publicpublic.combinedvsini_laspUncertainty of heliocentric radial velocity obtained by the LASPdoublemag_ps_yPan-STARRS y band magnitudedoubleloggThe uncertainty of alpha_mdoubleobsdateTarget observation datecharsnrrS/N of r filterdoublera_obsFiber pointing right ascension (degree)doublefehOptical depth at the Balmer edge of 3646 Ådoublealpha_mMetallicity uncertainty obtained by the LASPdoublefiberidFiber IDintlmjdLocal modified Julian daytime.epochintplanidPlan namecharfeh_errThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublealpha_m_errHeliocentric radial velocity obtained by the LASPdoubleteffProjected rotation velocity given by the LASPdoubleteff_errSurface gravity obtained by the LASPdoublemjdModified Julian daytime.epochintspidSpectrograph IDintcaohReduced chi-square in the fitting of the sixth group linesdoublehalpha_d02The 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.doubletio5_errMinimal chi-square in the fitting of the fifth group linesdoublenaThe name of the sixth group of spectral linesdoublehdelta_d02Reduced chi-square in the fitting of the second group linesdoubletio3_errThe 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.doublevsig_errPeak flux of [O III] 4959doublehbeta24Minimal chi-square in the fitting of the first group linesdoubleoiii_4960_fluxLine dispersion in natural logarithm of Mg II broad componentdoubletio3Line dispersion in natural logarithm of Lya narrow componentdoubletio1_errLine dispersion in natural logarithm of CIV narrow componentdoubletio2_errLine dispersion in natural logarithm of C IV broad componentdoubleewha_errPeak wavelength in natural logarithm of the first C III broad componentdoublehalpha_fluxPeak flux of Hbeta broad componentdoublemin_chi2_1Line dispersion in natural logarithm of the first Halpha broad componentdoublecah1Peak wavelength in natural logarithm of Lya narrow componentdoubletio1Peak flux of the second C III broad componentdoublecah1_errDegree of freedom in the fitting of the fifth group linesdoubletio5Peak flux of Lya broad componentdoublehgamma_d02The name of the fourth group of spectral linesdoublesii_6733_fluxPeak flux of the first Halpha broad componentdoublesii_6718_fluxPeak wavelength in natural logarithm of the first Mg II narrow componentdoublehalpha48Minimal chi-square in the fitting of the third group linesdoublecah3_errPeak flux of the first C III broad componentdoublehdelta48Degree of freedom in the fitting of the first group linesdoubleciv_peak_wavelengthPeak wavelength in natural logarithm of the first Halpha broad componentdoublehdelta24Degree of freedom in the fitting of the second group linesdoublenii_6585_fluxPeak flux of [O III] 5007doubleabs_gmagPeak flux of the first C III narrow componentdoubleciv_fwhmPeak flux of the second Halpha broad componentdoubletio4_errPeak wavelength in natural logarithm of Lya broad componentdoublehbeta48The name of the fifth group of spectral linesdoublemetal_lwLine dispersion in natural logarithm of [O III] 4959doublehgamma12The coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublehbeta_ewPeak flux of the first Mg II narrow componentdoublesii_6718_ewLine dispersion in natural logarithm of the first Mg II narrow componentdoublezetaLine dispersion in natural logarithm of Lya broad componentdoubleage_lwPeak wavelength in natural logarithm of the second Mg II narrow componentdoublenii_6585_ewPeak wavelength in natural logarithm of [O III] 4959doubleewhaPeak flux of Lya narrow componentdoublem_hPeak wavelength in natural logarithm of the second C III broad componentdoubleage_mwPeak flux of Mg II broad componentdoublecah2Peak flux of C IV narrow componentdoubleperiodPeak wavelength in natural logarithm of the first C III narrow componentdoublesubtypeLine dispersion in natural logarithm of the first C III narrow componentcharrPeak flux of the second C III narrow componentpos.eq.raintabs_gmag_errPeak wavelength in natural logarithm of the second C III narrow componentdoublecah3Peak flux of CIV broad componentdoubleciii_br_2_peak_fluxPeak flux of the second C III broad componentdoublenii6585_1_sigmaLine dispersion in natural logarithm of [S II] 6732doubleline_name_4FWHM of entire Lyacharciii_peak_wavelengthPeak wavelenth of entire C IIIdoublemgii_na_2_peak_fluxFWHM of entire Halphadoublemgii_areaPeak wavelength in natural logarithm of [N II] 6549doubleciv_na_1_peak_fluxPeak flux of C IV narrow componentdoubleciii_fwhmPeak wavelength in natural logarithm of [S II] 6732doublelya_ewPeak wavelength in natural logarithm of [S II] 6718doublesii6718_1_peak_fluxEW of entire Mg IIdoublehb_na_1_sigmaIntegrated Flux of entire Halphadoublendof_6Line dispersion of entire Lyaintpl_slopeLine dispersion of entire C IIIdoublelya_peak_wavelengthLine dispersion in natural logarithm of the second Halpha broad componentdoubleha_br_3_sigmaLine dispersion in natural logarithm of the third Halpha broad componentdoubleha_fwhmFWHM of entire Halphadoubleline_name_5Integrated Flux of entire Hbetacharhb_br_1_peak_fluxPeak flux of Hbeta broad componentdoublehb_br_1_sigmaLine dispersion in natural logarithm of Hbeta broad componentdoublendof_3EW of entire C IVintha_br_2_peak_wavelengthPeak wavelength in natural logarithm of the second Halpha broad componentdoublehb_peak_wavelengthPeak wavelenth of entire Hbetadoubleciii_na_2_peak_fluxEW of entire Lyaintline_name_1The name of the first group of spectral linescharfitting_status_6Peak wavelenth of entire Lyaintmgii_br_1_sigmaEW of entire Hbetadoublelya_br_1_sigmaLine dispersion in natural logarithm of Lya broad componentdoublesii6732_1_sigmaLine dispersion in natural logarithm of [S II] 6718doubleciii_sigmaPeak flux of Halpha broad componentdoublefe_op_fwhmLine dispersion in natural logarithm of [N II] 6549doublepl_normFWHM of entire Hbetadoubleha_na_1_sigmaPeak wavelength in natural logarithm of Halpha narrow componentdoublemgii_peak_wavelengthPeak wavelenth of entire Mg IIdoublemgii_sigmaLine dispersion of entire Mg IIdoublemin_chi2_3Minimal chi-square in the fitting of the third group linesdoubleoiii4959_1_peak_fluxEW of entire C IIIdoublefe_uv_normFWHM of entire C IVdoublefe_op_shiftIntegrated Flux of entire Mg IIdoubleha_areaPeak wavelenth of entire C IIIdoublesii6732_1_peak_fluxLine dispersion of entire Hbetadoubleoiii5007_1_sigmaLine dispersion in natural logarithm of [O III] 5007doubleoiii5007_1_peak_fluxPeak wavelenth of entire Hbetadoublehb_fwhmIntegrated Flux of entire C IVdoublepoly_bThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublered_chi2_2Reduced chi-square in the fitting of the second group linesdoubleciv_br_1_peak_fluxPeak flux of [N II] 6549doublered_chi2_5Reduced chi-square in the fitting of the fifth group linesintred_chi2_4Line dispersion of entire Mg IIdoublel3000Integrated Flux of entire Lyadoubleciv_sigmaPeak flux of [S II] 6732doublesn_ratio_contiContinuum S/Ndoublendof_2Integrated Flux of entire C IIIintgaia_vari_type_soscharfilefile save pathcharlya_areaIntegrated Flux of entire Lyadoublendof_1Degree of freedom in the fitting of the first group linesintoiii4959_1_sigmaLine dispersion in natural logarithm of [O III] 4959doublesii6718_1_sigmaLine dispersion in natural logarithm of [S II] 6718doublespecFITS filenamemeta.idcharbalmer_tau_eOptical depth at the Balmer edge of 3646 Ådoublefe_op_normNormalization parameter of Fe II spectrum in optical banddoubleciii_areaIntegrated Flux 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 componentdoubleciii_ewEW of entire C IIIdoubleciii_na_1_peak_fluxPeak flux of the first C III narrow componentintciii_na_2_peak_wavelengthPeak wavelength in natural logarithm of the second C III narrow