersion in natural logarithm of CIV narrow componentdoublepetromag_zPeak flux of the first C III broad componentdoublepetromagerr_uPeak wavelength in natural logarithm of the first C III broad componentdoublepetromagerr_gLine dispersion in natural logarithm of the first C III broad componentdoublepetromagerr_zPeak flux of the first C III narrow componentdoublepsfflux_uPeak wavelength in natural logarithm of the first C III narrow componentdoublepsfflux_gLine dispersion in natural logarithm of the first C III narrow componentdoublepsfflux_rPeak flux of the second C III narrow componentdoublepsfflux_iPeak wavelength in natural logarithm of the second C III narrow componentdoublepsffluxivar_uPeak flux of Mg II broad componentdoublepsffluxivar_gPeak wavelength in natural logarithm of Mg II broad componentdoublepsffluxivar_iPeak flux of the first Mg II narrow componentdoublepsffluxivar_zPeak wavelength in natural logarithm of the first Mg II narrow componentdoublefiberflux_uLine dispersion in natural logarithm of the first Mg II narrow componentdoublefiberflux_zPeak flux of Hbeta broad componentdoublefiberfluxivar_uPeak wavelength in natural logarithm of Hbeta broad componentdoublefiberfluxivar_gLine dispersion in natural logarithm of Hbeta broad componentdoublefiberfluxivar_rPeak flux of Hbeta narrow componentdoublefiberfluxivar_iPeak wavelength in natural logarithm of Hbeta narrow componentdoublefiberfluxivar_zLine dispersion in natural logarithm of Hbeta narrow componentdoublefiber2flux_uPeak flux of [O III] 4959doublefiber2flux_rLine dispersion in natural logarithm of [O III] 4959doublefiber2fluxivar_rPeak wavelength in natural logarithm of the first Halpha broad componentdoublepetroflux_uPeak wavelength in natural logarithm of the second Halpha broad componentdoublepetroflux_gLine dispersion in natural logarithm of the second Halpha broad componentdoublepetroflux_rPeak flux of Halpha broad componentdoublepetroflux_zLine dispersion in natural logarithm of the third Halpha broad componentdoublepetrofluxivar_uPeak flux of Halpha narrow componentdoublepetrofluxivar_gPeak wavelength in natural logarithm of Halpha narrow componentdoublepetrofluxivar_zPeak wavelength in natural logarithm of [N II] 6549doublepetrorad_uLine dispersion in natural logarithm of [N II] 6549doublepetrorad_gPeak flux of [N II] 6585doublepetrorad_rPeak wavelength in natural logarithm of [N II] 6585doublepetroraderr_uPeak wavelength in natural logarithm of [S II] 6718doublepetroraderr_gLine dispersion in natural logarithm of [S II] 6718doublepetroraderr_rPeak flux of [S II] 6732doublepetroraderr_zLine dispersion in natural logarithm of [S II] 6732doublepetror50_gLine dispersion of entire Lyadoublepetror50_rEW of entire Lyadoublepetror50_iPeak wavelenth of entire Lyadoublepetror50_zIntegrated Flux of entire Lyadoublepetror50err_rEW of entire C IVdoublepetror50err_iPeak wavelenth of entire C IVdoublepetror50err_zIntegrated Flux of entire C IVdoublepetror90_uFWHM of entire C IIIdoublepetror90_gLine dispersion of entire C IIIdoublepetror90_rEW of entire C IIIdoublepetror90_iPeak wavelenth of entire C IIIdoublepetror90err_gLine dispersion of entire Mg IIdoublepetror90err_rEW of entire Mg IIdoublepetror90err_iPeak wavelenth of entire Mg IIdoubleq_uFWHM of entire Hbetadoubleq_gLine dispersion of entire Hbetadoubleq_rEW of entire Hbetadoubleq_iPeak wavelenth of entire Hbetadoubleq_zIntegrated Flux of entire Hbetadoubleqerr_uFWHM of entire Halphadoubleqerr_rEW of entire Halphadoubleqerr_zIntegrated Flux of entire Halphadoubleu_gPeak flux of [O III] 5007doubleu_rContinuum S/Ndoubleu_iPeak flux of [S II] 6732doubleu_zLine dispersion in natural logarithm of [O III] 4959doubleuerr_uLine dispersion in natural logarithm of [N II] 6549doubleuerr_gLine dispersion in natural logarithm of Lya broad componentdoubleuerr_rMinimal chi-square in the fitting of the sixth group linesdoubleuerr_iPeak flux of the first Halpha broad componentdoubleuerr_zLine dispersion of entire Lyadoubleme1_uSlope of AGN power lawdoubleme1_iThe fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleme1_zLine dispersion in natural logarithm of Mg II broad componentdoubleme2_uPeak flux of the second Halpha broad componentdoubleme1e1err_uLine dispersion of entire Mg IIdoubleme1e1err_gFWHM of entire Lyadoubleme1e1err_rPeak wavelenth of entire C IIIdoubleme1e1err_iMinimal chi-square in the fitting of the third group linesdoubleme1e2err_uThe name of the first group of spectral linesdoubleme1e2err_gMinimal chi-square in the fitting of the fifth group linesdoubleme1e2err_zLine dispersion of entire C IIIdoubleme2e2err_gLine dispersion in natural logarithm of the first C III broad componentdoubleme2e2err_rPeak wavelenth of entire Hbetadoubleme2e2err_zPeak wavelength in natural logarithm of [S II] 6718doublemrrcc_uLine dispersion in natural logarithm of the first Halpha broad componentdoublemrrccerr_uFWHM of entire Halphadoublemrrccerr_iNormalization parameter of AGN power lawdoublemcr4_uLine dispersion in natural logarithm of CIV narrow componentdoublemcr4_iThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublemcr4_zReduced chi-square in the fitting of the first group linesdoubleme1psf_uThe fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleme1psf_gDegree of freedom in the fitting of the sixth group linesdoubleme1psf_zPeak wavelength in natural logarithm of Halpha narrow componentdoubleme2psf_uContinuum luminosity in common logarithm at rest-frame 5100 Ådoubleme2psf_gPeak flux of C IV narrow componentdoubleme2psf_iLine dispersion in natural logarithm of the second Halpha broad componentdoublemrrccpsf_uLine dispersion in natural logarithm of the first C III narrow componentdoublemrrccpsf_rPeak flux of the first C III broad componentdoublemrrccpsf_iPeak wavelenth of entire Lyadoublemcr4psf_uPeak flux of [N II] 6585doublemcr4psf_gPeak wavelength in natural logarithm of [O III] 5007doublemcr4psf_rPeak flux of the first Mg II narrow componentdoublemcr4psf_iFWHM of entire C IIIdoublemcr4psf_zLine dispersion in natural logarithm of the third Halpha broad componentdoubledevrad_uNormalization parameter of Fe II spectrum in UV banddoubledevrad_gFWHM of entire Mg IIdoubledevrad_rEW of entire Halphadoubledevrad_iIntegrated Flux of entire C IVdoubledevrad_zFWHM of entire Hbetadoubledevraderr_uLine dispersion in natural logarithm of Hbeta broad componentdoubledevraderr_gLine dispersion in natural logarithm of [N II] 6585doubledevraderr_rPeak wavelength in natural logarithm of [S II] 6732doubledevraderr_iWavelength shift of Fe II spectrum in UV banddoubledevab_uPeak wavelength in natural logarithm of Lya narrow componentdoubledevab_gIntegrated Flux of entire Halphadoubledevab_rReduced chi-square in the fitting of the third group linesdoubledevab_zPeak wavelength in natural logarithm of [N II] 6549doubledevaberr_gEW of entire Lyadoubledevaberr_rDegree of freedom in the fitting of the first group linesdoubledevaberr_iPeak flux of the first C III narrow componentdoubledevaberr_zPeak wavelength in natural logarithm of the second Mg II narrow componentdoubledevphi_gPeak flux of [O III] 4959doubledevphi_rDegree of freedom in the fitting of the fifth group linesdoubledevphi_idoubledevphi_zdoubledevmag_rdoubledevmag_idoubledevmag_zdoubledevmagerr_udoubledevmagerr_gdoubledevmagerr_rdoubledevmagerr_idoubledevmagerr_zdoubledevflux_udoubledevflux_gdoubledevflux_rdoubledevflux_idoubledevflux_zdoubledevfluxivar_udoubledevfluxivar_gdoubledevfluxivar_rdoubledevfluxivar_idoubledevfluxivar_zdoubleexprad_udoubleexprad_gdoubleexprad_rdoubleexprad_idoubleexprad_zdoubleexpraderr_udoubleexpraderr_gdoubleexpraderr_rdoubleexpraderr_idoubleexpraderr_zdoubleexpab_udoubleexpab_gdoubleexpab_rdoubleexpab_idoubleexpab_zdoubleexpaberr_udoubleexpaberr_gdoubleexpaberr_rdoubleexpaberr_idoubleexpaberr_zdoubleexpphi_udoubleexpphi_gdoubleexpphi_rdoubleexpphi_idoubleexpphi_zdoubleexpmag_udoubleexpmag_gdoubleexpmag_rdoubleexpmag_idoubleexpmag_zdoubleexpmagerr_udoubleexpmagerr_gdoubleexpmagerr_rdoubleexpmagerr_idoubleexpmagerr_zdoublemodelmag_udoublemodelmag_gdoublemodelmag_rdoublemodelmag_idoublemodelmag_zdoublemodelmagerr_udoublemodelmagerr_gdoublemodelmagerr_rdoublemodelmagerr_idoublemodelmagerr_zdoublecmodelmag_udoublecmodelmag_gdoublecmodelmag_rdoublecmodelmag_idoublecmodelmag_zdoublecmodelmagerr_udoublecmodelmagerr_gdoublecmodelmagerr_rdoublecmodelmagerr_idoublecmodelmagerr_zdoubleexpflux_udoubleexpflux_gdoubleexpflux_rdoubleexpflux_idoubleexpflux_zdoubleexpfluxivar_udoubleexpfluxivar_gdoubleexpfluxivar_rdoubleexpfluxivar_idoubleexpfluxivar_zdoublemodelflux_udoublemodelflux_gdoublemodelflux_rdoublemodelflux_idoublemodelflux_zdoublemodelfluxivar_udoublemodelfluxivar_gdoublemodelfluxivar_rdoublemodelfluxivar_idoublemodelfluxivar_zdoublecmodelflux_udoublecmodelflux_gdoublecmodelflux_rdoublecmodelflux_idoublecmodelflux_zdoublecmodelfluxivar_udoublecmodelfluxivar_gdoublecmodelfluxivar_rdoublecmodelfluxivar_idoublecmodelfluxivar_zdoubleaperflux7_udoubleaperflux7_gdoubleaperflux7_rdoubleaperflux7_idoubleaperflux7_zdoubleaperflux7ivar_udoubleaperflux7ivar_gdoubleaperflux7ivar_rdoubleaperflux7ivar_idoubleaperflux7ivar_zdoublelnlstar_udoublelnlstar_gdoublelnlstar_rdoublelnlstar_idoublelnlstar_zdoublelnlexp_udoublelnlexp_gdoublelnlexp_rdoublelnlexp_idoublelnlexp_zdoublelnldev_udoublelnldev_gdoublelnldev_rdoublelnldev_idoublelnldev_zdoublefracdev_udoublefracdev_gdoublefracdev_rdoublefracdev_idoublefracdev_zdoubleflags_ulongflags_glongflags_rlongflags_ilongflags_zlongtype_uinttype_ginttype_rinttype_iinttype_zintprobpsf_udoubleprobpsf_gdoubleprobpsf_rdoubleprobpsf_idoubleprobpsf_zdoublelamost_ra_2doublelamost_dec_2doublecxdoublecydoubleczdoubleraerrdoubledecerrdoublebdoubleldoubleoffsetra_udoubleoffsetra_gdoubleoffsetra_rdoubleoffsetra_idoubleoffsetra_zdoubleoffsetdec_udoubleoffsetdec_gdoubleoffsetdec_rdoubleoffsetdec_idoubleoffsetdec_zdoubleextinction_udoubleextinction_gdoubleextinction_rdoubleextinction_idoubleextinction_zdoublepsffwhm_udoublepsffwhm_gdoublepsffwhm_rdoublepsffwhm_idoublepsffwhm_zdoublemjdintairmass_udoubleairmass_gdoubleairmass_rdoubleairmass_idoubleairmass_zdoublephioffset_udoublephioffset_gdoublephioffset_rdoublephioffset_idoublephioffset_zdoublenprof_uintnprof_gintnprof_rintnprof_iintnprof_zintloadversioninthtmidlongfieldidlongparentidlongspecobjidlongudoublegdoublerdoubleidoublezdoubleerr_udoubleerr_gdoubleerr_rdoubleerr_idoubleerr_zdoubledered_udoubledered_gdoubledered_rdoubledered_idoubledered_zdoublecloudcam_uintcloudcam_gintcloudcam_rintcloudcam_iintcloudcam_zintresolvestatusintthingidintbalkanidintnobserveintndetectintnedgeintscoredoublecalibstatus_uintcalibstatus_gintcalibstatus_rintcalibstatus_iintcalibstatus_zintnmgypercount_udoublenmgypercount_gdoublenmgypercount_rdoublenmgypercount_idoublenmgypercount_zdoubletai_udoubletai_gdoubletai_rdoubletai_idoubletai_zdoubledistance_degreecharrerunFiber