J/A+A/699/A145/table2Stellar parameters and accretion properties for sources within 500pc, calculated from the Gaia DR3 H-alpha pseudo-equivalent widthrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGaiaDR3Gaia DR3 unique source identifier (GaiaDR3)meta.id;meta.mainb_FcontCE? 16th percentile of the GSP-Phot Halpha continuum flux density (flux_cont_lower_gspphot)W.nm**-1.m**-2phot.flux.density;spect.line;spect.continuumdoublenullableJmag? 2MASS J magnitude (1.25um) (Jmag)magphot.mag;em.IR.JfloatnullableB_FHaMed? 84th percentile of the med-GSP-Phot Halpha line-flux (FHalpha_upper_med-gspphot)W.nm**-1.m**-2phot.flux;spect.linedoublenullableb_FHaMed? 16th percentile of the med-GSP-Phot Halpha line-flux (FHalpha_lower_med-gspphot)W.nm**-1.m**-2phot.flux;spect.linedoublenullableLHaMed? Halpha line-luminosity, corrected using med-GSP-Phot extinction (LHalpha_med-gspphot)solLumphys.luminosity;em.line.HalphadoublenullableB_LHaMed? 84th percentile of the med-GSP-Phot Halpha line-luminosity (LHalpha_upper_med-gspphot)solLumphys.luminosity;em.line.Halpha;stat.maxdoublenullableRA_ICRSGaia Right ascension (ICRS) at Ep=2016.0 (RAdeg)degpos.eq.ra;meta.mainindexedDE_ICRSGaia Declination (ICRS) at Ep=2016.0 (DEdeg)degpos.eq.dec;meta.mainindexedGLONGaia Galactic longitude (l)degpos.galactic.lonGLATGaia Galactic latitude (b)degpos.galactic.latdoubleplxGaia parallax (plx)maspos.parallax.trigdoublee_plxStandard error of parallax (e_plx)masstat.error;pos.parallaxdoubleRPmagGaia integrated RP mean magnitude (RPmag)magphot.mag;em.opt.RdoubleGmag? Gaia integrated G mean magnitude (Gmag)magphot.mag;em.optdoublenullableBP-RP? Gaia BP-RP colour index (bp_rp)magphot.color;em.opt.B;em.opt.RdoublenullablepEWHaGaia Halpha pseudo-equivalent width (ew_espels_halpha)nmspect.line.widthdoublee_pEWHaUncertainty of Halpha pseudo-equivalent width (e_ew_espels_halpha)nmstat.errordoublergeoMedian of the geometric distance posterior (Bailer-Jones+, 2021, Cat. I/352) (r_med_geo)pcpos.distancedoubleb_rgeo16th percentile of the geometric distance posterior (r_lo_geo)pcpos.distancedoubleB_rgeo84th percentile of the geometric distance posterior (r_hi_geo)pcpos.distancedoubleEWHaEquivalent-width of the H-alpha line (EW)nmspect.line.eqWidthdoubleb_EWHa16th percentile of equivalent-width of the H-alpha line (EW_lower)nmspect.line.eqWidthdoubleB_EWHa84th percentile of equivalent-width of the H-alpha line (EW_upper)nmspect.line.eqWidthdoubleAG? Gaia extinction in G band from GSP-Phot (ag_gspphot) (1)magphys.absorptiondoublenullableb_AG? 16th percentile of extinction in G band (ag_gspphot_lower)magphys.absorptiondoublenullableB_AG? 84th percentile of extinction in G band (ag_gspphot_upper)magphys.absorptiondoublenullableARP? Gaia extinction in RP band from GSP-Phot (arp_gspphot) (1)magphys.absorptiondoublenullableb_ARP? 16th percentile of extinction in RP band (arp_gspphot_lower)magphys.absorptiondoublenullableB_ARP? 84th percentile of extinction in RP band (arp_gspphot_upper)magphys.absorptiondoublenullableABP? Gaia extinction in BP band from GSP-Phot (abp_gspphot) (1)magphys.absorptiondoublenullableb_ABP? 16th percentile of extinction in BP band (abp_gspphot_lower)magphys.absorptiondoublenullableB_ABP? 84th percentile of extinction in BP band (abp_gspphot_upper)magphys.absorptiondoublenullableRPmagCE? Extinction-corrected RP magnitude using GSP-Phot extinction (RP_mag_gspphot)magphot.mag;em.opt.Rdoublenullableb_RPmagCE? Lower limit to GSP-Phot RP magnitude (RP_mag_gspphot_lower)magphot.mag;stat.mindoublenullableB_RPmagCE? Upper limit to GSP-Phot RP magnitude (RP_mag_gspphot_upper)magphot.mag;stat.maxdoublenullableFcontNEContinuum flux density at the Halpha line, not corrected for extinction (flux_cont_noext)W.nm**-1.m**-2stat.paramdoubleb_FcontNE16th percentile of the non-extinction corrected Halpha continuum flux (flux_cont_noext_lower)W.nm**-1.m**-2phot.flux.density;spect.continuum;spect.linedoubleB_FcontNE84th percentile of the non-extinction corrected Halpha continuum flux (flux_cont_noext_upper)W.nm**-1.m**-2phot.flux.density;spect.line;spect.continuumdoubleFcontCE? Continuum flux density at the Halpha line, corrected using GSP-Phot extinction (flux_cont_gspphot)W.nm**-1.m**-2stat.paramdoublenullableB_FcontCE? 