componentintciv_br_1_peak_wavelengthPeak wavelength in natural logarithm of C IV broad componentdoubleciv_br_1_sigmaLine dispersion in natural logarithm of C IV broad componentdoubleciv_ewEW of entire C IVdoublefitting_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_br_1_peak_fluxPeak flux of the first Halpha broad componentdoubleha_br_1_sigmaLine dispersion in natural logarithm of the first Halpha broad componentdoubleha_br_2_sigmaLine dispersion in natural logarithm of the second Halpha broad componentdoubleha_ewEW of entire Halphadoubleha_na_1_peak_fluxPeak flux of Halpha narrow componentdoubleha_peak_wavelengthPeak wavelenth of entire Halphadoubleha_sigmaLine dispersion of entire Halphadoublehb_ewEW of entire Hbetadoublehb_na_1_peak_fluxPeak flux of Hbeta narrow componentdoublel5100Continuum luminosity in common logarithm at rest-frame 5100 Ådoublelya_br_1_peak_fluxPeak flux of Lya broad componentdoublelya_br_1_peak_wavelengthPeak wavelength in natural logarithm of Lya broad componentdoublelya_fwhmFWHM of entire Lyadoublelya_na_1_sigmaLine dispersion in natural logarithm of Lya narrow componentdoublelya_sigmaLine dispersion of entire Lyadoublemgii_br_1_peak_wavelengthPeak wavelength in natural logarithm of Mg II broad componentdoublemgii_ewEW of entire Mg IIdoublemgii_fwhmFWHM of entire Mg IIdoublemgii_na_1_peak_wavelengthPeak wavelength in natural logarithm of the first Mg II narrow componentdoublemin_chi2_2Minimal chi-square in the fitting of the second group linesdoublemin_chi2_4Minimal chi-square in the fitting of the fourth group linesdoublendof_5Degree of freedom in the fitting of the fifth group linesintnii6549_1_sigmaLine dispersion in natural logarithm of [N II] 6549doublenii6585_1_peak_fluxPeak flux of [N II] 6585doubleoiii5007_1_peak_wavelengthPeak wavelength in natural logarithm of [O III] 5007doubleclassSpectral typechardecDeclination from input catalog (degree)pos.eq.decdoublegaia_source_idThe "source_id" field of Gaia DR3 catalogchargp_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 designationcharfibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charhalpha24Continuum luminosity in common logarithm at rest-frame 1350 Ådoublekp6Continuum luminosity in common logarithm at rest-frame 5100 Ådoublehalpha70The coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublerv_errSurface gravity uncertainty obtained by the LASPdoublemag_ps_rPan-STARRS r band magnitudedoublervEffective temperature uncertainty obtained by the LASPdoublemag_ps_gPan-STARRS g band magnitudedoublefibermaskSpectral sub-types of white dwarf starsintpaschen13Minimal chi-square in the fitting of the second group linesdoublemag_ps_zPan-STARRS z band magnitudedoublelogg_errAlpha element abundance estimated by the LASPdoublesnrgS/N of g filterdoublesnruS/N of u filterdoubleps_idThe objID in the Pan-STARRS cataloglonghgamma54Reduced chi-square in the fitting of the first group linesdoubleraRight ascension from input catalog (degree)pos.eq.radoublehbeta12The 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.prodoubleoffsetsWhether 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)doublesubclassStellar spectral typecharuidUnique source identifier calculated with the "ura" and "udec" in table 9chardec_obsFiber pointing declination (degree)doubleobsidUnique spectrum ID for each observation of each targetmeta.idlongbalmer_teffElectron temperatureintciii_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_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_sigmaLine dispersion in natural logarithm of the second CIII narrow componentintciv_areaIntegrated Flux of entire C IVdoubleciv_na_1_sigmaLine dispersion in natural logarithm of CIV narrow componentdoublefe_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_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.intcah2_errLine dispersion in natural logarithm of the first C III broad componentdoublefitting_status_3FWHM of entire C IIIintciv_na_1_peak_wavelengthPeak flux of Halpha narrow componentdoublewith_norm_fluxEffective temperature obtained by the LASPintfitting_status_4Peak wavelenth of entire C IVintfe_uv_fwhmLine dispersion of entire Halphadoublecaoh_errDegree of freedom in the fitting of the sixth group linesdoublebalmer_normLine dispersion in natural logarithm of [N II] 6585doubleha_br_2_peak_fluxPeak flux of the second Halpha broad componentdoubleha_br_3_peak_fluxPeak flux of Halpha broad componentdoubleha_br_3_peak_wavelengthPeak wavelength in natural logarithm of the third Halpha broad componentdoubleha_na_1_peak_wavelengthPeak wavelength in natural logarithm of Halpha narrow componentdoublehb_areaIntegrated Flux of entire Hbetadoublehb_br_1_peak_wavelengthPeak wavelength in natural logarithm of Hbeta broad componentdoublehb_sigmaLine dispersion of entire Hbetadoubleha_br_1_peak_wavelengthEW of entire Halphadoublehalpha_ewLine dispersion in natural logarithm of Hbeta narrow componentdoublehbeta60The name of the first group of spectral linesdoublehdelta12The name of the second group of spectral linesdoublehalpha12Minimal chi-square in the fitting of the fourth group linesdoublehb_na_1_peak_wavelengthPeak flux of [S II] 6718doublel1350Continuum luminosity in common logarithm at rest-frame 1350 Ådoubleline_name_2The name of the second group of spectral linescharline_name_6The name of the sixth group of spectral linescharlya_na_1_peak_fluxPeak flux of Lya narrow componentdoublelya_na_1_peak_wavelengthPeak wavelength in natural logarithm of Lya narrow componentdoublemgii_br_1_peak_fluxPeak flux of Mg II broad componentdoublemgii_na_1_peak_fluxPeak flux of the first Mg II narrow componentdoublemgii_na_2_peak_wavelengthPeak wavelength in natural logarithm of the second Mg II narrow componentdoublemin_chi2_5Minimal chi-square in the fitting of the fifth group linesintnii6549_1_peak_fluxPeak flux of [N II] 6549doublenii6585_1_peak_wavelengthPeak wavelength in natural logarithm of [N II] 6585doublepoly_aThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublepoly_cThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublered_chi2_1Reduced chi-square in the fitting of the first group linesdoubleline_name_3Line dispersion of entire C IVcharmgii_na_2_sigmaPeak flux of [N II] 6585doublendof_4Peak wavelength in natural logarithm of the third Halpha broad componentintpaschen242Reduced chi-square in the fitting of the third group linesdoublekp12Degree of freedom in the fitting of the third group linesdoublem_h_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.doublered_chi2_3Peak wavelength in natural logarithm of [N II] 6585doublemgii_na_1_sigmaLine dispersion in natural logarithm of the third Halpha broad componentdoubleoiii4959_1_peak_wavelengthPeak wavelenth of entire Halphadoublenii_6550_fluxPeak wavelength in natural logarithm of Hbeta broad componentdoubleoiii_4960_ewPeak flux of Hbeta narrow componentdoublemetal_mwPeak wavelength in natural logarithm of Hbeta narrow componentdoublenii6549_1_peak_wavelengthFWHM of entire Mg IIdoublemin_chi2_6Peak wavelenth of entire Mg IIintoiii_5008_fluxPeak wavelength in natural logarithm of [O III] 5007doublered_chi2_6Reduced chi-square in the fitting of the sixth group linesintsii6732_1_peak_wavelengthPeak wavelength in natural logarithm of [S II] 6732doublesii_6733_ewPeak flux of the second Mg II narrow componentdoubletio4Minimal chi-square in the fitting of the sixth group linesdoublevsigLine dispersion in natural logarithm of [O III] 5007doublewd_subclassLine dispersion in natural logarithm of the second CIII narrow componentchartio2Peak wavelength in natural logarithm of C IV narrow componentdoublesii6718_1_peak_wavelengthLine dispersion in natural logarithm of Halpha narrow componentdoublezRedshiftdoublez_errRedshift uncertaintydoublemag_ps_iPan-STARRS i band magnitudedoublehgamma24Continuum luminosity in common logarithm at rest-frame 3000 Ådoublegaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublesnriS/N of i filterdoublehbeta_d02Degree of freedom in the fitting of the fourth group linesdoublesnrzS/N of z filterdoublepaschen142The name of the first group of spectral linesdoublezeta_errPeak wavelength in natural logarithm of C IV broad componentdoublehgamma48The 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.doublehdelta64The 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.doublekp18Reduced chi-square in the fitting of the fourth group linesdoubletypeReduced chi-square in the fitting of the fifth group linesdoublenii_6550_ewLine dispersion in natural logarithm of Hbeta broad componentdoubleoiii_5008_ewPeak wavelength in natural logarithm of Mg II broad componentdoublehbeta_fluxLine dispersion in natural logarithm of the second Mg II narrow componentdouble