pointing declination (degree)intcolverrFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]doublecolvThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublecolcerr_zContinuum luminosity in common logarithm at rest-frame 1350 Ådoublesky_uContinuum luminosity in common logarithm at rest-frame 3000 Ådoubleskyivar_gDegree of freedom in the fitting of the first group linesdoublecolcerr_rThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoubleskyivar_zMinimal chi-square in the fitting of the second group linesdoublecolc_iThe uncertainty of alpha_mdoublerowcerr_uEffective temperature obtained by the LASPdoublerowcerr_gEffective temperature uncertainty obtained by the LASPdoublecolcPan-STARRS i band magnitudedoublerowvPan-STARRS y band magnitudedoublelamost_dec_obsModified Julian daydoublerowc_uWhether there is a fiber offset during observationdoublerowc_gIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublesky_iThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prodoublerunFiber pointing right ascension (degree)intmodeS/N of i filterintcleanStellar spectral typeintrowc_iDeclination from input catalog (degree)doublerowc_zSpectral sub-types of white dwarf starsdoublerowverrThe "source_id" field of Gaia DR3 catalogdoublenchildS/N of z filterintlamost_versionUnique source identifier calculated with the "ura" and "udec" in table 9doublefiber2flux_iPeak flux of [O III] 5007doublefiberflux_gPeak flux of the second Mg II narrow componentdoublepetrorad_iLine dispersion in natural logarithm of [N II] 6585doublefiber2magerr_iPeak flux of CIV broad componentdoublefiber2mag_gDegree of freedom in the fitting of the sixth group linesdoublemcr4_gIntegrated Flux of entire C IIIdoubleme2e2err_uPeak wavelength in natural logarithm of the first C III broad componentdoubleme1_gPeak wavelength in natural logarithm of the second C III broad componentdoubleme2_zPeak wavelength in natural logarithm of the first C III narrow componentdoublemrrcc_zPeak flux of the second C III narrow componentdoublefiber2fluxivar_zPeak flux of the second Halpha broad componentdoublepetror50err_uFWHM of entire C IVdoubleme2psf_zFWHM of entire C IVdoublepetror50err_gLine dispersion of entire C IVdoubledevraderr_zRest-frame FWHM of Fe II spectrum in optical banddoubleme1_rWavelength shift of Fe II spectrum in optical banddoubledevmag_ufile save pathdoublemrrccerr_zThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prodoublefiber2fluxivar_iLine dispersion in natural logarithm of the first Halpha broad componentdoubleme2psf_rThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublepetroflux_iPeak wavelength in natural logarithm of the third Halpha broad componentdoublepsfmagerr_rThe name of the fourth group of spectral linesdoubleme2e2err_iPeak wavelength in natural logarithm of the first Halpha broad componentdoublemrrccpsf_gPeak wavelength in natural logarithm of the second Halpha broad componentdoubleqerr_gLine dispersion of entire Halphadoublemcr4_rPeak wavelength in natural logarithm of the third Halpha broad componentdoublesky_rThe name of the first group of spectral linesdoubledevab_iPeak flux of Halpha narrow componentdoublemrrccerr_gLine dispersion in natural logarithm of Halpha narrow componentdoublepetror90err_zIntegrated Flux of entire Mg IIdoublepetrofluxivar_iPeak flux of [N II] 6549doubleme2_gLine dispersion in natural logarithm of Hbeta narrow componentdoubleskyivar_rThe name of the second group of spectral linesdoublepsfmagerr_iThe fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublemrrcc_gContinuum luminosity in common logarithm at rest-frame 1350 Ådoubleqerr_iPeak wavelenth of entire Halphadoubleme2_rThe name of the fifth group of spectral linesdoubledevaberr_uPeak flux of Lya broad componentdoublepetror90err_uFWHM of entire Mg IIdoubledevphi_uLine dispersion in natural logarithm of Lya narrow componentdoublefiber2fluxivar_gPeak flux of the first Halpha broad componentdoublepetrorad_zPeak flux of [S II] 6718doublepetror50_uFWHM of entire Lyadoubleme1psf_rLine dispersion in natural logarithm of the first Mg II narrow componentdoublefiber2mag_zLine dispersion in natural logarithm of Lya broad componentdoubleu_uMinimal chi-square in the fitting of the first group linesdoublemrrccerr_rMinimal chi-square in the fitting of the second group linesdoublemrrccpsf_zMinimal chi-square in the fitting of the fourth group linesdoublepetrofluxivar_rLine dispersion in natural logarithm of Halpha narrow componentdoublemrrcc_rDegree of freedom in the fitting of the third group linesdoubleme1e1err_zPeak flux of [N II] 6549doublefiberflux_rPeak wavelength in natural logarithm of the second Mg II narrow componentdoublefiber2fluxivar_uLine dispersion in natural logarithm of [O III] 5007doubleme1e2err_rPeak wavelength in natural logarithm of [N II] 6585doublefiber2flux_zPeak wavelength in natural logarithm of [O III] 5007doublepsffluxivar_rLine dispersion in natural logarithm of Mg II broad componentdoubleme1psf_iLine dispersion in natural logarithm of [O III] 5007doublepsfmag_uReduced chi-square in the fitting of the second group linesdoublesky_zMinimal chi-square in the fitting of the first group linesdoublemrrcc_iThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublepetroraderr_iPeak wavelength in natural logarithm of [S II] 6732doubleme1e2err_iReduced chi-square in the fitting of the second group linesdoubleme2_iReduced chi-square in the fitting of the fifth group linesdoublepetror90_zIntegrated Flux of entire C IIIdoublefiber2flux_gPeak wavelength in natural logarithm of [O III] 4959doubledevmag_gFITS filenamedoublepetromagerr_rPeak flux of the second C III broad componentdoublepetromag_gPeak flux of C IV narrow componentdoublefiberflux_iLine dispersion in natural logarithm of the second Mg II narrow componentdoublepetromagerr_iPeak wavelength in natural logarithm of the second C III broad componentdoubleprobpsfRedshiftdoublerowc_rRight ascension from input catalog (degree)doublerowcPan-STARRS g band magnitudedoublefibermagerr_iThe fitting status of the sixth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublepsfflux_zLine dispersion in natural logarithm of the second CIII narrow componentdoubleskyivar_iThe fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublecamcolS/N of u filterintinsidemaskRedshift uncertaintyinttypeSpectral typeintrowcerr_rSurface gravity obtained by the LASPdoubleskyversionFiber IDintpsfmag_zMinimal chi-square in the fitting of the third group linesdoublecolcerr_iThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublelamost_raTarget designationpos.eq.radoublepsfmag_iThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublefibermagerr_uReduced chi-square in the fitting of the fifth group linesdoublelamost_obsidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.meta.idintfiber2magerr_rLine dispersion in natural logarithm of Lya narrow componentdoublexmatch_obs.twomassdeclFiber IDpos.eq.decdoubleerr_majFiber pointing right ascension (degree)doubleerr_angS/N of u filterintj_mS/N of r filterdoublej_cmsigS/N of i filterdoublej_msigcomS/N of z filterdoubleh_mStellar spectral typedoubleh_cmsigRedshiftdoubleh_msigcomRedshift uncertaintydoubleh_snrThe objID in the Pan-STARRS catalogdoublek_cmsigPan-STARRS r band magnitudedoublek_msigcomPan-STARRS i band magnitudedoublek_snrPan-STARRS z band magnitudedoubleph_qualPan-STARRS y band magnitudecharrd_flgThe "source_id" field of Gaia DR3 catalogintbl_flgThe "phot_g_mean_mag" field of Gaia DR3 catalogintcc_flgFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charndetWhether there is a fiber offset during observationintpxpaRight ascension from input catalog (degree)intgal_contamSpectral sub-types of white dwarf starsintmp_flgEffective temperature obtained by the LASPintpts_keyEffective temperature uncertainty obtained by the LASPint"date"Surface gravity uncertainty obtained by the LASPcharscanMetallicity uncertainty obtained by the LASPintglonHeliocentric radial velocity obtained by the LASPdoubleglatUncertainty of heliocentric radial velocity obtained by the LASPdoublex_scanAlpha element abundance estimated by the LASPdoubleh_psfchiOptical depth at the Balmer edge of 3646 Ådoublek_psfchiThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublej_msig_stdapThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublek_m_stdapContinuum luminosity in common logarithm at rest-frame 5100 Ådoublek_msig_stdapThe name of the first group of spectral linesdoubledist_edge_nsThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prointdist_edge_flgReduced chi-square in the fitting of the first group linescharuse_srcThe name of the second group of spectral linesintb_m_optDegree of freedom in the fitting of the second group linesdoublevr_m_optThe name of the first group of spectral linesdoublenopt_mchsThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intext_keyMinimal chi-square in the fitting of the third group linesintscan_keyReduced chi-square in the fitting of the third group linesintcoadd_keyDegree of freedom in the fitting of the third group linesintcoaddThe name of the fourth group of spectral linesintdistance_degreeThe fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublelamost_raTarget designationpos.eq.radoubledup_srcDegree of freedom in the fitting of the first group linesintj_m_stdapThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoubledist_optMinimal chi-square in the fitting of the second group linesdoublejdateThe uncertainty of alpha_mdoubleaThe fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.charlamost_dec_obsModified Julian daydoublelamost_decTarget observation datepos.eq.decdoubledist_edge_ewMinimal chi-square in the fitting of the first group linesint"__id__"Plan nameintdesignationS/N of g filtercharerr_minFiber pointing declination (degree)doublelamost_ra_obsLocal modified Julian daydoublelamost_drUnique spectrum ID for each observation of each targetintlamost_ra_2Spectrograph IDdoublelamost_versionUnique source identifier calculated with the "ura" and "udec" in table 9doubleh_msig_stdapContinuum luminosity in common logarithm at rest-frame 3000 Ådoublej_snrSpectral typedoubleproxIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublek_mPan-STARRS g band magnitudedoublehemisSurface gravity obtained by the LASPcharpxcntrDeclination from input catalog (degree)intj_psfchiProjected rotation velocity given by the LASPdoubleh_m_stdapContinuum luminosity in common logarithm at rest-frame 1350 Ådoublephi_optReduced chi-square in the fitting of the second group linesintlamost_obsidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.meta.idintxmatch_obs.usnob1lamost_decTarget