J/A+A/673/A114/clustersMain catalogue (Table 3)_RA.icrsRight ascension (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.raindexed_DE.icrsDeclination (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.decindexedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID? Internal cluster IDmeta.idintnullableCST[3/99] Astrometric SNR (cluster significance test) (G1)stat.snrdoubleN[10/153797] Number of member starsmeta.numberintCSTt[2.9/99] Astrometric SNR within tidal radius (G1)stat.snrdoubleNt[10/53464] Number of stars within tidal radiusmeta.numberintRA_ICRSRight ascension of densest point (ICRS) at Ep=2016.0degpos.eq.ra;meta.mainDE_ICRSDeclination of densest point (ICRS) at Ep=2016.0degpos.eq.dec;meta.mainGLONGalactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latdoubler50Radius containing 50% of members within the tidal radiusdegphys.angSizedoublercCore radius (approximate estimate)degphys.angSize;srcdoublertTidal radius (approximate estimate)degphys.angSize;srcdoublertotTotal radius (including tidal tails, coma, etc)degphys.angSizedoubler50pcRadius containing 50% of members in parsecspcphys.size.radiusdoublercpcCore radius in parsecspcphys.size.radiusdoublertpcTidal radius in parsecspcphys.size.radiusdoublertotpcTotal radius in parsecspcphys.size.radiusdoublepmRAMean proper motion in right ascension multipled by cos(dec)mas/yrpos.pm;pos.eq.radoubles_pmRAStandard deviation of pmRAmas/yrstat.stdev;pos.pm;pos.eq.radoublee_pmRAStandard error of pmRAmas/yrstat.error;pos.pm;pos.eq.radoublepmDEMean proper motion in declinationmas/yrpos.pm;pos.eq.decdoubles_pmDEStandard deviation of pmDEmas/yrstat.stdev;pos.pm;pos.eq.decdoublee_pmDEStandard error of pmDEmas/yrstat.error;pos.pm;pos.eq.decdoublePlxMean parallaxmaspos.parallax;stat.meandoubles_PlxStandard deviation of parallaxmasstat.stdev;pos.parallaxdoublee_PlxStandard error of parallaxmasstat.error;pos.parallaxdoubledist1616th percentile of maximum likelihood distancepcpos.distancedoubledist5050th percentile of maximum likelihood distancepcpos.distancedoubledist8484th percentile of maximum likelihood distancepcpos.distancedoubleNdistNumber of stars used for distance calculationmeta.numberintglobalPlx[0/1] Flag indicating clusters for which a star-by-star parallax offset correction was not possible during distance calculationmeta.codeintXX coordinate in galactocentric galactic coordinatespcpos.cartesian.x;pos.galactocentric;pos.galacticdoubleYY coordinate in galactocentric galactic coordinatespcpos.cartesian.y;pos.galactocentric;pos.galacticdoubleZZ coordinate in galactocentric galactic coordinatespcpos.cartesian.z;pos.galactocentric;pos.galacticdoubleRV? Mean Gaia DR3 radial velocitykm/sphys.veloc;pos.heliocentricdoublenullables_RV? Standard deviation of radial velocitykm/sstat.stdev;spect.dopplerVelocdoublenullablee_RV? Standard error of radial velocitykm/sstat.errordoublenullablen_RVNumber of member stars with a radial velocitymeta.noteintCMDCl2.5[0/1] 2.5th percentile of CMD classmeta.codedoubleCMDCl16[0/1] 16th percentile of CMD classmeta.codedoubleCMDCl50[0/1] 50th percentile of CMD classmeta.codedoubleCMDCl84[0/1] 84th percentile of CMD classmeta.codedoubleCMDCl97.5[0/1] 97.5th percentile of CMD classmeta.codedoubleCMDClHumanHuman-assigned CMD class (where available) (G2)meta.codecharlogAge1616th percentile of logarithm of cluster agelog(yr)time.agedoublelogAge5050th percentile of logarithm of cluster agelog(yr)time.agedoublelogAge8484th percentile of logarithm of cluster agelog(yr)time.agedoubleAV1616th percentile of V-band cluster extinctionmagphys.absorptiondoubleAV5050th percentile of V-band cluster extinctionmagphys.absorptiondoubleAV8484th percentile of V-band cluster extinctionmagphys.absorptiondoublediffAV1616th percentile of approximate V-band differential extinctionmagphys.absorption;arith.diffdoublediffAV5050th percentile of approximate V-band differential extinctionmagphys.absorption;arith.diffdoublediffAV8484th percentile of approximate V-band differential extinctionmagphys.absorption;arith.diffdoubleMOD1616th percentile of photometrically estimated distance modulusmagphot.mag.distModdoubleMOD5050th percentile of photometrically estimated distance modulusmagphot.mag.distModdoubleMOD8484th percentile of photometrically estimated distance modulusmagphot.mag.distModdoubleminClSize[-1/80] HDBSCAN parameter used to construct cluster membership list (-1 for membership lists not made with HDBSCAN)meta.code.member;instr.setupintisMerged[0/1] Flag indicating manually merged cluster membership listmeta.codeintisGMMMemb[0/1] Flag indicating cluster membership list constructed using additional Gaussian mixture model post-processing stepmeta.codeintNXmatches[0/23] Number of unique crossmatches to this clustermeta.numberintXmatchTypeType of crossmatch (G3)meta.codecharNameMain accepted cluster name (1)meta.id;meta.maincharAllNamesComma separated list of all crossmatched cluster namesmeta.idcharType[omg] Type of object (o: open cluster, m: moving group, g: globular cluster)src.classchar