public.catalogueoffsetsWhether there is a fiber offset during observationintgaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublesnrgS/N of g filterdoublezRedshiftdoublesnriS/N of i filterdoublez_errRedshift uncertaintydoublesnrrS/N of r filterdoublesubclassStellar spectral typecharmag_ps_yPan-STARRS y band magnitudedoublemag_ps_iPan-STARRS i band magnitudedoubledecDeclination from input catalog (degree)pos.eq.decdoublemag_ps_zPan-STARRS z band magnitudedoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charmag_ps_rPan-STARRS r band magnitudedoubleps_idThe objID in the Pan-STARRS cataloglongraRight ascension from input catalog (degree)pos.eq.radoublesnrzS/N of z filterdoublefibermaskSpectral sub-types of white dwarf starsintwith_norm_fluxEffective temperature obtained by the LASPintgaia_source_idThe "source_id" field of Gaia DR3 catalogcharobsdateTarget observation datecharmjdModified Julian daytime.epochintplanidPlan namecharra_obsFiber pointing right ascension (degree)doubledec_obsFiber pointing declination (degree)doubledesignationTarget designationcharspidSpectrograph IDintoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublelmjdLocal modified Julian daytime.epochintobsidUnique spectrum ID for each observation of each targetmeta.idlongsnruS/N of u filterdoubleuidUnique source identifier calculated with the "ura" and "udec" in table 9charfiberidFiber IDintmag_ps_gPan-STARRS g band magnitudedoubleclassSpectral 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.long
public.stellardec_obsFiber pointing declination (degree)doublemjdModified Julian daytime.epochintfiberidFiber IDintplanidPlan namecharobsidUnique spectrum ID for each observation of each targetmeta.idlongspidSpectrograph IDintsnruS/N of u filterdoublera_obsFiber pointing right ascension (degree)doubleobsdateTarget observation datecharuidUnique source identifier calculated with the "ura" and "udec" in table 9charmag_ps_yPan-STARRS y band magnitudedoublevsini_laspProjected rotation velocity given by the LASPdoublealpha_mAlpha element abundance estimated by the LASPdoublelogg_errSurface gravity obtained by the LASPdoublefeh_errMetallicity uncertainty obtained by the LASPdoubledecDeclination from input catalog (degree)pos.eq.decdoublealpha_m_errThe uncertainty of alpha_mdoubleteffSpectral sub-types of white dwarf starsdoublefehSurface gravity uncertainty obtained by the LASPdoublervHeliocentric radial velocity obtained by the LASPdoubleloggEffective temperature uncertainty obtained by the LASPdoublegaia_source_idThe "source_id" field of Gaia DR3 catalogcharfibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charlmjdLocal modified Julian daytime.epochintmag_ps_rPan-STARRS r band magnitudedoublerv_errUncertainty of heliocentric radial velocity obtained by the LASPdoublemag_ps_zPan-STARRS z band magnitudedoublemag_ps_gPan-STARRS g band magnitudedoublesnrgS/N of g filterdoublesnrzS/N of z filterdoubleps_idThe objID in the Pan-STARRS cataloglongraRight ascension from input catalog (degree)pos.eq.radoubleoffsetsWhether 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)doublesubclassStellar spectral typecharz_errRedshift uncertaintydoublegaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublegp_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.longteff_errEffective temperature obtained by the LASPdoublemag_ps_iPan-STARRS i band magnitudedoubleclassSpectral typecharsnriS/N of i filterdoublesnrrS/N of r filterdoublezRedshiftdoubledesignationTarget designationchar
public.astellaroffsetsWhether there is a fiber offset during observationinthdelta24Surface gravity uncertainty obtained by the LASPdoubleobsdateTarget observation datecharraRight ascension from input catalog (degree)pos.eq.radoublehdelta48Metallicity uncertainty obtained by the LASPdoublehgamma12Uncertainty of heliocentric radial velocity obtained by the LASPdoublehgamma24Alpha element abundance estimated by the LASPdoublekp12Spectral sub-types of white dwarf starsdoubleplanidPlan namechargaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublespidSpectrograph IDintgaia_source_idThe "source_id" field of Gaia DR3 catalogcharsnrrS/N of r filterdoublesnrgS/N of g filterdoublehgamma54Projected rotation velocity given by the LASPdoublekp6Effective temperature uncertainty obtained by the LASPdoublezRedshiftdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charmag_ps_iPan-STARRS i band magnitudedoublemag_ps_yPan-STARRS y band magnitudedoublehgamma_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.doublehalpha48Continuum luminosity in common logarithm at rest-frame 5100 Ådoublehbeta24The coefficient of the first term of the third-order polynomial in the continuum fittingdoublehalpha70The name of the first group of spectral linesdoublehdelta_d02Minimal chi-square in the fitting of the second group linesdoublehalpha12Continuum luminosity in common logarithm at rest-frame 1350 Ådoublehbeta48The coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublehbeta12Optical depth at the Balmer edge of 3646 Ådoublehalpha_d02Degree of freedom in the fitting of the first group linesdoublehbeta_d02The name of the second 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.prodoublehbeta60The coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublepaschen242Reduced chi-square in the fitting of the first group linesdoublehdelta64Heliocentric radial velocity obtained by the LASPdoubledec_obsFiber pointing declination (degree)doublefiberidFiber IDinthdelta12Surface gravity obtained by the LASPdoublemag_ps_rPan-STARRS r band magnitudedoublekp18Effective temperature obtained by the LASPdoublehgamma48The uncertainty of alpha_mdoublesnriS/N of i filterdoubleps_idThe objID in the Pan-STARRS cataloglongra_obsFiber pointing right ascension (degree)doublesubclassStellar spectral typecharclassSpectral typecharlmjdLocal modified Julian daytime.epochintobsidUnique 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)doublesnrzS/N of z filterdoubleuidUnique source identifier calculated with the "ura" and "udec" in table 9chargp_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.longz_errRedshift uncertaintydoublemjdModified Julian daytime.epochinthalpha24Continuum luminosity in common logarithm at rest-frame 3000 Ådoublemag_ps_zPan-STARRS z band magnitudedoublepaschen142Minimal chi-square in the fitting of the first group linesdoublesnruS/N of u filterdoubledecDeclination from input catalog (degree)pos.eq.decdoubledesignationTarget designationcharmag_ps_gPan-STARRS g band magnitudedouble