observation datepos.eq.decdoublelamost_ra_obsLocal modified Julian daydoubleidPlan namemeta.idintlamost_dec_2Fiber IDdoublefit_raS/N of u filterintfit_sdS/N of g filterintpmsdS/N of i filterinte_pmraS/N of z filterintrhoStellar spectral typeintxRedshift uncertaintyintyThe objID in the Pan-STARRS catalogintpmtotPan-STARRS g band magnitudeintmagoPan-STARRS r band magnitudeintmagePan-STARRS i band magnitudeintmagjPan-STARRS z band magnitudeintmagfPan-STARRS y band magnitudeintmagnThe "source_id" field of Gaia DR3 cataloginttyc1The "phot_g_mean_mag" field of Gaia DR3 cataloginttyc2Fiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]intfilenoIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)intrecnoRight ascension from input catalog (degree)intflagsDeclination from input catalog (degree)intndetSpectral sub-types of white dwarf starsint"zone"Effective temperature obtained by the LASPintepochEffective temperature uncertainty obtained by the LASPintdistance_degreeSurface gravity obtained by the LASPdoubletyc3Whether there is a fiber offset during observationintthetaRedshiftintlamost_ra_2Spectrograph IDdoublelamost_versionUnique source identifier calculated with the "ura" and "udec" in table 9doublee_sdFiber pointing declination (degree)doublelamost_dec_obsModified Julian daydoublee_pmsdSpectral typeintlamost_drUnique spectrum ID for each observation of each targetinte_raFiber pointing right ascension (degree)doublepmraS/N of r filterintlamost_raTarget designationpos.eq.radoublelamost_obsidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.meta.idintpublic"public".astellarsnruS/N of u filterdoublesnrgS/N of g filterdoublesnrrS/N of r filterdoublesnriS/N of i filterdoublesnrzS/N of z filterdoublesubclassStellar spectral typecharzRedshiftdoublez_errRedshift uncertaintydoubleps_idThe objID in the Pan-STARRS cataloglongmag_ps_rPan-STARRS r band magnitudedoublemag_ps_iPan-STARRS i band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublemag_ps_yPan-STARRS y band magnitudedoublegaia_source_idThe "source_id" field of Gaia DR3 catalogchargaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleraRight ascension from input catalog (degree)pos.eq.radoubledecDeclination from input catalog (degree)pos.eq.decdoublekp12Spectral sub-types of white dwarf starsdoublekp18Effective temperature obtained by the LASPdoublehdelta24Surface gravity uncertainty obtained by the LASPdoublehdelta48Metallicity uncertainty obtained by the LASPdoublehgamma12Uncertainty of heliocentric radial velocity obtained by the LASPdoublehgamma48The uncertainty of alpha_mdoublehgamma54Projected rotation velocity given by the LASPdoublehbeta12Optical depth at the Balmer edge of 3646 Ådoublehbeta24The coefficient of the first term of the third-order polynomial in the continuum fittingdoublehbeta60The coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublehalpha12Continuum luminosity in common logarithm at rest-frame 1350 Ådoublehalpha48Continuum luminosity in common logarithm at rest-frame 5100 Ådoublehalpha70The name of the first group of spectral linesdoublepaschen13The fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prodoublepaschen142Minimal chi-square in the fitting of the first group linesdoublehdelta_d02Minimal chi-square in the fitting of the second group linesdoubledec_obsFiber pointing declination (degree)pos.eq.decdoublehalpha_d02Degree of freedom in the fitting of the first group linesdoublehbeta48The coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublehdelta12Surface gravity obtained by the LASPdoublehdelta64Heliocentric radial velocity obtained by the LASPdoublehgamma24Alpha element abundance estimated by the LASPdoublehgamma_d02The fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublemjdModified Julian dayintobsdateTarget observation datetime.epochcharobsidUnique spectrum ID for each observation of each targetmeta.idlongoffsetsWhether there is a fiber offset during observationintpaschen242Reduced chi-square in the fitting of the first group linesdoubleplanidPlan namecharspidSpectrograph IDintlmjdLocal modified Julian dayintmag_ps_gPan-STARRS g band magnitudedoubleuidUnique source identifier calculated with the "ura" and "udec" in table 9chardesignationTarget designationcharfiberidFiber IDintra_obsFiber pointing right ascension (degree)pos.eq.radoubleclassSpectral typecharkp6Effective temperature uncertainty obtained by the LASPdoublehbeta_d02The name of the second group of spectral linesdoublehalpha24Continuum luminosity in common logarithm at rest-frame 3000 Ådoublegp_idFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.long"public".catalogueobsidUnique spectrum ID for each observation of each targetmeta.idlonguidUnique source identifier calculated with the "ura" and "udec" in table 9charobsdateTarget observation datetime.epochcharlmjdLocal modified Julian dayintmjdModified Julian dayintplanidPlan namecharspidSpectrograph IDintfiberidFiber IDintra_obsFiber pointing right ascension (degree)pos.eq.radoubledec_obsFiber pointing declination (degree)pos.eq.decdoublesnruS/N of u filterdoublesnrgS/N of g filterdoublesnrrS/N of r filterdoublesnriS/N of i filterdoublesnrzS/N of z filterdoublesubclassStellar spectral typecharzRedshiftdoublez_errRedshift uncertaintydoubleps_idThe objID in the Pan-STARRS cataloglongmag_ps_gPan-STARRS g band magnitudedoublemag_ps_rPan-STARRS r band magnitudedoublemag_ps_iPan-STARRS i band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublemag_ps_yPan-STARRS y band magnitudedoublegaia_source_idThe "source_id" field of Gaia DR3 catalogchargaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charoffsetsWhether there is a fiber offset during observationintoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleraRight ascension from input catalog (degree)pos.eq.radoubledecDeclination from input catalog (degree)pos.eq.decdoublefibermaskSpectral sub-types of white dwarf starsintwith_norm_fluxEffective temperature obtained by the LASPintclassSpectral typechargp_idFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.longdesignationTarget designationchar"public".combinedobsidUnique spectrum ID for each observation of each targetmeta.idlonguidUnique source identifier calculated with the "ura" and "udec" in table 9charobsdateTarget observation datetime.epochcharlmjdLocal modified Julian dayintmjdModified Julian dayintplanidPlan namecharspidSpectrograph IDintfiberidFiber IDintra_obsFiber pointing right ascension (degree)pos.eq.radoubledec_obsFiber pointing declination (degree)pos.eq.decdoublesnrgS/N of g filterdoublesnrrS/N of r filterdoublemag_ps_iPan-STARRS i band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublelogg_errEffective temperature uncertainty obtained by the LASPdoublefeh_errMetallicity uncertainty obtained by the LASPdoublerv_errUncertainty of heliocentric radial velocity obtained by the LASPdoublealpha_mProjected rotation velocity given by the LASPdoubleloggOptical depth at the Balmer edge of 3646 ÅdoublefehThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublehalpha24The name of the first group of spectral linesdoublehdelta24The name of the second group of spectral linesdoublehgamma54Minimal chi-square in the fitting of the second group linesdoublehbeta24Degree of freedom in the fitting of the second group linesdoublekp18Minimal chi-square in the fitting of the third group linesdoublehbeta48Degree of freedom in the fitting of the third group linesdoublehgamma_d02The fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublepaschen142Reduced chi-square in the fitting of the fourth group linesdoublehdelta64The name of the fifth group of spectral linesdoubletio1_errDegree of freedom in the fitting of the fifth group linesdoubletio5_errThe name of the sixth group of spectral linesdoublecah2Reduced chi-square in the fitting of the sixth group linesdoublecaoh_errDegree of freedom in the fitting of the sixth group linesdoublecah3_errPeak flux of Lya broad componentdoubletypePeak wavelength in natural logarithm of Lya broad componentdoublem_hLine dispersion in natural logarithm of Lya broad componentdoublecaohPeak flux of Lya narrow componentdoubletio5Peak wavelength in natural logarithm of Lya narrow componentdoublecah3Line dispersion in natural logarithm of Lya narrow componentdoublecah2_errPeak flux of CIV broad componentdoublecah1Peak wavelength in natural logarithm of C IV broad componentdoublezetaLine dispersion in natural logarithm of C IV broad componentdoubletio4Peak flux of C IV narrow componentdoubletio3_errPeak wavelength in natural logarithm of the first C III broad componentdoublenaLine dispersion in natural logarithm of the first C III broad componentdoubletio2Peak flux of the second C III broad componentdoublezeta_errPeak wavelength in natural logarithm of the second C III broad componentdoubleabs_gmag_errPeak flux of the first C III narrow componentdoubleperiodPeak wavelength in natural logarithm of the first C III narrow componentdoublerLine dispersion in natural logarithm of the first C III narrow componentintsubtypePeak flux of the second C III narrow componentcharwd_subclassLine dispersion in natural logarithm of the second CIII narrow componentcharhalpha_fluxPeak flux of Mg II broad componentdoublemetal_mwPeak wavelength in natural logarithm of Mg II broad componentdoublesii_6718_ewPeak flux of the first Mg II narrow componentdoublehbeta_ewLine dispersion in natural logarithm of the first Mg II narrow componentdoubleage_mwPeak flux of the second Mg II narrow componentdoublenii_6550_ewPeak wavelength in natural logarithm of the second Mg II narrow componentdoublesii_6718_fluxPeak flux of Hbeta broad componentdoublesii_6733_ewPeak wavelength in natural logarithm of Hbeta broad componentdoubleoiii_5008_fluxLine dispersion in natural logarithm of Hbeta broad componentdoublehalpha_ewPeak flux of Hbeta narrow componentdoublehbeta_fluxPeak wavelength in natural logarithm of Hbeta narrow componentdoubleoiii_5008_ewLine dispersion in natural logarithm of Hbeta narrow componentdoublenii_6585_fluxPeak flux of [O III] 4959doublesii_6733_fluxPeak wavelength in natural logarithm of [O III] 4959doublevsig_errLine dispersion in natural logarithm of [O III] 4959doubleoiii_4960_ewPeak wavelength in natural logarithm of [O III] 5007doublemetal_lwPeak flux of the first Halpha broad componentdoublehb_br_1_peak_wavelengthPeak wavelength in natural logarithm of the second Halpha broad componentdoublefe_op_normPeak flux of Halpha broad componentdoublebalmer_teffLine dispersion in natural logarithm of the third Halpha broad componentintred_chi2_6Peak flux of Halpha narrow componentintndof_2Line dispersion in natural logarithm of Halpha narrow componentintciv_ewPeak wavelength in natural logarithm of [N II] 6549doublelya_areaLine