J/A+A/673/A114/membersMember stars of clusters (corrected version)_DE.icrsDeclination (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.decindexed_RA.icrsRight ascension (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.raindexedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID? Internal cluster IDmeta.idintnullableGaiaDR3Gaia DR3 source IDmeta.id;meta.mainProb[0/1] Membership probabilitystat.probabilitydoubleRA_ICRSRight ascension of star (ICRS) at Ep=2016.0degpos.eq.ra;meta.mainindexede_RA_ICRSStandard error on RAarcsecstat.error;pos.eq.radoubleDE_ICRSDeclination of star (ICRS) at Ep=2016.0degpos.eq.dec;meta.mainindexede_DE_ICRSStandard error on DEarcsecstat.error;pos.eq.decdoubleGLONGalactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latdoublepmRAMean proper motion in right ascension multipled by cos(dec)mas/yrpos.pm;pos.eq.radoublee_pmRAStandard error of pmRAmas/yrstat.error;pos.pm;pos.eq.radoublepmDEMean proper motion in declinationmas/yrpos.pm;pos.eq.decdoublee_pmDEStandard error of pmDEmas/yrstat.error;pos.pm;pos.eq.decdoublePlxMean parallaxmaspos.parallax;stat.meandoublee_PlxStandard error of parallaxmasstat.error;pos.parallaxdoublepscol? Estimated pseudocolourum**-1stat.fit.paramdoublenullablee_pscol? Standard error on pseudocolorum**-1stat.errordoublenullablePlxpmRACorCorrelation between parallax and pmRAstat.correlationdoublePlxpmDECorCorrelation between parallax and pmDEstat.correlationdoublepmRApmDECorCorrelation between pmRA and pmdEstat.correlationdoublePlxpscolCor? Correlation between parallax and pseudocolourstat.correlationdoublenullablepmRApscolCor? Correlation between pmRA and pseudocolourstat.correlationdoublenullablepmDEpscolCor? Correlation between pmDE and pseudocolourstat.correlationdoublenullableSolved[31/95] Gaia DR3 flag indicating which parameters solved formeta.numberintELATEcliptic latitudedegpos.ecliptic.latdoublenueff? Effective wavenumber of source used in astrometric solutionum**-1em.freqdoublenullableRUWERenormalised unit weight errorstat.errordoubleFidelityV1Rybizki et al. (2022MNRAS.510.2597R) V1 fidelity parametermeta.codedoubleFGMean G-band fluxphot.flux.density;em.optdoublee_FGError on mean G-band fluxstat.errordoubleFBPMean BP-band fluxphot.flux.density;em.opt.Bdoublee_FBPError on mean BP-band fluxstat.errordoubleFRPMean RP-band fluxphot.flux.density;em.opt.Rdoublee_FRPError on mean RP-band fluxstat.errordoubleGmagMean G-band magnitudemagphot.mag;em.optdoubleBPmagMean BP-band magnitudemagphot.mag;em.opt.BdoubleRPmagMean RP-band magnitudemagphot.mag;em.opt.RdoubleBP-RPBP-RP colourmagphot.color;em.opt.B;em.opt.RdoubleBP-GBP-G colourmagphot.color;em.opt;em.optdoubleG-RPG-RP colourmagphot.color;em.opt;em.optdoubleRV? Mean Gaia DR3 radial velocitykm/sphys.veloc;pos.heliocentricdoublenullablee_RV? Standard error of radial velocitykm/sstat.errordoublenullablen_RV? Method used to obtain the RVmeta.notefloatnullableo_RV? Number of transits used to compute the RVmeta.numberfloatnullableo_RVd? Number of transits that underwent deblendingmeta.numberfloatnullableGRVSmag? Mean Grvs magnitudemagphot.mag;em.optdoublenullablee_GRVSmag? Error on mean Grvs magnitudemagstat.error;phot.magdoublenullableo_GRVSmag? Number of transits used to construct Grvs magnitudemeta.numberfloatnullableVbroad? Spectral line broadening parameterkm/sspect.line.broad;spect.linedoublenullablee_Vbroad? Error on the spectral line broadeningkm/sstat.errordoublenullableo_Vbroad? Number of transits used to compute vbroadmeta.numberfloatnullableNSS[0/6] Flag indicating source has additional information in the Gaia DR3 non single star tablesmeta.codeintrgeo? Median of the geometric distance posteriorpcpos.distancedoublenullablerpgeo? Median of the photogeometric distance posteriorpcpos.distancedoublenullableNameMain accepted cluster namemeta.id.parentcharinrtFlag indicating if cluster is within tidal radius (i.e. is a good member)meta.codecharVarFlagGaia DR3 photometric variability flagmeta.code;src.varcharRVSFlag indicating the availability of mean RVS spectrum for this sourcemeta.codechar