84th percentile of the GSP-Phot Halpha continuum flux density (flux_cont_upper_gspphot)W.nm**-1.m**-2phot.flux.density;spect.line;spect.continuumdoublenullableFHaNEHalpha line-flux, not corrected for extinction (FHalpha_noext)W.nm**-1.m**-2phot.flux;em.line.HalphadoubleB_FHaNE84th percentile of the non-extinction corrected Halpha line-flux (FHalpha_upper_noext)W.nm**-1.m**-2phot.flux;spect.linedoubleb_FHaNE16th percentile of the non-extinction corrected Halpha line-flux (FHalpha_lower_noext)W.nm**-1.m**-2phot.flux;spect.linedoubleLHaNEHalpha line-luminosity, not corrected for extinction (LHalpha_noext)solLumphys.luminosity;em.line.HalphadoubleB_LHaNE84th percentile of the non-extinction corrected Halpha line-luminosity (LHalpha_upper_noext)solLumphys.luminosity;em.line.Halpha;stat.maxdoubleb_LHaNE16th percentile of the non-extinction corrected Halpha line-luminosity (LHalpha_lower_noext)solLumphys.luminosity;em.line.Halpha;stat.mindoubleFHaCE? Halpha line-flux, corrected using GSP-Phot extinction (FHalpha_gspphot)W.m**-2phot.flux;em.line.HalphadoublenullableB_FHaCE? 84th percentile of the GSP-Phot Halpha line-flux (FHalpha_upper_gspphot)W.m**-2phot.flux;spect.linedoublenullableb_FHaCE? 16th percentile of the GSP-Phot Halpha line-flux (FHalpha_lower_gspphot)W.m**-2phot.flux;spect.linedoublenullableLHaCE? Halpha line-luminosity, corrected using GSP-Phot extinction (LHalpha_gspphot)solLumphys.luminosity;em.line.HalphadoublenullableB_LHaCE? 84th percentile of the GSP-Phot Halpha line-luminosity (LHalpha_upper_gspphot)solLumphys.luminosity;em.line.Halpha;stat.maxdoublenullableb_LHaCE? 16th percentile of the GSP-Phot Halpha line-luminosity (LHalpha_lower_gspphot)solLumphys.luminosity;em.line.Halpha;stat.mindoublenullablelogLaccNEAccretion luminosity, not corrected for extinction (log_Lacc_noext)log(solLum)phys.luminositydoubleB_logLaccNE84th percentile of the non-extinction corrected accretion luminosity (log_Lacc_upper_noext)log(solLum)phys.luminositydoubleb_logLaccNE16th percentile of the non-extinction corrected accretion luminosity (log_Lacc_lower_noext)log(solLum)phys.luminositydoubleE_logLaccNEUpper error of the non-extinction corrected accretion luminosity (e_log_Lacc_up_noext)log(solLum)stat.error;stat.maxdoublee_logLaccNELower error of the non-extinction corrected accretion luminosity (e_log_Lacc_low_noext)log(solLum)stat.errordoublelogLaccCE? Accretion luminosity, corrected using GSP-Phot extinction (log_Lacc_gspphot)log(solLum)phys.luminositydoublenullableB_logLaccCE? 84th percentile of the GSP-Phot accretion luminosity (log_Lacc_upper_gspphot)log(solLum)phys.luminositydoublenullableb_logLaccCE? 16th percentile of the GSP-Phot accretion luminosity (log_Lacc_lower_gspphot)log(solLum)phys.luminositydoublenullableE_logLaccCE? Upper error of the GSP-Phot accretion luminosity (e_log_Lacc_up_gspphot)log(solLum)stat.error;stat.maxdoublenullablee_logLaccCE? Lower error of the GSP-Phot accretion luminosity (e_log_Lacc_low_gspphot)log(solLum)stat.errordoublenullableRAWdeg? WISE Right ascension (J2000) (RAJ2000)degpos.eq.ranullableDEWdeg? WISE Declination (J2000) (DEJ2000)degpos.eq.decnullableW1mag? WISE W1 magnitude (3.35um) (W1mag)magphot.mag;em.IR.3-4umfloatnullableW2mag? WISE W2 magnitude (4.6um) (W2mag)magphot.mag;em.IR.4-8umfloatnullableW3mag? WISE W3 magnitude (11.6um) (W3mag)magphot.flux.density;em.IR.8-15umfloatnullableW4mag? WISE W4 magnitude (22.1um) (W4mag)magphot.flux.density;em.IR.15-30umfloatnullableHmag? 