dispersion in natural logarithm of [N II] 6549doubleha_peak_wavelengthPeak flux of [N II] 6585doublebalmer_normLine dispersion in natural logarithm of [N II] 6585doublemgii_br_1_peak_wavelengthPeak flux of [S II] 6718doubleciv_sigmaPeak wavelength in natural logarithm of [S II] 6718doubleciii_na_2_peak_wavelengthLine dispersion in natural logarithm of [S II] 6718intlya_na_1_peak_fluxPeak flux of [S II] 6732doublepoly_bPeak wavelength in natural logarithm of [S II] 6732doublemgii_na_1_peak_wavelengthFWHM of entire Lyadoublehb_ewLine dispersion of entire Lyadoublemgii_areaEW of entire Lyadoubleline_name_2Peak wavelenth of entire Lyacharha_sigmaIntegrated Flux of entire Lyadoublehb_sigmaEW of entire C IVdoubleciii_br_2_peak_fluxPeak wavelenth of entire C IVdoubleciv_na_1_peak_wavelengthIntegrated Flux of entire C IVdoubleline_name_4FWHM of entire C IIIcharmgii_ewEW of entire C IIIdoublehb_na_1_peak_wavelengthPeak wavelenth of entire C IIIdoublelya_br_1_peak_wavelengthFWHM of entire Mg IIdoublel3000Line dispersion of entire Mg IIdoublemgii_na_2_sigmaEW of entire Mg IIdoubleciv_br_1_peak_wavelengthFWHM of entire Hbetadoublemgii_peak_wavelengthLine dispersion of entire Hbetadoubleciii_ewEW of entire Hbetadoubleciv_br_1_peak_fluxIntegrated Flux of entire Hbetadoublehb_areaFWHM of entire Halphadoubleha_br_3_peak_fluxLine dispersion of entire Halphadoublefe_uv_fwhmEW of entire Halphadoubleoiii5007_1_peak_fluxPeak flux of [O III] 5007doublesn_ratio_contiContinuum S/Ndoublesii6732_1_peak_fluxPeak flux of [S II] 6732doubleoiii4959_1_sigmaLine dispersion in natural logarithm of [O III] 4959doublenii6549_1_sigmaLine dispersion in natural logarithm of [N II] 6549doublemin_chi2_6Minimal chi-square in the fitting of the sixth group linesintha_br_1_peak_fluxPeak flux of the first Halpha broad componentdoublelya_sigmaLine dispersion of entire Lyadoublefitting_status_5The fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intline_name_5The name of the fifth group of spectral linescharmgii_sigmaLine dispersion of entire Mg IIdoublemin_chi2_3Minimal chi-square in the fitting of the third group linesdoubleline_name_3The name of the first group of spectral linescharred_chi2_2Reduced chi-square in the fitting of the second group linesdoubleciii_sigmaLine dispersion of entire C IIIdoubleciii_br_1_peak_wavelengthPeak wavelength in natural logarithm of the first C III broad componentdoubleciii_br_1_sigmaLine dispersion in natural logarithm of the first C III broad componentdoublehb_peak_wavelengthPeak wavelenth of entire Hbetadoublesii6718_1_peak_wavelengthPeak wavelength in natural logarithm of [S II] 6718doubleha_br_1_sigmaLine dispersion in natural logarithm of the first Halpha broad componentdoublel1350Continuum luminosity in common logarithm at rest-frame 1350 Ådoubleciii_na_2_peak_fluxPeak flux of the second C III narrow componentintha_fwhmFWHM of entire Halphadoubleha_na_1_sigmaLine dispersion in natural logarithm of Halpha narrow componentdoublepl_normNormalization parameter of AGN power lawdoubleciii_areaIntegrated Flux of entire C IIIdoubleha_br_3_peak_wavelengthPeak wavelength in natural logarithm of the third Halpha broad componentdoublepoly_cThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublendof_6Degree of freedom in the fitting of the sixth group linesintoiii5007_1_sigmaLine dispersion in natural logarithm of [O III] 5007doubleciv_na_1_peak_fluxPeak flux of C IV narrow componentdoublefitting_status_3The fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intha_br_2_sigmaLine dispersion in natural logarithm of the second Halpha broad componentdoubleciv_fwhmFWHM of entire C IVdoubleciii_na_1_sigmaLine dispersion in natural logarithm of the first C III narrow componentintlya_peak_wavelengthPeak wavelenth of entire Lyadoublemin_chi2_4Minimal chi-square in the fitting of the fourth group linesdoublenii6585_1_peak_fluxPeak flux of [N II] 6585doublemgii_na_1_peak_fluxPeak flux of the first Mg II narrow componentdoublefe_uv_normNormalization parameter of Fe II spectrum in UV banddoublemgii_fwhmFWHM of entire Mg IIdoubleha_ewEW of entire Halphadoubleciv_areaIntegrated Flux of entire C IVdoublehb_fwhmFWHM of entire Hbetadoublenii6585_1_sigmaLine dispersion in natural logarithm of [N II] 6585doublefe_op_fwhmRest-frame FWHM of Fe II spectrum in optical banddoublelya_na_1_peak_wavelengthPeak wavelength in natural logarithm of Lya narrow componentdoubleha_areaIntegrated Flux of entire Halphadoublered_chi2_3Reduced chi-square in the fitting of the third group linesdoubleha_na_1_peak_fluxPeak flux of Halpha narrow componentdoublenii6549_1_peak_wavelengthPeak wavelength in natural logarithm of [N II] 6549doublelya_br_1_peak_fluxPeak flux of Lya broad componentdoublelya_ewEW of entire Lyadoublendof_1Degree of freedom in the fitting of the first group linesintciii_na_1_peak_fluxPeak flux of the first C III narrow componentintmgii_na_2_peak_wavelengthPeak wavelength in natural logarithm of the second Mg II narrow componentdoubleoiii4959_1_peak_fluxPeak flux of [O III] 4959doublendof_5Degree of freedom in the fitting of the fifth group linesintgaia_vari_type_soscharfilefile save pathcharspecFITS filenamechardecDeclination from input catalog (degree)pos.eq.decdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]chargaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublehalpha48Continuum luminosity in common logarithm at rest-frame 1350 Ådoublehgamma24Continuum luminosity in common logarithm at rest-frame 3000 Ådoublehalpha70Degree of freedom in the fitting of the first group linesdoublehbeta12The coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublealpha_m_errHeliocentric radial velocity obtained by the LASPdoublervAlpha element abundance estimated by the LASPdoublekp12The fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleoffsetsWhether there is a fiber offset during observationinthdelta_d02The fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prodoublehbeta_d02Reduced chi-square in the fitting of the first group linesdoubleps_idThe objID in the Pan-STARRS cataloglongraRight ascension from input catalog (degree)pos.eq.radoublesnriS/N of i filterdoublesubclassStellar spectral typecharz_errRedshift uncertaintydoublefibermaskSpectral sub-types of white dwarf starsintmag_ps_gPan-STARRS g band magnitudedoublemag_ps_yPan-STARRS y band magnitudedoubleoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublesnrzS/N of z filterdoublewith_norm_fluxEffective temperature obtained by the LASPintzRedshiftdoubleage_lwPeak flux of [O III] 5007doublebalmer_tau_ePeak wavelength in natural logarithm of the first Halpha broad componentdoubleciii_br_1_peak_fluxPeak flux of the first C III broad componentdoubleciii_br_2_peak_wavelengthPeak wavelength in natural logarithm of the second C III broad componentdoubleciii_fwhmFWHM of entire C IIIdoubleciii_na_1_peak_wavelengthPeak wavelength in natural logarithm of the first C III narrow componentintciii_na_2_sigmaPeak flux of the second Halpha broad componentintciii_peak_wavelengthPeak wavelenth of entire C IIIdoubleciv_br_1_sigmaFWHM of entire C IVdoubleciv_na_1_sigmaLine dispersion in natural logarithm of CIV narrow componentdoubleciv_peak_wavelengthLine dispersion of entire C IVdoubleewha_errLine dispersion in natural logarithm of CIV narrow componentdoublefe_op_shiftWavelength shift of Fe II spectrum in optical banddoublefe_uv_shiftWavelength shift of Fe II spectrum in UV banddoublefitting_status_1The fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prointfitting_status_2Line dispersion in natural logarithm of the first Halpha broad componentintfitting_status_4The fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intfitting_status_6Peak wavelength in natural logarithm of the third Halpha broad componentintha_br_1_peak_wavelengthPeak wavelength in natural logarithm of the first Halpha broad componentdoubleha_br_2_peak_fluxPeak flux of the second Halpha broad componentdoubleha_br_2_peak_wavelengthPeak wavelength in natural logarithm of the second Halpha broad componentdoubleha_br_3_sigmaLine dispersion in natural logarithm of the third Halpha broad componentdoublehalpha_d02Continuum luminosity in common logarithm at rest-frame 5100 Ådoubleha_na_1_peak_wavelengthPeak wavelength in natural logarithm of Halpha narrow componentdoublehb_br_1_peak_fluxIntegrated Flux of entire Mg IIdoublehb_br_1_sigmaLine dispersion in natural logarithm of Hbeta broad componentdoublehbeta60The name of the fourth group of spectral linesdoublehb_na_1_peak_fluxPeak flux of [N II] 6549doublehb_na_1_sigmaLine dispersion in natural logarithm of Hbeta narrow componentdoublehdelta12The coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublehgamma48The name of the first group of spectral linesdoublekp6Degree of freedom in the fitting of the fourth group linesdoublel5100Continuum luminosity in common logarithm at rest-frame 5100 Ådoubleline_name_1Peak wavelenth of entire Halphacharline_name_6Peak wavelength in natural logarithm of Halpha narrow componentcharlya_br_1_sigmaLine dispersion in natural logarithm of Lya broad componentdoublelya_fwhmFWHM of entire Lyadoublelya_na_1_sigmaLine dispersion in natural logarithm of Lya narrow componentdoublemgii_br_1_sigmaLine dispersion in natural logarithm of Mg II broad componentdoublemgii_na_1_sigmaLine dispersion in natural logarithm of the first Mg II narrow componentdoublemgii_na_2_peak_fluxPeak wavelenth of entire Mg IIdoublem_h_errMinimal chi-square in the fitting of the sixth group linesdoublemin_chi2_1Minimal chi-square in the fitting of the first group linesdoublemin_chi2_2Minimal chi-square in the fitting of the second group linesdoublemin_chi2_5Minimal chi-square in the fitting of the fifth group linesintndof_3Degree of freedom in the fitting of the third group linesintndof_4Line dispersion in natural logarithm of the second Halpha broad componentintnii6549_1_peak_fluxPeak flux of [N II] 6549doublenii_6550_fluxLine dispersion in natural logarithm of [O III] 5007doublenii6585_1_peak_wavelengthPeak wavelength in natural logarithm of [N II] 6585doubleoiii4959_1_peak_wavelengthIntegrated Flux of entire Halphadoubleoiii_4960_fluxLine dispersion in natural logarithm of Mg II broad componentdoubleoiii5007_1_peak_wavelengthPeak wavelength in natural logarithm of [O III] 5007doublepaschen13Reduced chi-square in the fitting of the second group linesdoublepaschen242Minimal chi-square in the fitting of the first group linesdoublepl_slopeSlope of AGN power lawdoublepoly_aThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublered_chi2_1Reduced chi-square in the fitting of the first group linesdoublered_chi2_4Peak wavelength in natural logarithm of [N II] 6585doublered_chi2_5Reduced chi-square in the fitting of the fifth group