public.mstellarra_obsFiber pointing right ascension (degree)doubleobsdateTarget observation datecharlmjdLocal modified Julian daytime.epochintmjdModified Julian daytime.epochintfiberidFiber IDintspidSpectrograph IDintsnruS/N of u filterdoubleplanidPlan namecharmag_ps_rPan-STARRS r band magnitudedoublenaThe 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.doublelogg_errSurface gravity obtained by the LASPdoublezetaReduced chi-square in the fitting of the second group linesdoubletio5Alpha element abundance estimated by the LASPdoublecah1Continuum luminosity in common logarithm at rest-frame 1350 Ådoublemag_ps_zPan-STARRS z band magnitudedoubletio3The coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublecah2_errThe name of the first group of spectral linesdoublesnriS/N of i filterdoubletio1Optical depth at the Balmer edge of 3646 Ådoublem_hSurface gravity uncertainty obtained by the LASPdoublez_errRedshift uncertaintydoubletio4The coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublezeta_errDegree of freedom in the fitting of the second group linesdoublesnrrS/N of r filterdoubleps_idThe objID in the Pan-STARRS cataloglongtypeThe name of the first group of spectral linesdoublemag_ps_yPan-STARRS y band magnitudedoublemag_ps_iPan-STARRS i band magnitudedoublemag_ps_gPan-STARRS g band magnitudedoubleraRight ascension from input catalog (degree)pos.eq.radoublegaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoubleewhaHeliocentric radial velocity obtained by the LASPdoubletio5_errContinuum luminosity in common logarithm at rest-frame 5100 Ådoublecah2The uncertainty of alpha_mdoublegaia_source_idThe "source_id" field of Gaia DR3 catalogcharewha_errUncertainty of heliocentric radial velocity obtained by the LASPdoubletio1_errMinimal chi-square in the fitting of the first group linesdoublezRedshiftdoublesnrzS/N of z filterdoublesnrgS/N of g filterdoubletio2_errReduced chi-square in the fitting of the first group 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.prodoublecah1_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.doublesubclassStellar spectral typechartio3_errDegree of freedom in the fitting of the first group linesdoubleloggEffective temperature uncertainty obtained by the LASPdoubledecDeclination from input catalog (degree)pos.eq.decdoubledec_obsFiber pointing declination (degree)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.longfibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]chartio4_errThe name of the second group of spectral linesdoubletio2The coefficient of the first term of the third-order polynomial in the continuum fittingdoublem_h_errMetallicity uncertainty obtained by the LASPdoublecaoh_errMinimal chi-square in the fitting of the second group linesdoublecah3Projected rotation velocity given by the LASPdoubleoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleuidUnique source identifier calculated with the "ura" and "udec" in table 9charteffSpectral sub-types of white dwarf starsdoubleobsidUnique spectrum ID for each observation of each targetmeta.idlongteff_errEffective temperature obtained by the LASPdoublecaohContinuum luminosity in common logarithm at rest-frame 3000 ÅdoubleoffsetsWhether there is a fiber offset during observationintclassSpectral typechardesignationTarget designationchar
public.cvobsdateTarget observation datecharzRedshiftdoublesubclassStellar spectral typecharperiodEffective temperature obtained by the LASPdoubleplanidPlan namecharra_obsFiber pointing right ascension (degree)doublemag_ps_yPan-STARRS y band magnitudedoublerEffective temperature uncertainty obtained by the LASPpos.eq.raintgaia_source_idThe "source_id" field of Gaia DR3 catalogcharabs_gmag_errSurface gravity uncertainty obtained by the LASPdoublesnrrS/N of r filterdoublez_errRedshift uncertaintydoubledecDeclination from input catalog (degree)pos.eq.decdoublemag_ps_zPan-STARRS z band magnitudedoubledec_obsFiber pointing declination (degree)doubleoffsetsWhether there is a fiber offset during observationintfiberidFiber IDintoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublelmjdLocal modified Julian daytime.epochintsnrgS/N of g filterdoublemag_ps_gPan-STARRS g band magnitudedoubledesignationTarget designationcharmag_ps_iPan-STARRS i band magnitudedoublesnriS/N of i filterdoubleuidUnique source identifier calculated with the "ura" and "udec" in table 9charsnruS/N of u filterdoubleabs_gmagSurface gravity obtained by the LASPdoublemjdModified Julian daytime.epochintps_idThe objID in the Pan-STARRS cataloglongsnrzS/N of z filterdoublemag_ps_rPan-STARRS r band magnitudedoubleraRight ascension from input catalog (degree)pos.eq.radoublespidSpectrograph IDintfibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]chargaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoubleclassSpectral 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.longsubtypeSpectral sub-types of white dwarf starscharobsidUnique spectrum ID for each observation of each targetmeta.idlong
public.wduidUnique source identifier calculated with the "ura" and "udec" in table 9chargaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublesnriS/N of i filterdoublemjdModified Julian daytime.epochintdec_obsFiber pointing declination (degree)doubledesignationTarget designationchargaia_source_idThe "source_id" field of Gaia DR3 catalogcharmag_ps_gPan-STARRS g band magnitudedoublespidSpectrograph IDintgp_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.longlmjdLocal modified Julian daytime.epochintoffsetsWhether there is a fiber offset during observationintobsdateTarget observation datecharoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doubleplanidPlan namecharps_idThe objID in the Pan-STARRS cataloglongwd_subclassSpectral sub-types of white dwarf starscharobsidUnique spectrum ID for each observation of each targetmeta.idlongraRight ascension from input catalog (degree)pos.eq.radoublemag_ps_iPan-STARRS i band magnitudedoublefiberidFiber IDintmag_ps_rPan-STARRS r band magnitudedoublesnrrS/N of r filterdoublezRedshiftdoublera_obsFiber pointing right ascension (degree)doublesubclassStellar spectral typecharloggSurface gravity obtained by the LASPdoublesnrgS/N of g filterdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charmag_ps_yPan-STARRS y band magnitudedoublesnruS/N of u filterdoubleteffEffective temperature obtained by the LASPdoublez_errRedshift uncertaintydoublelogg_errSurface gravity uncertainty obtained by the LASPdoubleteff_errEffective temperature uncertainty obtained by the LASPdoublemag_ps_zPan-STARRS z band magnitudedoublesnrzS/N of z filterdoubledecDeclination from input catalog (degree)pos.eq.decdoubleclassSpectral typechar