2MASS H magnitude (1.65um) (Hmag)magphot.mag;em.IR.HfloatnullableKsmag? 2MASS Ks magnitude (2.17um) (Ksmag)magphot.mag;em.IR.Kfloatnullablee_W1mag? Mean error on W1 magnitude (e_W1mag)magstat.error;phot.magfloatnullablee_W2mag? Mean error on W2 magnitude (e_W2mag)magstat.error;phot.magfloatnullablee_W3mag? Mean error on W3 magnitude (e_W3mag)magstat.error;phot.magfloatnullablee_W4mag? Mean error on W4 magnitude (e_W4mag)magstat.error;phot.magfloatnullablee_Jmag? Mean error on J magnitude (e_Jmag)magstat.error;phot.magfloatnullablee_Hmag? Mean error on H magnitude (e_Hmag)magstat.error;phot.magfloatnullablee_Ksmag? Mean error on Ks magnitude (e_Ksmag)magstat.error;phot.magfloatnullableangDist? Distance separating the positions of the Gaia DR3 source and the associated WISE source (angDist)arcsecpos.angDistancedoublenullablelambda? Wavelength at which linefinder detects Halpha emission, corresponding to the extremum (wavelength_nm)nmem.wldoublenullableLineFlux? Value of flux at the given wavelength (line_flux) (2)W.nm**-1.m**-2phot.fluxdoublenullableDepth? Difference between the line flux and the flux in estimated continuum (depth) (2)W.nm**-1.m**-2phot.flux.density;arith.diffdoublenullableWidth? Distance between the closest inflection points (width) (2)nmpos.distancedoublenullableSigni? Ratio between line depth and flux error at the extremum in the externally calibrated spectrum (significance) (2)meta.notedoublenullableGMAGCE? Absolute Magnitude corrected using GSP-Phot extinction (Mg_gspphot)magphys.magAbsdoublenullableE_GMAGCE? Upper error of the GSP-Phot absolute magnitude (E_Mg_gspphot)magstat.error;stat.maxdoublenullablee_GMAGCE? Lower error of the GSP-Phot absolute magnitude (e_Mg_gspphot)magstat.errordoublenullableBPintCE? Intrinsic BP magnitude corrected using GSP-Phot extinction (BPint_gspphot)magphot.mag;em.opt.BdoublenullableE_BPintCE? Upper error of GSP-Phot intrinsic BP magnitude (E_BPint_gspphot)magstat.error;stat.maxdoublenullablee_BPintCE? Lower error of GSP-Phot intrinsic BP magnitude (e_BPint_gspphot)magstat.errordoublenullableMassMeanCE? Stellar mass estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using GSP-Phot extinction (Mass_mean_gspphot)solMassphys.massdoublenullableMassStdCE? Standard deviation of GSP-Phot stellar mass (Mass_std_gspphot)solMassstat.errordoublenullablelogLumMeanCE? Stellar luminosity (log) estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using GSP-Phot extinction (Luminosity_mean_gspphot)log(solLum)phys.luminositydoublenullablelogLumStdCE? Standard deviation of GSP-Phot stellar luminosity (log) (Luminosity_std_gspphot)log(solLum)stat.errordoublenullableRadMeanCE? Stellar radius estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using GSP-Phot extinction (Radius_mean_gspphot)solRadphys.size.radiusdoublenullableRadStdCE? Standard deviation of GSP-Phot stellar radius (Radius_std_gspphot)solRadstat.errordoublenullableTempMeanCE? Effective temperature estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using GSP-Phot extinction (Temperature_mean_gspphot)Kphys.temperature.effectivedoublenullableTempStdCE? Standard deviation of GSP-Phot effective temperature (Temperature_std_gspphot)Kstat.errordoublenullableloggMeanCE? Surface gravity (log) estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using GSP-Phot extinction (logg_mean_gspphot)log(cm.s**-2)phys.gravitydoublenullableloggStdCE? Standard deviation of GSP-Phot surface gravity (log) (logg_std_gspphot)log(cm.s**-2)stat.errordoublenullableNAGMeanNumber of neighbouring stars used to calculate med-GSP-Phot extinction from GSP-Phot extinction in G band (ag_gspphot_count_med-gspphot)meta.numberfloatAGMean? Mean of GSP-Phot extinction in G band (ag_gspphot_mean_med-gspphot)magphys.absorptiondoublenullableAGStd? Standard deviation of med-GSP-Phot extinction (ag_gspphot_std_med-gspphot)magstat.errordoublenullableAGMin? Minimum GSP-Phot extinction (ag_gspphot_min_med-gspphot)magphys.absorptiondoublenullableAG25? 