linesintsii6718_1_peak_fluxLine dispersion in natural logarithm of [S II] 6732doublesii6732_1_peak_wavelengthPeak wavelength in natural logarithm of [S II] 6732doublesii6732_1_sigmaPeak wavelenth of entire Hbetadoubletio2_errPeak flux of the first C III broad componentdoubletio4_errThe fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublevsini_laspSurface gravity uncertainty obtained by the LASPdoublegaia_source_idThe "source_id" field of Gaia DR3 catalogcharclassSpectral typecharteff_errThe uncertainty of alpha_mdoubletio1The fitting status of the sixth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublesii6718_1_sigmaIntegrated Flux of entire C IIIdoubleabs_gmagPeak wavelength in natural logarithm of the second C III narrow componentdoublemgii_br_1_peak_fluxLine dispersion of entire C IIIdoubletio3Peak wavelength in natural logarithm of C IV narrow componentdoublehalpha12The fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublesnruS/N of u filterdoubledesignationTarget designationcharmag_ps_rPan-STARRS r band magnitudedoubleteffSurface gravity obtained by the LASPdoublehgamma12Minimal chi-square in the fitting of the fourth group linesdoublecah1_errMinimal chi-square in the fitting of the fifth group linesdoubleewhaReduced chi-square in the fitting of the fifth group linesdoublenii_6585_ewPeak wavelength in natural logarithm of the first Mg II narrow componentdoublevsigLine dispersion in natural logarithm of the second Mg II narrow componentdoublehdelta48Reduced chi-square in the fitting of the third group linesdoublegp_idFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.long"public".cvobsidUnique spectrum ID for each observation of each targetmeta.idlonglmjdLocal modified Julian dayintmjdModified Julian dayintplanidPlan namecharspidSpectrograph IDintfiberidFiber IDintsnruS/N of u filterdoublesnrgS/N of g filterdoublesnrrS/N of r filterdoublesnriS/N of i filterdoublesnrzS/N of z filterdoubleps_idThe objID in the Pan-STARRS cataloglongmag_ps_rPan-STARRS r band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublesubtypeSpectral sub-types of white dwarf starscharrEffective temperature uncertainty obtained by the LASPintabs_gmagSurface gravity obtained by the LASPdoubleabs_gmag_errSurface gravity uncertainty obtained by the LASPdoubleclassSpectral typechardecDeclination from input catalog (degree)pos.eq.decdoubledec_obsFiber pointing declination (degree)pos.eq.decdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]chargaia_source_idThe "source_id" field of Gaia DR3 catalogcharmag_ps_iPan-STARRS i band magnitudedoublemag_ps_yPan-STARRS y band magnitudedoubleobsdateTarget observation datetime.epochcharoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleraRight ascension from input catalog (degree)pos.eq.radoublera_obsFiber pointing right ascension (degree)pos.eq.radoubleuidUnique source identifier calculated with the "ura" and "udec" in table 9chardesignationTarget designationchargp_idFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.longperiodEffective temperature obtained by the LASPdoublez_errRedshift uncertaintydoublezRedshiftdoublemag_ps_gPan-STARRS g band magnitudedoublesubclassStellar spectral typechargaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoubleoffsetsWhether there is a fiber offset during observationint"public".galaxyfiberidFiber IDintdec_obsFiber pointing declination (degree)pos.eq.decdoublesnruS/N of u filterdoublesnrgS/N of g filterdoublesnrrS/N of r filterdoublesnriS/N of i filterdoublesnrzS/N of z filterdoublesubclassStellar spectral typecharzRedshiftdoublez_errRedshift uncertaintydoubleps_idThe objID in the Pan-STARRS cataloglongmag_ps_gPan-STARRS g band magnitudedoublemag_ps_rPan-STARRS r band magnitudedoublemag_ps_iPan-STARRS i band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublemag_ps_yPan-STARRS y band magnitudedoublegaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charoffsetsWhether there is a fiber offset during observationintoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleraRight ascension from input catalog (degree)pos.eq.radoubledecDeclination from input catalog (degree)pos.eq.decdoubleoiii_4960_ewSurface gravity obtained by the LASPdoubleoiii_5008_ewMetallicity uncertainty obtained by the LASPdoublenii_6550_fluxHeliocentric radial velocity obtained by the LASPdoublenii_6550_ewUncertainty of heliocentric radial velocity obtained by the LASPdoublehalpha_ewThe uncertainty of alpha_mdoublenii_6585_fluxProjected rotation velocity given by the LASPdoublenii_6585_ewOptical depth at the Balmer edge of 3646 Ådoublesii_6718_fluxThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublesii_6733_fluxThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublesii_6733_ewContinuum luminosity in common logarithm at rest-frame 1350 Ådoubleage_mwContinuum luminosity in common logarithm at rest-frame 5100 Ådoublemetal_lwThe name of the first group of spectral linesdoublevsigMinimal chi-square in the fitting of the first group linesdoubledesignationTarget designationchargaia_source_idThe "source_id" field of Gaia DR3 catalogcharsii_6718_ewThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoubleoiii_5008_fluxSurface gravity uncertainty obtained by the LASPdoublehalpha_fluxAlpha element abundance estimated by the LASPdoubleoiii_4960_fluxEffective temperature uncertainty obtained by the LASPdoublelmjdLocal modified Julian dayintmjdModified Julian dayintobsdateTarget observation datetime.epochcharobsidUnique spectrum ID for each observation of each targetmeta.idlongmetal_mwThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prodoublevsig_errReduced chi-square in the fitting of the first group linesdoubleplanidPlan namecharra_obsFiber pointing right ascension (degree)pos.eq.radoublespidSpectrograph IDintuidUnique source identifier calculated with the "ura" and "udec" in table 9charclassSpectral typecharhbeta_fluxSpectral sub-types of white dwarf starsdoublehbeta_ewEffective temperature obtained by the LASPdoublegp_idFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.longage_lwContinuum luminosity in common logarithm at rest-frame 3000 Ådouble"public".inputcatalogfiberidTarget observation dateintra_obsModified Julian daypos.eq.radoubledec_obsPlan namepos.eq.decdoublemag7S/N of z filterdoubletfromRedshiftcharoffsetsThe objID in the Pan-STARRS cataloginttnamePan-STARRS y band magnitudecharmag2Fiber pointing declination (degree)doublemagtypeFiber IDcharunitidLocal modified Julian daycharraPan-STARRS r band magnitudepos.eq.radoubleepochPan-STARRS z band magnitudecharobsidUnique spectrum ID for each observation of each targetmeta.idlongmag3S/N of u filterdoublemag1Fiber pointing right ascension (degree)doublemag4S/N of g filterdoubleobjtypeSpectrograph IDcharobsdateUnique source identifier calculated with the "ura" and "udec" in table 9time.epochchartsourceSpectral typecharoffsets_vPan-STARRS g band magnitudedoubletcommentRedshift uncertaintycharfibertypeStellar spectral typechardecPan-STARRS i band magnitudepos.eq.decdoublemag6S/N of i filterdoublemag5S/N of r filterdoublespidTarget designationintplanidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.char"public".mecobs_numberTarget observation dateintobsid_listLocal modified Julian daycharmidmjm_listModified Julian daycharz_listPlan namecharteff_listSpectrograph IDcharlogg_listFiber IDcharrv_listFiber pointing declination (degree)chargaia_vari_type_sosS/N of u filtercharuidUnique spectrum ID for each observation of each targetcharuraUnique source identifier calculated with the "ura" and "udec" in table 9doublefeh_listFiber pointing right ascension (degree)charudecFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.doublegp_idTarget designationlong"public".med_cataloguemobsidUnique spectrum ID for each observation of each targetmeta.idcharobsidUnique source identifier calculated with the "ura" and "udec" in table 9meta.idlongdesignationTarget observation datecharobsdateLocal modified Julian daytime.epochcharlmjdModified Julian dayintmjdPlan nameintplanidSpectrograph IDcharspidFiber IDintfiberidFiber pointing right ascension (degree)intlmjmFiber pointing declination (degree)longbandS/N of u filtercharra_obsS/N of g filterpos.eq.radoubledec_obsS/N of r filterpos.eq.decdoublesnrS/N of i filterdoublegaia_source_idS/N of z filterchargaia_bp_mean_magStellar spectral typedoublegaia_rp_mean_magRedshiftdoublefibertypeRedshift uncertaintycharoffsetsThe objID in the Pan-STARRS catalogintoffsets_vPan-STARRS g band magnitudedoubleraPan-STARRS r band magnitudepos.eq.radoubledecPan-STARRS i band magnitudepos.eq.decdoublerv_b0Pan-STARRS z band magnitudedoublerv_b0_errPan-STARRS y band magnitudedoublerv_b1The "source_id" field of Gaia DR3 catalogdoublerv_b1_errThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublerv_b_flagFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]intrv_r0Whether there is a fiber offset during observationdoublerv_r1Right ascension from input catalog (degree)doublerv_r1_errDeclination from input catalog (degree)doublerv_r_flagSpectral sub-types of white dwarf starsintrv_br0_errEffective temperature uncertainty obtained by the LASPdoublerv_br1_errSurface gravity uncertainty obtained by the LASPdoublerv_br_flagMetallicity uncertainty obtained by the LASPintrv_lasp0_errUncertainty of heliocentric radial velocity obtained by the LASPdoublerv_lasp1Alpha element abundance estimated by the LASPdoublecoaddProjected rotation velocity given by the LASPintfibermaskOptical depth at the Balmer edge of 3646 Åintbad_bThe coefficient of the first term of the third-order polynomial in the continuum fittingintmoon_angleThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublelunardateContinuum luminosity in common logarithm at rest-frame 1350 ÅintsubprojectContinuum luminosity in common logarithm at rest-frame 5100 Åcharbad_rThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingintrv_br1Surface gravity obtained by the LASPdoublerv_lasp0Heliocentric radial velocity obtained by the LASPdoublerv_lasp1_errThe uncertainty of alpha_mdoublerv_br0Effective temperature obtained by the LASPdoublerv_r0_errIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublegaia_g_mean_magSpectral typedoubleuidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.charmoon_flgContinuum luminosity in common logarithm at rest-frame 3000 Åchargp_idTarget designationlong"public".med_combinedmobsidUnique spectrum ID for each observation of each targetmeta.idcharobsidUnique source identifier calculated with the "ura" and "udec" in table 9meta.idlongra_obsS/N of g filterpos.eq.radoubledec_obsS/N of r filterpos.eq.decdoublesnrS/N of i filterdoublegaia_source_idS/N of z filterchargaia_bp_mean_magStellar spectral typedoublegaia_rp_mean_magRedshiftdoubleoffsetsThe