public.qsoline_name_3The name of the first group of spectral linescharra_obsFiber pointing right ascension (degree)doublefe_op_normSurface gravity uncertainty obtained by the LASPdoublemag_ps_yPan-STARRS y band magnitudedoublesnrrS/N of r filterdoublezRedshiftdoublefe_op_fwhmMetallicity uncertainty obtained by the LASPdoublefe_uv_shiftSurface gravity obtained by the LASPdoublered_chi2_2Reduced chi-square in the fitting of the second group linesdoublemag_ps_iPan-STARRS i band magnitudedoublegaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublemag_ps_zPan-STARRS z band magnitudedoubledecDeclination from input catalog (degree)pos.eq.decdoublesubclassStellar spectral typecharpl_normUncertainty of heliocentric radial velocity obtained by the LASPdoublesnrzS/N of z filterdoublesnriS/N of i filterdoublesnruS/N of u filterdoublemag_ps_rPan-STARRS r band magnitudedoubleraRight ascension from input catalog (degree)pos.eq.radoublepl_slopeAlpha element abundance estimated by the LASPdoublesnrgS/N of g filterdoublendof_1Degree of freedom in the fitting of the first group linesintndof_2Degree of freedom in the fitting of the second group linesintoffsetsWhether there is a fiber offset during observationintps_idThe objID in the Pan-STARRS cataloglongfiberidFiber IDintmag_ps_gPan-STARRS g band magnitudedoublebalmer_teffProjected rotation velocity given by the LASPintsn_ratio_contiSpectral sub-types of white dwarf starsdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charplanidPlan namecharmgii_br_1_peak_wavelengthPeak wavelength in natural logarithm of Mg II broad componentdoublemgii_br_1_peak_fluxPeak flux of Mg II broad componentdoublenii6549_1_peak_fluxPeak flux of [N II] 6549doubleciv_na_1_sigmaLine dispersion in natural logarithm of CIV narrow componentdoubleciv_na_1_peak_fluxPeak flux of C IV narrow componentdoubleciii_br_1_peak_wavelengthPeak wavelength in natural logarithm of the first C III broad componentdoublered_chi2_6Reduced chi-square in the fitting of the sixth group linesintnii6549_1_peak_wavelengthPeak wavelength in natural logarithm of [N II] 6549doubleha_br_2_peak_wavelengthPeak wavelength in natural logarithm of the second Halpha broad componentdoubleha_br_1_sigmaLine dispersion in natural logarithm of the first Halpha broad componentdoublelya_na_1_peak_wavelengthPeak wavelength in natural logarithm of Lya narrow componentdoubleciii_br_2_peak_fluxPeak flux of the second C III broad componentdoubleha_br_2_sigmaLine dispersion in natural logarithm of the second Halpha broad componentdoubleha_br_1_peak_wavelengthPeak wavelength in natural logarithm of the first Halpha broad componentdoublelya_br_1_peak_fluxPeak flux of Lya broad componentdoubleline_name_4The name of the fourth group of spectral linescharhb_br_1_peak_wavelengthPeak wavelength in natural logarithm of Hbeta broad componentdoublefitting_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.intmgii_na_1_peak_wavelengthPeak wavelength in natural logarithm of the first Mg II narrow componentdoublendof_5Degree of freedom in the fitting of the fifth group linesintndof_6Degree of freedom in the fitting of the sixth group linesintline_name_6The name of the sixth group of spectral linescharha_na_1_peak_wavelengthPeak wavelength in natural logarithm of Halpha narrow componentdoublehb_na_1_sigmaLine dispersion in natural logarithm of Hbeta narrow componentdoublenii6585_1_peak_fluxPeak flux of [N II] 6585doublenii6585_1_peak_wavelengthPeak wavelength in natural logarithm of [N II] 6585doubleciii_na_1_peak_fluxPeak flux of the first C III narrow componentintha_br_2_peak_fluxPeak flux of the second Halpha broad componentdoublelya_br_1_sigmaLine dispersion in natural logarithm of Lya broad componentdoublehb_na_1_peak_fluxPeak flux of Hbeta narrow componentdoublehb_br_1_sigmaLine dispersion in natural logarithm of Hbeta broad componentdoubleoiii5007_1_peak_wavelengthPeak wavelength in natural logarithm of [O III] 5007doublehb_na_1_peak_wavelengthPeak wavelength in natural logarithm of Hbeta narrow componentdoublemgii_na_1_peak_fluxPeak flux of the first Mg II narrow componentdoubleoiii5007_1_sigmaLine dispersion in natural logarithm of [O III] 5007doubleoiii5007_1_peak_fluxPeak flux of [O III] 5007doublemgii_na_2_peak_fluxPeak flux of the second Mg II narrow componentdoublemgii_na_1_sigmaLine dispersion in natural logarithm of the first Mg II narrow componentdoublemin_chi2_6Minimal chi-square in the fitting of the sixth group linesintciii_br_2_peak_wavelengthPeak wavelength in natural logarithm of the second C III broad componentdoublelya_na_1_peak_fluxPeak flux of Lya narrow componentdoublered_chi2_4Reduced chi-square in the fitting of the fourth group linesdoubleciii_br_1_peak_fluxPeak flux of the first C III broad componentdoubleciii_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 componentintciv_br_1_peak_fluxPeak flux of CIV broad componentdoubleciii_na_2_peak_fluxPeak flux of the second C III narrow componentintciii_na_2_sigmaLine dispersion in natural logarithm of the second CIII narrow componentintmgii_fwhmFWHM of entire Mg IIdoubleciv_sigmaLine dispersion of entire C IVdoublemgii_sigmaLine dispersion of entire Mg IIdoubleciii_sigmaLine dispersion of entire C IIIdoubleha_fwhmFWHM of entire Halphadoublesii6718_1_peak_wavelengthPeak wavelength in natural logarithm of [S II] 6718doublesii6732_1_peak_fluxPeak flux of [S II] 6732doublehb_fwhmFWHM of entire Hbetadoubleciii_ewEW of entire C IIIdoubleciii_peak_wavelengthPeak wavelenth of entire C IIIdoubleha_sigmaLine dispersion of entire Halphadoublelya_areaIntegrated Flux of entire Lyadoublesii6732_1_peak_wavelengthPeak wavelength in natural logarithm of [S II] 6732doublelya_ewEW of entire Lyadoubleha_ewEW of entire Halphadoublemgii_areaIntegrated Flux of entire Mg IIdoublehb_peak_wavelengthPeak wavelenth of entire Hbetadoubleciii_areaIntegrated Flux of entire C IIIdoubleha_peak_wavelengthPeak wavelenth of entire Halphadoublemgii_ewEW of entire Mg IIdoublehb_sigmaLine dispersion of entire Hbetadoublehb_areaIntegrated Flux of entire Hbetadoubleciv_ewEW of entire C IVdoubleciv_peak_wavelengthPeak wavelenth of entire C IVdoublehb_ewEW of entire Hbetadoublesii6718_1_peak_fluxPeak flux of [S II] 6718doublegaia_source_idThe "source_id" field of Gaia DR3 catalogchardec_obsFiber pointing declination (degree)doublel5100Continuum luminosity in common logarithm at rest-frame 5100 Ådoubleline_name_1The name of the first group of spectral linescharline_name_2The name of the second group of spectral linescharpoly_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 fittingdoublebalmer_tau_eOptical depth at the Balmer edge of 3646 Ådoublefe_op_shiftHeliocentric radial velocity obtained by the LASPdoublefitting_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.intobsdateTarget observation datecharmjdModified Julian daytime.epochintred_chi2_1Reduced chi-square in the fitting of the first group linesdoublefitting_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.prointmin_chi2_1Minimal chi-square in the fitting of the first group linesdoubleclassSpectral typecharlmjdLocal modified Julian daytime.epochintoffsets_vIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublespidSpectrograph IDintciii_br_1_sigmaLine dispersion in natural logarithm of the first C III broad componentdoubleciii_fwhmFWHM of entire C IIIdoubleha_br_3_peak_fluxPeak flux of Halpha broad componentdoubleha_na_1_peak_fluxPeak flux of Halpha narrow componentdoubleciv_fwhmFWHM of entire C IVdoublefe_uv_normEffective temperature obtained by the LASPdoublelya_peak_wavelengthPeak wavelenth of entire Lyadoublemgii_na_2_peak_wavelengthPeak wavelength in natural logarithm of the second Mg II narrow componentdoublenii6549_1_sigmaLine dispersion in natural logarithm of [N II] 6549doublenii6585_1_sigmaLine dispersion in natural logarithm of [N II] 6585doubleciv_areaIntegrated Flux of entire C IVdoubleha_areaIntegrated Flux of entire Halphadoublehb_br_1_peak_fluxPeak flux of Hbeta broad componentdoubleline_name_5The name of the fifth group of spectral linescharmgii_na_2_sigmaLine dispersion in natural logarithm of the second Mg II narrow componentdoublemin_chi2_3Minimal chi-square in the fitting of the third group linesdoublemgii_br_1_sigmaLine dispersion in natural logarithm of Mg II broad componentdoubleoiii4959_1_peak_wavelengthPeak wavelength in natural logarithm of [O III] 4959doublesii6732_1_sigmaLine dispersion in natural logarithm of [S II] 6732doublebalmer_normThe uncertainty of alpha_mdoubleha_br_3_peak_wavelengthPeak wavelength in natural logarithm of the third Halpha broad componentdoubleha_br_3_sigmaLine dispersion in natural logarithm of the third Halpha broad componentdoublelya_fwhmFWHM