25th percentile of GSP-Phot extinction in RP band (ag_gspphot_25%_med-gspphot)magphys.absorptiondoublenullableAG50? Median (50th percentile) of GSP-Phot extinction in G band (ag_gspphot_50%_med-gspphot) (3)magphys.absorptiondoublenullableAG75? 75th percentile of GSP-Phot extinction in G band (ag_gspphot_75%_med-gspphot)magphys.absorptiondoublenullableAGMax? Maximum GSP-Phot extinction in G band (ag_gspphot_max_med-gspphot)magphys.absorptiondoublenullableNARPMeanNumber of neighbouring stars used to calculate the med-GSP-Phot extinction from GSP-Phot extinction in RP band (arp_gspphot_count_med-gspphot)meta.numberfloatARPMean? Mean of GSP-Phot extinction in RP band (arp_gspphot_mean_med-gspphot)magphys.absorptiondoublenullableARPStd? Standard deviation of GSP-Phot extinction in RP band (arp_gspphot_std_med-gspphot)magstat.errordoublenullableARPMin? Minimum GSP-Phot extinction in RP band (arp_gspphot_min_med-gspphot)magphys.absorptiondoublenullableARP25? 25th percentile of GSP-Phot extinction in RP band (arp_gspphot_25%_med-gspphot)magphys.absorptiondoublenullableARP50? Median (50th percentile) GSP-Phot extinction in RP band (arp_gspphot_50%_med-gspphot) (3)magphys.absorptiondoublenullableARP75? 75th percentile of GSP-Phot extinction in RP band (arp_gspphot_75%_med-gspphot)magphys.absorptiondoublenullableARPMax? Maximum GSP-Phot extinction in RP band (arp_gspphot_max_med-gspphot)magphys.absorptiondoublenullableNABPMeanNumber of neighbouring stars used to calculate the med-GSP-Phot extinction from GSP-Phot extinction in BP band (abp_gspphot_count_med-gspphot)meta.numberfloatABPMean? Mean of GSP-Phot extinction in BP band (abp_gspphot_mean_med-gspphot)magphys.absorptiondoublenullableABPStd? Standard deviation of GSP-Phot extinction in BP band (abp_gspphot_std_med-gspphot)magstat.errordoublenullableABPMin? Minimum GSP-Phot extinction in BP band (abp_gspphot_min_med-gspphot)magphys.absorptiondoublenullableABP25? 25th percentile of GSP-Phot extinction in BP band (abp_gspphot_25%_med-gspphot)magphys.absorptiondoublenullableABP50? Median (50th percentile) GSP-Phot extinction in BP band (abp_gspphot_50%_med-gspphot) (3)magphys.absorptiondoublenullableABP75? 75th percentile of GSP-Phot extinction in BP band (abp_gspphot_75%_med-gspphot)magphys.absorptiondoublenullableABPMax? Maximum GSP-Phot extinction in BP band (abp_gspphot_max_med-gspphot)magphys.absorptiondoublenullableNSepNumber of neighbouring stars used for separation calculation (Separation_count_med-gspphot)meta.numberfloatSepRMean? Mean angular separation of neighbouring stars used in med-GSP-Phot extinction calculation (Separation_mean_med-gspphot)arcsecpos.angDistance;stat.meandoublenullableSepStd? Standard deviation of angular separation (Separation_std_med-gspphot)arcsecstat.errordoublenullableSepMin? Minimum angular separation among neighbouring stars (Separation_min_med-gspphot)arcsecpos.angDistance;stat.mindoublenullableSep25? 25th percentile of angular separation (Separation_25%_med-gspphot)arcsecpos.angDistancedoublenullableSep50? Median (50th percentile) angular separation (Separation_50%_med-gspphot)arcsecpos.angDistance;stat.mediandoublenullableSep75? 