objID in the Pan-STARRS catalogintraPan-STARRS r band magnitudepos.eq.radoubledecPan-STARRS i band magnitudepos.eq.decdoublerv_b0_errPan-STARRS y band magnitudedoublerv_b1The "source_id" field of Gaia DR3 catalogdoublerv_b1_errThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublerv_b_flagFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]intrv_r1Right ascension from input catalog (degree)doublerv_r_flagSpectral sub-types of white dwarf starsintrv_br0_errEffective temperature uncertainty obtained by the LASPdoublerv_br1Surface gravity obtained by the LASPdoublerv_br1_errSurface gravity uncertainty obtained by the LASPdoublerv_lasp0Heliocentric radial velocity obtained by the LASPdoublerv_lasp1Alpha element abundance estimated by the LASPdoublerv_lasp1_errThe uncertainty of alpha_mdoublefibermaskOptical depth at the Balmer edge of 3646 Åintbad_bThe coefficient of the first term of the third-order polynomial in the continuum fittingintmoon_angleThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublelunardateContinuum luminosity in common logarithm at rest-frame 1350 ÅintsubprojectContinuum luminosity in common logarithm at rest-frame 5100 Åcharvsini_laspThe name of the first group of spectral linesdoublelogg_cnnThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prodoublesi_feMinimal chi-square in the fitting of the second group linesdoublemg_feReduced chi-square in the fitting of the second group linesdoubleo_feDegree of freedom in the fitting of the second group linesdoublefeh_laspThe name of the first group of spectral linesdoublefeh_lasp_errThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublealpha_m_cnnMinimal chi-square in the fitting of the third group linesdoubleteff_lasp_errReduced chi-square in the fitting of the third group linesdoublefeh_cnnDegree of freedom in the fitting of the third group linesdoubleni_feThe name of the fourth group of spectral linesdoubleteff_cnnThe fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublecu_feMinimal chi-square in the fitting of the fourth group linesdoublen_feReduced chi-square in the fitting of the fourth group linesdoublelogg_lasp_errDegree of freedom in the fitting of the fourth group linesdoublevsini_lasp_errThe name of the fifth group of spectral linesdoublecr_feThe fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleti_feMinimal chi-square in the fitting of the fifth group linesdoubles_feDegree of freedom in the fitting of the fifth group linesdoubleal_feThe name of the sixth group of spectral linesdoublefileDegree of freedom in the fitting of the sixth group linescharspecPeak flux of Lya broad componentcharrv_r1_errDeclination from input catalog (degree)doublespidFiber IDintteff_laspDegree of freedom in the fitting of the first group linesdoublebad_rThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingintc_feThe name of the second group of spectral linesdoublerv_br_flagMetallicity uncertainty obtained by the LASPintrv_lasp0_errUncertainty of heliocentric radial velocity obtained by the LASPdoublecoaddProjected rotation velocity given by the LASPintrv_b0Pan-STARRS z band magnitudedoublelmjdModified Julian dayintlogg_laspMinimal chi-square in the fitting of the first group linesdoublemjdPlan nameintobsdateLocal modified Julian daytime.epochcharrv_r0_errIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleplanidSpectrograph IDcharca_feReduced chi-square in the fitting of the first group linesdoublegaia_vari_type_sosMinimal chi-square in the fitting of the sixth group linescharbandS/N of u filtercharrv_br0Effective temperature obtained by the LASPdoublefibertypeRedshift uncertaintychargaia_g_mean_magSpectral typedoublefiberidFiber pointing right ascension (degree)intmoon_flgContinuum luminosity in common logarithm at rest-frame 3000 ÅcharuidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.charalpha_m_laspThe fitting status of the sixth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublealpha_m_lasp_errThe fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubledesignationTarget observation datecharoffsets_vPan-STARRS g band magnitudedoublerv_r0Whether there is a fiber offset during observationdoublelmjmFiber pointing declination (degree)longgp_idTarget designationlongm_h_cnnReduced chi-square in the fitting of the fifth group linesdouble"public".med_inputcatalogobsidUnique spectrum ID for each observation of each targetmeta.idlongobsdateUnique source identifier calculated with the "ura" and "udec" in table 9time.epochcharfiberidTarget observation dateintunitidLocal modified Julian daycharra_obsModified Julian daypos.eq.radoubledec_obsPlan namepos.eq.decdoubleobjtypeSpectrograph IDcharmagtypeFiber IDcharmag1Fiber pointing right ascension (degree)doublefibertypeStellar spectral typechartfromRedshiftcharoffsetsThe objID in the Pan-STARRS catalogintraPan-STARRS r band magnitudepos.eq.radoubleepochPan-STARRS z band magnitudecharmag2Fiber pointing declination (degree)doubledecPan-STARRS i band magnitudepos.eq.decdoubletnamePan-STARRS y band magnitudecharmag4S/N of g filterdoublemag5S/N of r filterdoublemag7S/N of z filterdoubletcommentRedshift uncertaintychartsourceSpectral typecharspidTarget designationintplanidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.charoffsets_vPan-STARRS g band magnitudedoublemag6S/N of i filterdoublemag3S/N of u filterdouble"public".med_mecobs_numberTarget observation dateintfeh_lasp_listSpectrograph IDcharexp_numberFiber IDintlmjm_listFiber pointing right ascension (degree)charrv_b0_listFiber pointing declination (degree)charrv_b1_listS/N of u filtercharrv_r0_listS/N of g filtercharrv_r1_listS/N of r filtercharrv_br1_listS/N of z filtercharobsid_listLocal modified Julian daycharteff_lasp_listModified Julian daycharuidUnique spectrum ID for each observation of each targetcharlogg_lasp_listPlan namecharuraUnique source identifier calculated with the "ura" and "udec" in table 9doublegaia_vari_type_sosSpectral typecharudecFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.doublerv_br0_listS/N of i filterchargp_idTarget designationlong"public".med_planlmjm_listSpectrograph IDcharmagLocal modified Julian daydoubleseeingModified Julian daydoubledecTarget observation datepos.eq.decdoublepidUnique spectrum ID for each observation of each targetintexptimePlan namecharobsdateUnique source identifier calculated with the "ura" and "udec" in table 9time.epochcharraTarget designationpos.eq.radoubleplanidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.char"public".med_stellarmobsidUnique spectrum ID for each observation of each targetmeta.idcharobsidUnique source identifier calculated with the "ura" and "udec" in table 9meta.idlongdesignationTarget observation datecharobsdateLocal modified Julian daytime.epochcharlmjdModified Julian dayintmjdPlan nameintspidFiber IDintfiberidFiber pointing right ascension (degree)intlmjmFiber pointing declination (degree)longbandS/N of u filterchardec_obsS/N of r filterpos.eq.decdoublesnrS/N of i filterdoublegaia_source_idS/N of z filterchargaia_bp_mean_magStellar spectral typedoubleoffsetsThe objID in the Pan-STARRS catalogintraPan-STARRS r band magnitudepos.eq.radoubledecPan-STARRS i band magnitudepos.eq.decdoubleteff_lasp_errPan-STARRS y band magnitudedoublelogg_laspThe "source_id" field of Gaia DR3 catalogdoublefeh_laspFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]doublevsini_lasp_errRight ascension from input catalog (degree)doublerv_b0Declination from input catalog (degree)doublerv_b1_errEffective temperature uncertainty obtained by the LASPdoublerv_b_flagSurface gravity obtained by the LASPintrv_r0Surface gravity uncertainty obtained by the LASPdoublerv_r1Heliocentric radial velocity obtained by the LASPdoublerv_r_flagAlpha element abundance estimated by the LASPintrv_br0The uncertainty of alpha_mdoublerv_br1Optical depth at the Balmer edge of 3646 Ådoublerv_br_flagThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingintrv_lasp0The coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublerv_lasp1_errContinuum luminosity in common logarithm at rest-frame 5100 Ådoubleteff_cnnDegree of freedom in the fitting of the first group linesdoublefeh_cnnThe fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublen_feReduced chi-square in the fitting of the second group linesdoubleo_feDegree of freedom in the fitting of the second group linesdoublemg_feThe name of the first group of spectral linesdoubleal_feThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublesi_feMinimal chi-square in the fitting of the third group linesdoubles_feReduced chi-square in the fitting of the third group linesdoubleca_feDegree of freedom in the fitting of the third group linesdoublecr_feThe fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleni_feMinimal chi-square in the fitting of the fourth group linesdoublealpha_m_laspDegree of freedom in the fitting of the fourth group linesdoublealpha_m_lasp_errThe name of the fifth group of spectral linesdoublemoon_angleThe fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doublelunardateMinimal chi-square in the fitting of the fifth group linesintmoon_flgReduced chi-square in the fitting of the fifth group lineschargp_idTarget designationlonglogg_lasp_errThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublecoaddThe name of the first group of spectral linesintrv_br1_errThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublelogg_cnnThe name of the second group of spectral linesdoublerv_r0_errMetallicity uncertainty obtained by the LASPdoublerv_r1_errUncertainty of heliocentric radial velocity obtained by the LASPdoublerv_br0_errProjected rotation velocity given by the LASPdoubleteff_laspPan-STARRS z band magnitudedoublem_h_cnnReduced chi-square in the fitting of the first group linesdoublera_obsS/N of g filterpos.eq.radoublegaia_rp_mean_magRedshiftdoubleoffsets_vPan-STARRS g band magnitudedoublevsini_laspIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleplanidSpectrograph IDcharrv_b0_errSpectral sub-types of white dwarf starsdoubleti_feThe name of the fourth group of spectral linesdoublecu_feReduced chi-square in the fitting of the fourth group linesdoublealpha_m_cnnMinimal chi-square in the fitting of the first group linesdoublerv_b1Effective temperature obtained by the LASPdoublefibertypeRedshift uncertaintychargaia_g_mean_magSpectral typedoublefibermaskThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prointrv_lasp0_errContinuum luminosity in common logarithm at rest-frame 1350 Ådoublerv_lasp1Continuum luminosity in common logarithm at rest-frame 3000 Ådoublefeh_lasp_errWhether there is a fiber offset during observationdoublec_feMinimal chi-square in the fitting of the second group linesdoubleuidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.char"public".mstellarobsidUnique