of entire Lyadoublelya_sigmaLine dispersion of entire Lyadoublemgii_peak_wavelengthPeak wavelenth of entire Mg IIdoublemin_chi2_2Minimal chi-square in the fitting of the second group linesdoubleoiii4959_1_sigmaLine dispersion in natural logarithm of [O III] 4959doublered_chi2_3Reduced chi-square in the fitting of the third group linesdoubleoiii4959_1_peak_fluxPeak flux of [O III] 4959doublesii6718_1_sigmaLine dispersion in natural logarithm of [S II] 6718doubleciv_br_1_peak_wavelengthPeak wavelength in natural logarithm of C IV broad componentdoubleciv_br_1_sigmaLine dispersion in natural logarithm of C IV broad componentdoubleha_br_1_peak_fluxPeak flux of the first Halpha broad componentdoubleha_na_1_sigmaLine dispersion in natural logarithm of Halpha narrow componentdoublelya_br_1_peak_wavelengthPeak wavelength in natural logarithm of Lya broad componentdoubleobsidUnique spectrum ID for each observation of each targetmeta.idlonguidUnique source identifier calculated with the "ura" and "udec" in table 9charz_errRedshift uncertaintydoublel1350Continuum luminosity in common logarithm at rest-frame 1350 Ådoublefe_uv_fwhmEffective temperature uncertainty obtained by the LASPdoublel3000Continuum luminosity in common logarithm at rest-frame 3000 Ådoublemin_chi2_4Minimal chi-square in the fitting of the fourth group linesdoublendof_3Degree of freedom in the fitting of the third group linesintpoly_cThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoubleciii_na_2_peak_wavelengthPeak wavelength in natural logarithm of the second C III narrow componentintciv_na_1_peak_wavelengthPeak wavelength in natural logarithm of C IV narrow componentdoublendof_4Degree of freedom in the fitting of the fourth group linesintfitting_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.intlya_na_1_sigmaLine dispersion in natural logarithm of Lya narrow componentdoublegp_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.longmin_chi2_5Minimal chi-square in the fitting of the fifth group linesintred_chi2_5Reduced chi-square in the fitting of the fifth group linesintfitting_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.intfitting_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.intdesignationTarget designationchar
public.galaxyobsdateTarget observation datecharuidUnique source identifier calculated with the "ura" and "udec" in table 9charsnruS/N of u filterdoublesnrgS/N of g filterdoubleplanidPlan namechargaia_source_idThe "source_id" field of Gaia DR3 catalogcharlmjdLocal modified Julian daytime.epochintmjdModified Julian daytime.epochintobsidUnique spectrum ID for each observation of each targetmeta.idlongsnriS/N of i filterdoublespidSpectrograph IDintra_obsFiber pointing right ascension (degree)doublesnrrS/N of r filterdoubledec_obsFiber pointing declination (degree)doublefiberidFiber IDintsii_6733_ewContinuum luminosity in common logarithm at rest-frame 1350 Ådoublemetal_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.prodoubleage_mwContinuum luminosity in common logarithm at rest-frame 5100 Ådoublesii_6718_ewThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingdoublevsigMinimal chi-square in the fitting of the first group linesdoublesii_6733_fluxThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublegaia_g_mean_magThe "phot_g_mean_mag" field of Gaia DR3 catalogdoubleclassSpectral typechardecDeclination from input catalog (degree)pos.eq.decdoublefibertypeFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]charnii_6550_fluxHeliocentric radial velocity obtained by the LASPdoublesii_6718_fluxThe coefficient of the first term of the third-order polynomial in the continuum fittingdoubleoiii_4960_ewSurface gravity obtained by the LASPdoubleoiii_5008_fluxSurface gravity uncertainty obtained by the LASPdoublenii_6585_ewOptical depth at the Balmer edge of 3646 Ådoublemag_ps_iPan-STARRS i band magnitudedoublemag_ps_rPan-STARRS r band magnitudedoublenii_6550_ewUncertainty of heliocentric radial velocity obtained by the LASPdoublehbeta_ewEffective temperature obtained by the LASPdoublenii_6585_fluxProjected rotation velocity given by the LASPdoublehalpha_ewThe uncertainty of alpha_mdoubleps_idThe objID in the Pan-STARRS cataloglongvsig_errReduced chi-square in the fitting of the first group linesdoubleraRight ascension from input catalog (degree)pos.eq.radoubleoffsetsWhether there is a fiber offset during observationintsubclassStellar spectral typecharhbeta_fluxSpectral sub-types of white dwarf starsdoublezRedshiftdoublesnrzS/N of z filterdoublez_errRedshift uncertaintydoubleoffsets_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.longage_lwContinuum luminosity in common logarithm at rest-frame 3000 Ådoublemag_ps_gPan-STARRS g band magnitudedoublemag_ps_zPan-STARRS z band magnitudedoublehalpha_fluxAlpha element abundance estimated by the LASPdoublemetal_lwThe name of the first group of spectral linesdoubleoiii_4960_fluxEffective temperature uncertainty obtained by the LASPdoubleoiii_5008_ewMetallicity uncertainty obtained by the LASPdoublemag_ps_yPan-STARRS y band magnitudedoubledesignationTarget designationchar
public.mecteff_listSpectrograph IDcharobsid_listLocal modified Julian daycharobs_numberTarget observation dateintlogg_listFiber IDcharuidUnique spectrum ID for each observation of each targetcharuraUnique source identifier calculated with the "ura" and "udec" in table 9doublez_listPlan namechargaia_vari_type_sosS/N of u filtercharrv_listFiber pointing declination (degree)charfeh_listFiber pointing right ascension (degree)charmidmjm_listModified Julian daychargp_idTarget designationlongudecFor 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.double
public.plandecTarget observation datepos.eq.decdoubleexptimePlan namecharlmjmSpectrograph IDlongmagLocal modified Julian daydoubleobsdateUnique source identifier calculated with the "ura" and "udec" in table 9charpidUnique spectrum ID for each observation of each targetintplanidFor 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.charraTarget designationpos.eq.radoubleseeingModified Julian daydouble
public.inputcatalogoffsets_vPan-STARRS g band magnitudedoubledecPan-STARRS i band magnitudepos.eq.decdoubleraPan-STARRS r band magnitudepos.eq.radoubleoffsetsThe objID in the Pan-STARRS catalogintunitidLocal modified Julian daycharfiberidTarget observation dateinttcommentRedshift uncertaintycharmag3S/N of u filterdoubleobsdateUnique source identifier calculated with the "ura" and "udec" in table 9charmag1Fiber pointing right ascension (degree)doublemag6S/N of i filterdoublemag4S/N of g filterdoubleepochPan-STARRS z band magnitudecharobjtypeSpectrograph IDcharobsidUnique spectrum ID for each observation of each targetmeta.idlongdec_obsPlan namedoublera_obsModified Julian daydoublefibertypeStellar spectral typecharmag7S/N of z filterdoublemagtypeFiber IDcharmag5S/N of r filterdoubletfromRedshiftcharmag2Fiber pointing declination (degree)doubletnamePan-STARRS y band magnitudechartsourceSpectral typecharplanidFor 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.charspidTarget designationint