75th percentile of angular separation (Separation_75%_med-gspphot)arcsecpos.angDistancedoublenullableSepMax? Maximum angular separation among neighbouring stars (Separation_max_med-gspphot)arcsecpos.angDistance;stat.maxdoublenullableBPint? Intrinsic BP magnitude corrected using med-GSP-Phot extinction (BPint_med-gspphot)magphot.mag;arith.diffdoublenullableE_BPint? Upper error of med-GSP-Phot intrinsic BP magnitude (E_BPint_med-gspphot)magstat.error;stat.maxdoublenullablee_BPint? Lower error of med-GSP-Phot intrinsic BP magnitude (e_BPint_med-gspphot)magstat.errordoublenullableGMAG? Absolute Magnitude corrected using med-GSP-Phot extinction (Mg_med-gspphot)magphys.magAbsdoublenullableE_GMAG? Upper error of the med-GSP-Phot absolute magnitude (E_Mg_med-gspphot)magstat.error;stat.maxdoublenullablee_GMAG? Lower error of the med-GSP-Phot absolute magnitude (e_Mg_med-gspphot)magstat.errordoublenullableMassMeanB? Stellar mass estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using med-GSP-Phot extinction (Mass_mean_med-gspphot)solMassphys.massdoublenullableMassStdB? Standard deviation of med-GSP-Phot stellar mass (Mass_std_med-gspphot)solMassstat.errordoublenullablelogLumMeanB? Stellar luminosity (log) estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using med-GSP-Phot extinction (Luminosity_mean_med-gspphot)log(solLum)phys.luminositydoublenullablelogLumStd? Standard deviation of med-GSP-Phot stellar luminosity (log) (Luminosity_std_med-gspphot)log(solLum)stat.errordoublenullableRadMean? Stellar radius estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using med-GSP-Phot extinction (Radius_mean_med-gspphot)solRadphys.size.radiusdoublenullableRadStd? Standard deviation of med-GSP-Phot stellar radius (Radius_std_med-gspphot)solRadstat.errordoublenullableTempMean? Effective temperature estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using med-GSP-Phot extinction (Temperature_mean_med-gspphot)Kphys.temperature.effectivedoublenullableTempStd? Standard deviation of med-GSP-Phot effective temperature (Temperature_std_med-gspphot)Kstat.errordoublenullableloggMean? Surface gravity (log) estimated from the Baraffe et al. (2015A&A...577A..42B) tracks using med-GSP-Phot extinction (logg_mean_med-gspphot)log(cm.s**-2)phys.gravitydoublenullableloggStd? Standard deviation of med-GSP-Phot surface gravity (log) (logg_std_med-gspphot)log(cm.s**-2)stat.errordoublenullableRPmagMed? Extinction-corrected RPmag using med-GSP-Phot extinction (RPmag_med-gspphot)magphot.mag;em.opt.Rdoublenullableb_RPmagMed? Lower limit to med-GSP-Phot RPmag (RPmag_med-gspphot_lower)magphot.mag;stat.mindoublenullableB_RPmagMed? Upper limit to med-GSP-Phot RPmag (RPmag_med-gspphot_upper)magphot.mag;stat.maxdoublenullableFcontMed? Continuum flux density at the Halpha line, corrected using med-GSP-Phot extinction (flux_cont_med-gspphot)W.nm**-1.m**-2stat.paramdoublenullableb_FcontMed? 16th percentile of the med-GSP-Phot Halpha continuum flux density (flux_cont_lower_med-gspphot)W.nm**-1.m**-2phot.flux.density;spect.line;spect.continuumdoublenullableB_FcontMed? 84th percentile of the med-GSP-Phot Halpha continuum flux density (flux_cont_upper_med-gspphot)W.nm**-1.m**-2phot.flux.density;spect.line;spect.continuumdoublenullableFHaMed? Halpha line-flux, corrected using med-GSP-Phot extinction (FHalpha_med-gspphot)W.nm**-1.m**-2phot.flux;em.line.Halphadoublenullableb_LHaMed? 16th percentile of the med-GSP-Phot Halpha line-luminosity (LHalpha_lower_med-gspphot)solLumphys.luminosity;em.line.Halpha;stat.mindoublenullablelogLaccMed? Accretion luminosity, corrected using med-GSP-Phot extinction (log_Lacc_med-gspphot)log(solLum)phys.luminositydoublenullableB_logLaccMed? 84th percentile of the med-GSP-Phot accretion luminosity (log_Lacc_upper_med-gspphot)log(solLum)phys.luminositydoublenullableb_logLaccMed? 