spectrum ID for each observation of each targetmeta.idlonguidUnique source identifier calculated with the "ura" and "udec" in table 9charobsdateTarget observation datetime.epochcharlmjdLocal modified Julian dayintmjdModified Julian dayintplanidPlan namecharspidSpectrograph IDintsnrrS/N of r filterdoublesnriS/N of i filterdoublesnrzS/N of z filterdoublesubclassStellar spectral typecharzRedshiftdoublez_errRedshift uncertaintydoubleps_idThe objID in the Pan-STARRS cataloglongmag_ps_gPan-STARRS g band magnitudedoublemag_ps_rPan-STARRS r band magnitudedoublemag_ps_iPan-STARRS i band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublemag_ps_yPan-STARRS y band magnitudedoublegaia_source_idThe "source_id" field of Gaia DR3 catalogcharfibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charoffsetsWhether there is a fiber offset during observationintraRight ascension from input catalog (degree)pos.eq.radoubledecDeclination from input catalog (degree)pos.eq.decdoubleteffSpectral sub-types of white dwarf starsdoubleteff_errEffective temperature obtained by the LASPdoublelogg_errSurface gravity obtained by the LASPdoubleewhaHeliocentric radial velocity obtained by the LASPdoubleewha_errUncertainty of heliocentric radial velocity obtained by the LASPdoubletio5Alpha element abundance estimated by the LASPdoublecah3Projected rotation velocity given by the LASPdoubletio2The coefficient of the first term of the third-order polynomial in the continuum fittingdoubletio3The coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublecah1Continuum luminosity in common logarithm at rest-frame 1350 Ådoubletio5_errContinuum luminosity in common logarithm at rest-frame 5100 Ådoublecah2_errThe name of the first group of spectral linesdoublecah3_errThe fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prodoubletio2_errReduced chi-square in the fitting of the first group linesdoubletio3_errDegree of freedom in the fitting of the first group linesdoublezetaReduced chi-square in the fitting of the second group linesdoublezeta_errDegree of freedom in the fitting of the second group linesdoubletypeThe name of the first group of spectral linesdoublenaThe fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubledec_obsFiber pointing declination (degree)pos.eq.decdoublegaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoubletio1Optical depth at the Balmer edge of 3646 Ådoubletio4The coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublem_hSurface gravity uncertainty obtained by the LASPdoublecaoh_errMinimal chi-square in the fitting of the second group linesdoublecah2The uncertainty of alpha_mdoublecah1_errThe fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.doubleloggEffective temperature uncertainty obtained by the LASPdoubletio1_errMinimal chi-square in the fitting of the first group linesdoublera_obsFiber pointing right ascension (degree)pos.eq.radoublesnrgS/N of g filterdoublesnruS/N of u filterdoubleclassSpectral typecharfiberidFiber IDintoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublegp_idFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.longcaohContinuum luminosity in common logarithm at rest-frame 3000 Ådoublem_h_errMetallicity uncertainty obtained by the LASPdoubletio4_errThe name of the second group of spectral linesdoubledesignationTarget designationchar"public".planpidUnique spectrum ID for each observation of each targetintdecTarget observation datepos.eq.decdoubleseeingModified Julian daydoubleexptimePlan namecharlmjmSpectrograph IDlongmagLocal modified Julian daydoubleobsdateUnique source identifier calculated with the "ura" and "udec" in table 9time.epochcharraTarget designationpos.eq.radoubleplanidFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.char"public".qsoobsidUnique spectrum ID for each observation of each targetmeta.idlonglmjdLocal modified Julian dayintmjdModified Julian dayintplanidPlan namecharspidSpectrograph IDintfiberidFiber IDintdec_obsFiber pointing declination (degree)pos.eq.decdoublesnruS/N of u filterdoublesnrgS/N of g filterdoublesnrrS/N of r filterdoublesnriS/N of i filterdoublesnrzS/N of z filterdoublezRedshiftdoubleps_idThe objID in the Pan-STARRS cataloglongmag_ps_rPan-STARRS r band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublemag_ps_yPan-STARRS y band magnitudedoublegaia_source_idThe "source_id" field of Gaia DR3 catalogchargaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoubleraRight ascension from input catalog (degree)pos.eq.radoublesn_ratio_contiSpectral sub-types of white dwarf starsdoublefe_uv_fwhmEffective temperature uncertainty obtained by the LASPdoublefe_op_normSurface gravity uncertainty obtained by the LASPdoublefe_op_fwhmMetallicity uncertainty obtained by the LASPdoublepl_normUncertainty of heliocentric radial velocity obtained by the LASPdoublebalmer_normThe uncertainty of alpha_mdoublepoly_aThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublepoly_bThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoubleline_name_1The name of the first group of spectral linescharmin_chi2_1Minimal chi-square in the fitting of the first group linesdoublendof_1Degree of freedom in the fitting of the first group linesintline_name_2The name of the second group of spectral linescharmin_chi2_2Minimal chi-square in the fitting of the second group linesdoublered_chi2_2Reduced chi-square in the fitting of the second group linesdoublendof_2Degree of freedom in the fitting of the second group linesintline_name_3The name of the first group of spectral linescharfitting_status_3The fitting status of the third group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intred_chi2_3Reduced chi-square in the fitting of the third group linesdoubleline_name_4The name of the fourth group of spectral linescharfitting_status_4The fitting status of the fourth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intmin_chi2_4Minimal chi-square in the fitting of the fourth group linesdoublendof_4Degree of freedom in the fitting of the fourth group linesintline_name_5The name of the fifth group of spectral linescharndof_5Degree of freedom in the fitting of the fifth group linesintfitting_status_6The fitting status of the sixth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intred_chi2_6Reduced chi-square in the fitting of the sixth group linesintlya_br_1_peak_fluxPeak flux of Lya broad componentdoublelya_br_1_sigmaLine dispersion in natural logarithm of Lya broad componentdoublelya_na_1_peak_fluxPeak flux of Lya narrow componentdoublelya_na_1_peak_wavelengthPeak wavelength in natural logarithm of Lya narrow componentdoublelya_na_1_sigmaLine dispersion in natural logarithm of Lya narrow componentdoubleciv_br_1_sigmaLine dispersion in natural logarithm of C IV broad componentdoubleciv_na_1_peak_fluxPeak flux of C IV narrow componentdoubleciv_na_1_peak_wavelengthPeak wavelength in natural logarithm of C IV narrow componentdoubleciv_na_1_sigmaLine dispersion in natural logarithm of CIV narrow componentdoubleciii_br_1_peak_fluxPeak flux of the first C III broad componentdoubleciii_br_1_sigmaLine dispersion in natural logarithm of the first C III broad componentdoubleciii_br_2_peak_wavelengthPeak wavelength in natural logarithm of the second C III broad componentdoubleciii_na_1_peak_fluxPeak flux of the first C III narrow componentintciii_na_1_peak_wavelengthPeak wavelength in natural logarithm of the first C III narrow componentintciii_na_1_sigmaLine dispersion in natural logarithm of the first C III narrow componentintciii_na_2_peak_wavelengthPeak wavelength in natural logarithm of the second C III narrow componentintmgii_br_1_peak_fluxPeak flux of Mg II broad componentdoublemgii_br_1_peak_wavelengthPeak wavelength in natural logarithm of Mg II broad componentdoublemgii_na_1_peak_fluxPeak flux of the first Mg II narrow componentdoublemgii_na_2_peak_fluxPeak flux of the second Mg II narrow componentdoublemgii_na_2_peak_wavelengthPeak wavelength in natural logarithm of the second Mg II narrow componentdoublemgii_na_2_sigmaLine dispersion in natural logarithm of the second Mg II narrow componentdoublehb_br_1_peak_fluxPeak flux of Hbeta broad componentdoublehb_br_1_sigmaLine dispersion in natural logarithm of Hbeta broad componentdoublehb_na_1_peak_fluxPeak flux of Hbeta narrow componentdoublehb_na_1_peak_wavelengthPeak wavelength in natural logarithm of Hbeta narrow componentdoublehb_na_1_sigmaLine dispersion in natural logarithm of Hbeta narrow componentdoubleoiii4959_1_peak_fluxPeak flux of [O III] 4959doubleoiii4959_1_peak_wavelengthPeak wavelength in natural logarithm of [O III] 4959doubleoiii4959_1_sigmaLine dispersion in natural logarithm of [O III] 4959doubleoiii5007_1_peak_wavelengthPeak wavelength in natural logarithm of [O III] 5007doubleoiii5007_1_sigmaLine dispersion in natural logarithm of [O III] 5007doubleha_br_3_sigmaLine dispersion in natural logarithm of the third Halpha broad componentdoubleha_na_1_peak_fluxPeak flux of Halpha narrow componentdoubleha_na_1_sigmaLine dispersion in natural logarithm of Halpha narrow componentdoublenii6549_1_peak_fluxPeak flux of [N II] 6549doublenii6549_1_peak_wavelengthPeak wavelength in natural logarithm of [N II] 6549doublenii6549_1_sigmaLine dispersion in natural logarithm of [N II] 6549doublenii6585_1_peak_fluxPeak flux of [N II] 6585doublenii6585_1_sigmaLine dispersion in natural logarithm of [N II] 6585doublesii6718_1_peak_fluxPeak flux of [S II] 6718doublesii6718_1_peak_wavelengthPeak wavelength in natural logarithm of [S II] 6718doublesii6718_1_sigmaLine dispersion in natural logarithm of [S II] 6718doublesii6732_1_peak_fluxPeak flux of [S II] 6732doublelya_ewEW of entire Lyadoublelya_peak_wavelengthPeak wavelenth of entire Lyadoublelya_areaIntegrated Flux of entire Lyadoubleciv_fwhmFWHM of entire C IVdoubleciv_sigmaLine dispersion of entire C IVdoubleciv_ewEW of entire C IVdoubleciv_peak_wavelengthPeak wavelenth of entire C IVdoubleciii_fwhmFWHM of entire C IIIdoubleciii_ewEW of entire C IIIdoubleciii_areaIntegrated Flux of entire C IIIdoublemgii_fwhmFWHM of entire Mg IIdoublemgii_sigmaLine dispersion of entire Mg IIdoublemgii_peak_wavelengthPeak wavelenth of entire Mg IIdoublemgii_areaIntegrated Flux of entire Mg IIdoublehb_fwhmFWHM of entire Hbetadoublehb_sigmaLine dispersion of entire Hbetadoublehb_ewEW of entire Hbetadoublehb_peak_wavelengthPeak wavelenth of entire Hbetadoublehb_areaIntegrated Flux of entire Hbetadoubleha_fwhmFWHM of entire Halphadoubleha_sigmaLine dispersion of entire Halphadoubleha_ewEW of entire Halphadoubleha_areaIntegrated Flux of entire HalphadoubledecDeclination from input catalog (degree)pos.eq.decdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charl5100Continuum luminosity in common logarithm