public.med_combinedteff_cnnThe name of the second group of spectral linesdoublegaia_rp_mean_magRedshiftdoublegaia_source_idS/N of z filtercharalpha_m_laspThe name of the first group of spectral linesdoublebandS/N of u filtercharc_feMinimal chi-square in the fitting of the third group linesdoubleca_feDegree of freedom in the fitting of the second group linesdoubleni_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.doublerv_r1Right ascension from input catalog (degree)doublerv_b0_errPan-STARRS y band magnitudedoubleplanidSpectrograph IDcharbad_rThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingintraPan-STARRS r band magnitudepos.eq.radoubledec_obsS/N of r filterdoubleobsdateLocal modified Julian daycharm_h_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.doublelogg_lasp_errReduced chi-square in the fitting of the third group linesdoublefeh_cnnThe name of the fourth group of spectral linesdoubleti_feDegree of freedom in the fitting of the first group linesdoubleobsidUnique source identifier calculated with the "ura" and "udec" in table 9meta.idlonglogg_cnnDegree of freedom in the fitting of the third group linesdoublespidFiber IDintlunardateContinuum luminosity in common logarithm at rest-frame 1350 Åints_feThe name of the first group of spectral linesdoublelmjdModified Julian daytime.epochintrv_b1The "source_id" field of Gaia DR3 catalogdoublerv_r0Whether there is a fiber offset during observationdoublesnrS/N of i filterdoublemjdPlan nametime.epochintteff_lasp_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.prodoubledesignationTarget observation datecharlogg_laspMinimal chi-square in the fitting of the second group linesdoublera_obsS/N of g filterdoublealpha_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.doubledecPan-STARRS i band magnitudepos.eq.decdoublevsini_lasp_errReduced chi-square in the fitting of the second group linesdoublelmjmFiber pointing declination (degree)longoffsets_vPan-STARRS g band magnitudedoublerv_b1_errThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublecu_feDegree of freedom in the fitting of the fourth group linesdoublemg_feMinimal chi-square in the fitting of the fourth group linesdoublegaia_vari_type_sosMinimal chi-square in the fitting of the sixth group linescharfeh_laspThe name of the fifth group of spectral linesdoublespecPeak flux of Lya broad componentmeta.idcharfeh_lasp_errDegree of freedom in the fitting of the fifth group linesdoublecr_feReduced chi-square in the fitting of the fifth group linesdoublealpha_m_cnnReduced chi-square in the fitting of the fourth group linesdoubleteff_laspMinimal chi-square in the fitting of the fifth group linesdoublesi_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.doublen_feThe 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.doublefileDegree of freedom in the fitting of the sixth group linescharo_feThe name of the sixth group of spectral linesdoublerv_r1_errDeclination from input catalog (degree)doublerv_b_flagFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]intsubprojectContinuum luminosity in common logarithm at rest-frame 5100 Åcharmoon_angleThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublerv_br1Surface gravity obtained by the LASPdoublerv_br1_errSurface gravity uncertainty obtained by the LASPdoublerv_br_flagMetallicity uncertainty obtained by the LASPintfibermaskOptical depth at the Balmer edge of 3646 Åintrv_br0_errEffective temperature uncertainty obtained by the LASPdoublerv_lasp0_errUncertainty of heliocentric radial velocity obtained by the LASPdoublerv_b0Pan-STARRS z band magnitudedoublecoaddProjected rotation velocity given by the LASPintrv_lasp1_errThe uncertainty of alpha_mdoublevsini_laspReduced chi-square in the fitting of the first group linesdoublefiberidFiber pointing right ascension (degree)intrv_r0_errIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublegaia_bp_mean_magStellar spectral typedoublerv_r_flagSpectral sub-types of white dwarf starsintfibertypeRedshift uncertaintycharuidFor 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.charmobsidUnique spectrum ID for each observation of each targetcharrv_br0Effective temperature obtained by the LASPdoubleoffsetsThe objID in the Pan-STARRS catalogintrv_lasp1Alpha element abundance estimated by the LASPdoublegaia_g_mean_magSpectral typedoublemoon_flgContinuum luminosity in common logarithm at rest-frame 3000 Åcharrv_lasp0Heliocentric radial velocity obtained by the LASPdoubleal_feMinimal chi-square in the fitting of the first group linesdoublegp_idTarget designationlongbad_bThe coefficient of the first term of the third-order polynomial in the continuum fittingint
public.med_cataloguedec_obsS/N of r filterdoublespidFiber IDintoffsets_vPan-STARRS g band magnitudedoublebad_rThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingintcoaddProjected rotation velocity given by the LASPintrv_r0_errIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublerv_lasp0_errUncertainty of heliocentric radial velocity obtained by the LASPdoublerv_b1The "source_id" field of Gaia DR3 catalogdoublerv_lasp1_errThe uncertainty of alpha_mdoubledecPan-STARRS i band magnitudepos.eq.decdoublerv_b_flagFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]intoffsetsThe objID in the Pan-STARRS catalogintraPan-STARRS r band magnitudepos.eq.radoublerv_b0_errPan-STARRS y band magnitudedoublefibermaskOptical depth at the Balmer edge of 3646 Åintgaia_bp_mean_magStellar spectral typedoublesubprojectContinuum luminosity in common logarithm at rest-frame 5100 Åchargaia_source_idS/N of z filtercharrv_r1_errDeclination from input catalog (degree)doublerv_r_flagSpectral sub-types of white dwarf starsintrv_b0Pan-STARRS z band magnitudedoublegaia_rp_mean_magRedshiftdoublerv_r1Right ascension from input catalog (degree)doublerv_r0Whether there is a fiber offset during observationdoublelunardateContinuum luminosity in common logarithm at rest-frame 1350 Åintrv_br0Effective temperature obtained by the LASPdoublerv_br0_errEffective temperature uncertainty obtained by the LASPdoublefibertypeRedshift uncertaintycharrv_b1_errThe "phot_g_mean_mag" field of Gaia DR3 catalogdoublerv_lasp1Alpha element abundance estimated by the LASPdoublerv_lasp0Heliocentric radial velocity obtained by the LASPdoublerv_br_flagMetallicity uncertainty obtained by the LASPintrv_br1Surface gravity obtained by the LASPdoublebad_bThe coefficient of the first term of the third-order polynomial in the continuum fittingintrv_br1_errSurface gravity uncertainty obtained by the LASPdoublelmjmFiber pointing declination (degree)longgp_idTarget designationlongmoon_angleThe coefficient of the cubic term of the third-order polynomial in the continuum fittingdoubledesignationTarget observation datecharsnrS/N of i filterdoublemjdPlan nametime.epochintgaia_g_mean_magSpectral typedoubleobsidUnique source identifier calculated with the "ura" and "udec" in table 9meta.idlongobsdateLocal modified Julian daycharlmjdModified Julian daytime.epochintmobsidUnique spectrum ID for each observation of each targetcharplanidSpectrograph IDcharfiberidFiber pointing right ascension (degree)intmoon_flgContinuum luminosity in common logarithm at rest-frame 3000 Åcharra_obsS/N of g filterdoublebandS/N of u filtercharuidFor 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_stellarrv_b_flagSurface gravity obtained by the LASPintrv_b0Declination from input catalog (degree)doublerv_r0Surface gravity uncertainty obtained by the LASPdoublerv_b0_errSpectral sub-types of white dwarf starsdoublefeh_lasp_errWhether there is a fiber offset during observationdoublelogg_laspThe "source_id" field of Gaia DR3 catalogdoubleti_feThe name of the fourth group of spectral linesdoublefeh_laspFiber type of target [Obj, Sky, F-std, Unused, PosErr, Dead]doublevsini_lasp_errRight ascension from input catalog (degree)doublelogg_lasp_errThe "phot_g_mean_mag" field of Gaia DR3 catalogdoubledesignationTarget observation datecharmjdPlan nametime.epochintgaia_source_idS/N of z filtercharraPan-STARRS r band magnitudepos.eq.radoublerv_lasp1_errContinuum luminosity in common logarithm at rest-frame 5100 Ådoublen_feReduced chi-square in the fitting of the second group linesdoublerv_lasp0The coefficient of the cubic