16th percentile of the med-GSP-Phot accretion luminosity (log_Lacc_lower_med-gspphot)log(solLum)phys.luminositydoublenullableE_logLaccMed? Upper error of the med-GSP-Phot accretion luminosity (e_log_Lacc_up_med-gspphot)log(solLum)stat.error;stat.maxdoublenullablee_logLaccMed? Lower error of the med-GSP-Phot accretion luminosity (e_log_Lacc_low_med-gspphot)log(solLum)stat.errordoublenullableMaccCE? Mass accretion rate, corrected with GSP-Phot extinction (Macc_gspphot)solMass/yrarith.ratedoublenullableB_MaccCE? 84th percentile of the GSP-Phot mass accretion rate (Macc_upper_gspphot)solMass/yrarith.rate;phys.massdoublenullableb_MaccCE? 16th percentile of the GSP-Phot mass accretion rate (Macc_lower_gspphot)solMass/yrarith.rate;phys.massdoublenullableMaccMed? Mass accretion rate, corrected with med-GSP-Phot extinction (Macc_med-gspphot)solMass/yrarith.ratedoublenullableB_MaccMed? 84th percentile of the GSP-Phot mass accretion rate (Macc_upper_med-gspphot)solMass/yrarith.rate;phys.massdoublenullableb_MaccMed? 16th percentile of the GSP-Phot mass accretion rate (Macc_lower_med-gspphot)solMass/yrarith.rate;phys.massdoublenullableFlgCMDFlag indicating whether the source falls within the YSO-compatible region of the CMD (flag_CMD) (4)meta.codecharFlgGaiaScanFlag indicating whether the source falls in the sky regions affected by the Gaia scanning-law (flag_Gaia_Scanning) (4)meta.codecharFlgabove? Flag indicating whether accretion is observed above the level of chromospheric emission (flag_above_chromospheric_level) (4)meta.codecharFlgIRFlag indicating signals of strong infrared excess (flag_IR) (4)meta.codecharFlg-pEWFlag indicating pEW less than -1 (flag_pEW) (4)meta.codecharFlg-combFlag of sources with both flag-IR and flag-pEW = True (flag_combined) (4)meta.codecharXPcontFlag indicating the availability of Gaia mean BP/RP spectrum in continuous representation for this source (has_xp_continuous)meta.codecharAllWISE? WISE All-Sky Release Catalog name, JHHMMSS.ss+DDMMSS.s (AllWISE)meta.idchar
J/A+A/699/A145/table4Fraction of accretors and median accretion properties for 34 Sco-Cen clustersNpEWtotNumber of sources per cluster with measured Gaia pseudo-equivalent width (N_pEW_tot)meta.numberintB_Lacc2? 84th percentile of mass-adjusted med-GSP-Phot accretion luminosity (Lacc_84_corrected_med-gspphot) (2)solLumphys.luminositydoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSigMA[1/35] Membership label for each cluster (SigMA) (1)meta.code.memberintNaccNumber of accretors per cluster (sources with pseudo-equivalent width less than -1nm) (N_acc)meta.numberintfaccFraction of accretors per cluster (f_acc)meta.numberdoublee_faccError of fraction of accretors (e_f_acc)stat.errordoubleRegionTraditional Sco-Cen subregions (Region) (1)meta.notecharAgeP-BpRpAge from PARSEC models and Bp-Rp colors (AgeP-BpRp) (1)Myrtime.agefloate_AgeP-BpRpLower P-BpRp 1 sigma age interval (e_AgeP-BpRp) (1)Myrstat.errorfloatE_AgeP-BpRpUpper P-BpRp 1 sigma age interval (E_AgeP-BpRp) (1)Myrstat.error;stat.maxfloatAgeP-GRpAge from PARSEC models and G-Rp colors (AgeP-GRp) (1)Myrtime.agefloate_AgeP-GRpLower P-GRp 1 sigma age interval (e_AgeP-GRp) (1)Myrstat.errorfloatE_AgeP-GRpUpper P-GRp 1 sigma age interval (E_AgeP-GRp) (1)Myrstat.error;stat.maxfloatAgeB-BpRpAge from BHAC15 models and Bp-Rp colors (AgeB-BpRp) (1)Myrtime.agefloate_AgeB-BpRpLower B-BpRp 1 sigma age interval (e_AgeB-BpRp) (1)Myrstat.errorfloatE_AgeB-BpRpUpper B-BpRp 1 sigma age interval (E_AgeB-BpRp) (1)Myrstat.error;stat.maxfloatAgeB-GRpAge from BHAC15 models and G-Rp colors (AgeB-GRp) (1)Myrtime.agefloate_AgeB-GRpLower B-GRp 1 sigma age interval (e_AgeB-GRp) (1)Myrstat.errorfloatE_AgeB-GRpUpper B-GRp 1 sigma age interval (E_AgeB-GRp) (1)Myrstat.error;stat.maxfloatNExt1? Number of sources per cluster with med-GSP-Phot extinction available (count_med-gspphot)meta.numberfloatnullableMass1? Median mass (corrected with med-GSP-Phot extinction) of the cluster (Mass_median_med-gspphot)solMassphys.massdoublenullableLacc1? Median accretion luminosity (corrected with med-GSP-Phot extinction) of the cluster (Lacc_median_med-gspphot)solLumphys.luminositydoublenullableMacc1? Median mass accretion rate (corrected with med-GSP-Phot extinction) of the cluster (Macc_median_med-gspphot)solMass/yrarith.rate;phys.mass;stat.mediandoublenullableb_Lacc1? 