at rest-frame 5100 Ådoublebalmer_tau_eOptical depth at the Balmer edge of 3646 Ådoublepoly_cThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublefe_uv_shiftSurface gravity obtained by the LASPdoublefe_op_shiftHeliocentric radial velocity obtained by the LASPdoublepl_slopeAlpha element abundance estimated by the LASPdoublebalmer_teffProjected rotation velocity given by the LASPintfe_uv_normEffective temperature obtained by the LASPdoublemag_ps_iPan-STARRS i band magnitudedoubleobsdateTarget observation datetime.epochcharoffsetsWhether there is a fiber offset during observationintred_chi2_1Reduced chi-square in the fitting of the first group linesdoublera_obsFiber pointing right ascension (degree)pos.eq.radoublesubclassStellar spectral typecharz_errRedshift uncertaintydoubleoiii5007_1_peak_fluxPeak flux of [O III] 5007doubleha_br_1_peak_wavelengthPeak wavelength in natural logarithm of the first Halpha broad componentdoubleciv_br_1_peak_fluxPeak flux of CIV broad componentdoublendof_6Degree of freedom in the fitting of the sixth group linesintha_br_2_peak_fluxPeak flux of the second Halpha broad componentdoubleciv_areaIntegrated Flux of entire C IVdoubleha_br_3_peak_fluxPeak flux of Halpha broad componentdoubleha_br_1_sigmaLine dispersion in natural logarithm of the first Halpha broad componentdoubleha_br_3_peak_wavelengthPeak wavelength in natural logarithm of the third Halpha broad componentdoublendof_3Degree of freedom in the fitting of the third group linesintlya_sigmaLine dispersion of entire Lyadoubleciii_peak_wavelengthPeak wavelenth of entire C IIIdoublefitting_status_1The fitting status of the first group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.prointfitting_status_2The fitting status of the second group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intha_peak_wavelengthPeak wavelenth of entire Halphadoubleha_na_1_peak_wavelengthPeak wavelength in natural logarithm of Halpha narrow componentdoubleha_br_1_peak_fluxPeak flux of the first Halpha broad componentdoubleciii_sigmaLine dispersion of entire C IIIdoublelya_fwhmFWHM of entire Lyadoublemgii_ewEW of entire Mg IIdoublemin_chi2_6Minimal chi-square in the fitting of the sixth group linesintha_br_2_sigmaLine dispersion in natural logarithm of the second Halpha broad componentdoublemgii_na_1_peak_wavelengthPeak wavelength in natural logarithm of the first Mg II narrow componentdoublemgii_br_1_sigmaLine dispersion in natural logarithm of Mg II broad componentdoublered_chi2_4Reduced chi-square in the fitting of the fourth group linesdoublesii6732_1_peak_wavelengthPeak wavelength in natural logarithm of [S II] 6732doublesii6732_1_sigmaLine dispersion in natural logarithm of [S II] 6732doublehb_br_1_peak_wavelengthPeak wavelength in natural logarithm of Hbeta broad componentdoubleciii_br_2_peak_fluxPeak flux of the second C III broad componentdoubleciii_br_1_peak_wavelengthPeak wavelength in natural logarithm of the first C III broad componentdoublelya_br_1_peak_wavelengthPeak wavelength in natural logarithm of Lya broad componentdoubleciii_na_2_sigmaLine dispersion in natural logarithm of the second CIII narrow componentintgp_idFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.longuidUnique source identifier calculated with the "ura" and "udec" in table 9charciii_na_2_peak_fluxPeak flux of the second C III narrow componentintciv_br_1_peak_wavelengthPeak wavelength in natural logarithm of C IV broad componentdoublefitting_status_5The fitting status of the fifth group lines, and the value larger than 0 means a success fitting. See https://idlastro.gsfc.nasa.gov/ftp/pro/markwardt/mpfit.pro for other values.intclassSpectral typecharl1350Continuum luminosity in common logarithm at rest-frame 1350 Ådoublel3000Continuum luminosity in common logarithm at rest-frame 3000 Ådoubleline_name_6The name of the sixth group of spectral linescharmin_chi2_3Minimal chi-square in the fitting of the third group linesdoublemag_ps_gPan-STARRS g band magnitudedoublemin_chi2_5Minimal chi-square in the fitting of the fifth group linesintdesignationTarget designationcharred_chi2_5Reduced chi-square in the fitting of the fifth group linesintha_br_2_peak_wavelengthPeak wavelength in natural logarithm of the second Halpha broad componentdoublemgii_na_1_sigmaLine dispersion in natural logarithm of the first Mg II narrow componentdoublenii6585_1_peak_wavelengthPeak wavelength in natural logarithm of [N II] 6585doubleoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)double"public".stellarobsdateTarget observation datetime.epochcharmjdModified Julian dayintplanidPlan namecharspidSpectrograph IDintfiberidFiber IDintra_obsFiber pointing right ascension (degree)pos.eq.radoublesnruS/N of u filterdoublesnrgS/N of g filterdoublesnrrS/N of r filterdoublesnriS/N of i filterdoublesnrzS/N of z filterdoublesubclassStellar spectral typecharzRedshiftdoubleps_idThe objID in the Pan-STARRS cataloglongmag_ps_gPan-STARRS g band magnitudedoublemag_ps_rPan-STARRS r band magnitudedoublemag_ps_iPan-STARRS i band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublegaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charoffsetsWhether there is a fiber offset during observationintdecDeclination from input catalog (degree)pos.eq.decdoubleteffSpectral sub-types of white dwarf starsdoubleloggEffective temperature uncertainty obtained by the LASPdoublelogg_errSurface gravity obtained by the LASPdoublefehSurface gravity uncertainty obtained by the LASPdoublefeh_errMetallicity uncertainty obtained by the LASPdoublervHeliocentric radial velocity obtained by the LASPdoublerv_errUncertainty of heliocentric radial velocity obtained by the LASPdoublealpha_mAlpha element abundance estimated by the LASPdoublevsini_laspProjected rotation velocity given by the LASPdoubledec_obsFiber pointing declination (degree)pos.eq.decdoublealpha_m_errThe uncertainty of alpha_mdoublemag_ps_yPan-STARRS y band magnitudedoublegaia_source_idThe "source_id" field of Gaia DR3 catalogcharuidUnique source identifier calculated with the "ura" and "udec" in table 9charteff_errEffective temperature obtained by the LASPdoublez_errRedshift uncertaintydoublelmjdLocal modified Julian dayintoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleobsidUnique spectrum ID for each observation of each targetmeta.idlongclassSpectral typecharraRight ascension from input catalog (degree)pos.eq.radoubledesignationTarget designationchargp_idFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.long"public".wduidUnique source identifier calculated with the "ura" and "udec" in table 9charobsdateTarget observation datetime.epochcharlmjdLocal modified Julian dayintmjdModified Julian dayintplanidPlan namecharspidSpectrograph IDintfiberidFiber IDintra_obsFiber pointing right ascension (degree)pos.eq.radoubledec_obsFiber pointing declination (degree)pos.eq.decdoublesnruS/N of u filterdoublesnrgS/N of g filterdoublesnrrS/N of r filterdoublesnriS/N of i filterdoublesnrzS/N of z filterdoublesubclassStellar spectral typecharzRedshiftdoublez_errRedshift uncertaintydoubleps_idThe objID in the Pan-STARRS cataloglongmag_ps_gPan-STARRS g band magnitudedoublemag_ps_rPan-STARRS r band magnitudedoublemag_ps_iPan-STARRS i band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublemag_ps_yPan-STARRS y band magnitudedoublegaia_source_idThe "source_id" field of Gaia DR3 catalogchargaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charoffsetsWhether there is a fiber offset during observationintraRight ascension from input catalog (degree)pos.eq.radoubledecDeclination from input catalog (degree)pos.eq.decdoublewd_subclassSpectral sub-types of white dwarf starscharteffEffective temperature obtained by the LASPdoubleteff_errEffective temperature uncertainty obtained by the LASPdoubleloggSurface gravity obtained by the LASPdoublelogg_errSurface gravity uncertainty obtained by the LASPdoubleobsidUnique spectrum ID for each observation of each targetmeta.idlongoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleclassSpectral typechardesignationTarget designationchargp_idFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.longTAP_SCHEMATAP_SCHEMA.columnsarraysizeLocal modified Julian daycharprincipalstdcolumn_indexUnique spectrum ID for each observation of each targetintprincipalstdcolumn_nameTarget designationcharprincipalstddatatypeTarget observation datecharprincipalstddescriptionSpectrograph IDcharprincipalstdindexedS/N of u filterintprincipalstdprincipalS/N of g filterintprincipalstdschema_nameUnique source identifier calculated with the "ura" and "udec" in table 9charprincipalstd"size"Plan nameintprincipalstdstdS/N of r filterintprincipalstdtable_nameFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.charprincipalstducdFiber pointing declination (degree)charprincipalstdunitFiber pointing right ascension (degree)charprincipalstdutypeFiber IDcharprincipalstdxtypeModified Julian daycharprincipalstd TAP_SCHEMA.tables table_name table_name TAP_SCHEMA.key_columnsfrom_columnUnique source identifier calculated with the "ura" and "udec" in table 9charprincipalstdkey_idUnique spectrum ID for each observation of each targetcharprincipalstdtarget_columnFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.charprincipalstd TAP_SCHEMA.keys key_id key_id TAP_SCHEMA.columns from_column column_name TAP_SCHEMA.columns target_column column_name TAP_SCHEMA.keysdescriptionTarget designationcharprincipalstdfrom_tableUnique source identifier calculated with the "ura" and "udec" in table 9charprincipalstdkey_idUnique spectrum ID for each observation of each targetcharprincipalstdtarget_tableFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.charprincipalstdutypeTarget observation datecharprincipalstd TAP_SCHEMA.tables from_table table_name TAP_SCHEMA.tables target_table table_name TAP_SCHEMA.schemasdescriptionTarget designationcharprincipalstdschema_indexUnique spectrum ID for each observation of each targetintprincipalstdschema_nameUnique source identifier calculated with the "ura" and "udec" in table 9charprincipalstdutypeFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.charprincipalstdTAP_SCHEMA.tablesdescriptionLocal modified Julian daycharprincipalstdschema_nameUnique source identifier calculated with the "ura" and "udec" in table 9charprincipalstdtable_indexUnique spectrum ID for each observation of each targetintprincipalstdtable_nameFor each LAMOST source, the equatorial coordinates ("ura" and "udec" in table 9) used to calculate "uid" were from which survey (Pan-STARRS, Gaia or LAMOST), "gp_id" gives the corresponding source identifier in that survey.charprincipalstdtable_typeTarget designationcharprincipalstdutypeTarget observation datecharprincipalstd TAP_SCHEMA.schemas schema_name schema_name