term of the third-order polynomial in the continuum fittingdoublerv_r1Heliocentric radial velocity obtained by the LASPdoublefeh_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.doublerv_br0_errProjected rotation velocity given by the LASPdoublerv_lasp0_errContinuum luminosity in common logarithm at rest-frame 1350 Ådoubles_feReduced chi-square in the fitting of the third group linesdoublemg_feThe name of the first group of spectral linesdoublerv_r1_errUncertainty of heliocentric radial velocity obtained by the LASPdoublealpha_m_laspDegree of freedom in the fitting of the fourth group linesdoubleni_feMinimal chi-square in the fitting of the fourth group 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.doublecr_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.doublerv_r_flagAlpha element abundance estimated by the LASPinto_feDegree of freedom in the fitting of the second group linesdoublerv_br1Optical depth at the Balmer edge of 3646 Ådoublemoon_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.doublerv_lasp1Continuum luminosity in common logarithm at rest-frame 3000 ÅdoublelunardateMinimal chi-square in the fitting of the fifth group linesintteff_cnnDegree of freedom in the fitting of the first group linesdoublefibermaskThe 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.prointcu_feReduced chi-square in the fitting of the fourth group linesdoublecoaddThe name of the first group of spectral linesintrv_br1_errThe coefficient of the first term of the third-order polynomial in the continuum fittingdoublesi_feMinimal chi-square in the fitting of the third group linesdoublealpha_m_lasp_errThe name of the fifth group of spectral linesdoublerv_r0_errMetallicity uncertainty obtained by the LASPdoublerv_br_flagThe coefficient of the quadratic term of the third-order polynomial in the continuum fittingintm_h_cnnReduced chi-square in the fitting of the first group linesdoublelmjmFiber pointing declination (degree)longspidFiber IDintlogg_cnnThe name of the second group of spectral linesdoubledecPan-STARRS i band magnitudepos.eq.decdoubleobsdateLocal modified Julian daycharrv_b1_errEffective temperature uncertainty obtained by the LASPdoubleteff_lasp_errPan-STARRS y band magnitudedoublelmjdModified Julian daytime.epochintc_feMinimal chi-square in the fitting of the second group linesdoublerv_br0The uncertainty of alpha_mdoublera_obsS/N of g filterdoublebandS/N of u filtercharfiberidFiber pointing right ascension (degree)intplanidSpectrograph IDcharobsidUnique source identifier calculated with the "ura" and "udec" in table 9meta.idlonggaia_g_mean_magSpectral typedoublefibertypeRedshift uncertaintycharmobsidUnique spectrum ID for each observation of each targetchargaia_rp_mean_magRedshiftdoubleoffsets_vPan-STARRS g band magnitudedoubleca_feDegree of freedom in the fitting of the third group linesdoublerv_b1Effective temperature obtained by the LASPdoubleuidFor 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.charvsini_laspIf the "offsets" field is true, "offsets_v" gives the offset distance from the target"s coordinator in input catalog (arcsec)doublegaia_bp_mean_magStellar spectral typedoubleteff_laspPan-STARRS z band magnitudedoublesnrS/N of i filterdoublealpha_m_cnnMinimal chi-square in the fitting of the first group linesdoubledec_obsS/N of r filterdoublegp_idTarget designationlongoffsetsThe objID in the Pan-STARRS catalogintmoon_flgReduced chi-square in the fitting of the fifth group lineschar
public.med_mecrv_r1_listS/N of r filtercharrv_b1_listS/N of u filtercharlmjm_listFiber pointing right ascension (degree)charrv_br1_listS/N of z filtercharrv_r0_listS/N of g filtercharexp_numberFiber IDintrv_br0_listS/N of i filtercharrv_b0_listFiber pointing declination (degree)charobs_numberTarget observation dateintobsid_listLocal modified Julian daycharlogg_lasp_listPlan namecharfeh_lasp_listSpectrograph IDchargaia_vari_type_sosSpectral typecharuraUnique source identifier calculated with the "ura" and "udec" in table 9doubleudecFor 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.doubleteff_lasp_listModified Julian daychargp_idTarget designationlonguidUnique spectrum ID for each observation of each targetchar
public.med_plandecTarget observation datepos.eq.decdoubleexptimePlan namecharlmjm_listSpectrograph IDcharmagLocal modified Julian daydoubleobsdateUnique source identifier calculated with the "ura" and "udec" in table 9charpidUnique spectrum ID for each observation of each targetintplanidFor 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.charraTarget designationpos.eq.radoubleseeingModified Julian daydouble
public.med_inputcatalogobjtypeSpectrograph IDcharmag1Fiber pointing right ascension (degree)doubletnamePan-STARRS y band magnitudecharmag6S/N of i filterdoublemag4S/N of g filterdoublefiberidTarget observation dateinttfromRedshiftcharmagtypeFiber IDchartcommentRedshift uncertaintycharmag3S/N of u filterdoubleepochPan-STARRS z band magnitudecharraPan-STARRS r band magnitudepos.eq.radoubleobsdateUnique source identifier calculated with the "ura" and "udec" in table 9charmag7S/N of z filterdoublera_obsModified Julian daydoublemag5S/N of r filterdoubleoffsetsThe objID in the Pan-STARRS catalogintdecPan-STARRS i band magnitudepos.eq.decdoublemag2Fiber pointing declination (degree)doubledec_obsPlan namedoubleobsidUnique spectrum ID for each observation of each targetmeta.idlongfibertypeStellar spectral typechartsourceSpectral typecharplanidFor 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.charunitidLocal modified Julian daycharspidTarget designationintoffsets_vPan-STARRS g band magnitudedouble
tap_schematap_schema.schemasdescriptionTarget designationcharschema_indexUnique spectrum ID for each observation of each targetintschema_nameUnique source identifier calculated with the "ura" and "udec" in table 9charutypeFor 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
tap_schema.tablesdescriptionLocal modified Julian daycharschema_nameUnique source identifier calculated with the "ura" and "udec" in table 9chartable_indexUnique spectrum ID for each observation of each targetinttable_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.chartable_typeTarget designationcharutypeTarget observation datechar
tap_schema.schemas
schema_name
schema_name
tap_schema.columnsarraysizeLocal modified Julian daycharcolumn_indexUnique spectrum ID for each observation of each targetintcolumn_nameTarget designationchardatatypeTarget observation datechardescriptionSpectrograph IDcharindexedS/N of u filterintprincipalS/N of g filterintschema_nameUnique source identifier calculated with the "ura" and "udec" in table 9char"size"Plan nameintstdS/N of r filterinttable_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.charucdFiber pointing declination (degree)charunitFiber pointing right ascension (degree)charutypeFiber IDcharxtypeModified Julian daychar
tap_schema.tables
table_name
table_name
tap_schema.keysdescriptionTarget designationcharfrom_tableUnique source identifier calculated with the "ura" and "udec" in table 9charkey_idUnique spectrum ID for each observation of each targetchartarget_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.charutypeTarget observation datechar
tap_schema.tables
from_table
table_name
tap_schema.tables
target_table
table_name
tap_schema.key_columnsfrom_columnUnique source identifier calculated with the "ura" and "udec" in table 9charkey_idUnique spectrum ID for each observation of each targetchartarget_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.char
tap_schema.keys
key_id
key_id
tap_schema.columns
from_column
column_name
tap_schema.columns
target_column
column_name