16th percentile of med-GSP-Phot accretion luminosity (Lacc_16_med-gspphot)solLumphys.luminositydoublenullableB_Lacc1? 84th percentile of med-GSP-Phot accretion luminosity (Lacc_84_med-gspphot)solLumphys.luminositydoublenullableb_Macc1? 16th percentile of med-GSP-Phot mass accretion rate (Macc_16_med-gspphot)solMass/yrarith.rate;phys.massdoublenullableB_Macc1? 84th percentile of med-GSP-Phot mass accretion rate (Macc_84_med-gspphot)solMass/yrarith.rate;phys.massdoublenullableNExt2? Number of sources per cluster with med-GSP-Phot extinction available used for mass-adjusted median calculations (count_corrected_med-gspphot)meta.numberfloatnullableMass2? Median mass-adjusted mass (corrected with med-GSP-Phot extinction) of the cluster (Mass_median_corrected_med-gspphot) (2)solMassphys.massdoublenullableLacc2? Median mass-adjusted accretion luminosity (corrected with med-GSP-Phot extinction) of the cluster (Lacc_median_corrected_med-gspphot) (2)solLumphys.luminositydoublenullableMacc2? Median mass-adjusted mass accretion rate (corrected with med-GSP-Phot extinction) of the cluster (Macc_median_corrected_med-gspphot) (2)solMass/yrarith.rate;phys.mass;stat.mediandoublenullableb_Lacc2? 16th percentile of mass-adjusted med-GSP-Phot accretion luminosity (Lacc_16_corrected_med-gspphot) (2)solLumphys.luminositydoublenullableb_Macc2? 16th percentile of mass-adjusted med-GSP-Phot mass accretion rate (Macc_16_corrected_med-gspphot) (2)solMass/yrarith.rate;phys.massdoublenullableB_Macc2? 84th percentile of mass-adjusted med-GSP-Phot mass accretion rate (Macc_84_corrected_med-gspphot) (2)solMass/yrarith.rate;phys.massdoublenullableNExt3? Number of sources per cluster with GSP-Phot extinction available used for mass-adjusted median calculations (count_gspphot) (2)meta.numberfloatnullableMass3? Median mass-adjusted mass (corrected with GSP-Phot extinction) of the cluster (Mass_median_gspphot) (2)solMassphys.massdoublenullableLacc3? Median accretion luminosity (corrected with GSP-Phot extinction) (Lacc_median_gspphot)solLumphys.luminositydoublenullableMacc3? Median mass accretion rate (corrected with GSP-Phot extinction) of the cluster (Macc_median_gspphot)solMass/yrarith.rate;phys.mass;stat.mediandoublenullableb_Lacc3? 16th percentile of GSP-Phot accretion luminosity (Lacc_16_gspphot)solLumphys.luminositydoublenullableB_Lacc3? 84th percentile of GSP-Phot accretion luminosity (Lacc_84_gspphot)solLumphys.luminositydoublenullableb_Macc3? 16th percentile of GSP-Phot mass accretion rate (Macc_16_gspphot)solMass/yrarith.rate;phys.massdoublenullableB_Macc3? 84th percentile of GSP-Phot mass accretion rate (Macc_84_gspphot)solMass/yrarith.rate;phys.massdoublenullableNExt4? Number of sources per cluster with GSP-Phot extinction available used for mass-adjusted median calculations (count_corrected_gspphot)meta.numberfloatnullableMass4? Median mass-adjusted mass (corrected with GSP-Phot extinction) of the cluster (Mass_median_corrected_gspphot)solMassphys.massdoublenullableLacc4? Median mass-adjusted accretion luminosity (corrected with GSP-Phot extinction) of the cluster (Lacc_median_corrected_gspphot)solLumphys.luminositydoublenullableMacc4? Median mass-adjusted mass accretion rate (corrected with med-GSP-Phot extinction) of the cluster (Macc_median_corrected_gspphot)solMass/yrarith.rate;phys.mass;stat.mediandoublenullableb_Lacc4? 16th percentile of mass-adjusted GSP-Phot accretion luminosity (Lacc_16_corrected_gspphot)solLumphys.luminositydoublenullableB_Lacc4? 84th percentile of mass-adjusted GSP-Phot accretion luminosity (Lacc_84_corrected_gspphot)solLumphys.luminositydoublenullableb_Macc4? 16th percentile of mass-adjusted GSP-Phot mass accretion rate (Macc_16_corrected_gspphot)solMass/yrarith.rate;phys.massdoublenullableB_Macc4? 84th percentile of mass-adjusted GSP-Phot mass accretion rate (Macc_84_corrected_gspphot)solMass/yrarith.rate;phys.massdoublenullableSlLacc-Lstar? Slope of accretion luminosity - stellar luminosity correlation per cluster (slope_Lacc_Lstar)meta.crypticdoublenullablee_SlLacc-Lstar? Error of Lacc-Lstar slope (e_slope_Lacc_Lstar)stat.errordoublenullableSlMacc-Mstar? Slope of mass accretion rate - stellar mass correlation per cluster (slope_Macc_Mstar)meta.crypticdoublenullablee_SlMacc-Mstar? Error of Macc-Mstar slope (e_slope_Macc_Mstar)stat.errordoublenullableGroupCluster Name (Group) (1)meta.idchar
J/A+A/699/A145/table6Fraction of accretors and median accretion properties for various star-forming regions and groups within 500pcNameName of region or group (Name)meta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAgeAge of region or group (Age)Myrtime.age;obs.fieldfloatRefMembReference for membership (Membership_ref) (1)meta.bibcharRefAgeReference for age (Age_ref) (1)meta.bibcharNpEWtotNumber of sources with measured Gaia pseudo-equivalent width (N_pEW_tot)meta.numberintNaccNumber of accretors (sources with pseudo-equivalent less than -1) (N_acc)meta.numberintPAgeaccPercentage of accretors (percentage_acc)meta.numberdoublee_PAgeaccError of percentage of accretors (e_percentage_acc)stat.errordoubleNExt3Number of sources GSP-Phot extinction available (count_gspphot)meta.numberintLacc3? Median accretion luminosity (corrected with GSP-Phot extinction) (Lacc_median_gspphot)solLumphys.luminositydoublenullableb_Lacc3? 16th percentile of GSP-Phot accretion luminosity (Lacc_16_gspphot)solLumphys.luminositydoublenullableB_Lacc3? 84th percentile of GSP-Phot accretion luminosity (Lacc_84_gspphot)solLumphys.luminositydoublenullableMacc3? Median mass accretion rate (corrected with GSP-Phot extinction) (Macc_median_gspphot)solMass/yrarith.rate;phys.mass;stat.mediandoublenullableb_Macc3? 16th percentile of GSP-Phot mass accretion rate (Macc_16_gspphot)solMass/yrarith.rate;phys.massdoublenullableB_Macc3? 84th percentile of GSP-Phot mass accretion rate (Macc_84_gspphot)solMass/yrarith.rate;phys.massdoublenullableMass3? Median mass (corrected with GSP-Phot extinction) (Mass_median_gspphot)solMassphys.massdoublenullableNExt1Number of sources med-GSP-Phot extinction available (count_med-gspphot)meta.numberintLacc1? Median accretion luminosity (corrected with med-GSP-Phot extinction) (Lacc_median_med-gspphot)solLumphys.luminositydoublenullableb_Lacc1? 16th percentile of med-GSP-Phot accretion luminosity (Lacc_16_med-gspphot)solLumphys.luminositydoublenullableB_Lacc1? 84th percentile of med-GSP-Phot accretion luminosity (Lacc_84_med-gspphot)solLumphys.luminositydoublenullableMacc1? Median mass accretion rate (corrected with med-GSP-Phot extinction) (Macc_median_med-gspphot)solMass/yrarith.rate;phys.mass;stat.mediandoublenullableb_Macc1? 16th percentile of med-GSP-Phot mass accretion rate (Macc_16_med-gspphot)solMass/yrarith.rate;phys.massdoublenullableB_Macc1? 84th percentile of med-GSP-Phot mass accretion rate (Macc_84_med-gspphot)solMass/yrarith.rate;phys.massdoublenullableMass1? Median mass (corrected with med-GSP-Phot extinction) (Mass_median_med-gspphot)solMassphys.massdoublenullable