J/A+A/673/A114/crossmaAll (non-)xmatched clusters (Table B.1)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID? Internal cluster ID (blank if object has no crossmatched cluster in our work)meta.id;meta.mainintnullableNameLitName in literature cataloguemeta.idcharSourceCatSource catalogue referencemeta.id;meta.datasetcharTypeSourceCatComma separated list of all source catalogue crossmatch types for this crossmatchsrc.classcharSep[0/2]? Separation between cluster centresdegpos.angDistancedoublenullableSepTidal[0/0.94]? Separation in terms of largest tidal radiuspos.angDistancedoublenullableSepTidalLit[0/1]? Separation in terms of literature tidal radiuspos.angDistancedoublenullableSepTidalData[0/1]? Separation in terms of tidal radius in this workpos.angDistancedoublenullablepmRASep[0/17.41]? Separation in pmRA times cos(dec) between this work and literaturemas/yrpos.angDistancedoublenullablepmRASigma? pmRA separation in terms of uncertainty on pmRA in this work and literature added in quadraturepos.angDistancedoublenullablepmDESep[0/11.24]? Separation in pmDE between this work and literaturemas/yrpos.angDistancedoublenullablepmDESigma? pmDE separation in terms of uncertainty on pmRA in this work and literature added in quadraturepos.angDistancedoublenullablePlxSep[0/2.8]? Separation in parallax between this work and literaturemaspos.angDistancedoublenullablePlxSigma? Parallax separation in terms of uncertainty on pmRA in this work and literature added in quadraturepos.angDistancedoublenullablemaxSigma? Maximum value of pmRASepSigma, pmDESepSigma, and PlxSepSigma (must be less than 2.0 for a valid astrometric match)pos.pm;pos.eq.ra;stat.maxdoublenullablemeanSigma? Mean value of pmRASepSigma, pmDESepSigma, and PlxSepSigmapos.pm;pos.eq.ra;stat.meandoublenullable
J/A+A/673/A114/clustrejObjects rejected from main catalogueCSTt[3/99] Astrometric SNR within tidal radiusstat.snrdouble_RA.icrsRight ascension (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.raindexed_DE.icrsDeclination (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.decindexedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[7167/7787] Internal cluster IDmeta.idintCST[3/99] Astrometric SNR (cluster significance test) (G1)stat.snrdoubleN[10/104862] Number of member starsmeta.numberintNt[10/40000] Number of stars within tidal radiusmeta.numberintRA_ICRSRight ascension of densest point (ICRS) at Ep=2016.0degpos.eq.ra;meta.mainDE_ICRSDeclination of densest point (ICRS) at Ep=2016.0degpos.eq.dec;meta.mainGLONGalactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latdoubler50Radius containing 50% of members within the tidal radiusdegphys.angSizedoublercCore radius (approximate estimate)degphys.angSize;srcdoublertTidal radius (approximate estimate)degphys.angSize;srcdoublertotTotal radius (including tidal tails, coma, etc)degphys.angSizedoubler50pcRadius containing 50% of members in parsecspcphys.size.radiusdoublercpcCore radius in parsecspcphys.size.radiusdoublertpcTidal radius in parsecspcphys.size.radiusdoublertotpcTotal radius in parsecspcphys.size.radiusdoublepmRAMean proper motion in right ascension multipled by cos(dec)mas/yrpos.pm;pos.eq.radoubles_pmRAStandard deviation of pmRAmas/yrstat.stdev;pos.pm;pos.eq.radoublee_pmRAStandard error of pmRAmas/yrstat.error;pos.pm;pos.eq.radoublepmDEMean proper motion in declinationmas/yrpos.pm;pos.eq.decdoubles_pmDEStandard deviation of pmDEmas/yrstat.stdev;pos.pm;pos.eq.decdoublee_pmDEStandard error of pmDEmas/yrstat.error;pos.pm;pos.eq.decdoublePlxMean parallaxmaspos.parallax;stat.meandoubles_PlxStandard deviation of parallaxmasstat.stdev;pos.parallaxdoublee_PlxStandard error of parallaxmasstat.error;pos.parallaxdoubledist1616th percentile of maximum likelihood distancepcpos.distancedoubledist5050th percentile of maximum likelihood distancepcpos.distancedoubledist8484th percentile of maximum likelihood distancepcpos.distancedoubleNdist[7/46664] Number of stars used for distance calculationmeta.numberintglobalPlx[0/1] Flag indicating clusters for which a star-by-star parallax offset correction was not possible during distance calculationmeta.codeintXX coordinate in galactocentric galactic coordinatespcpos.cartesian.x;pos.galactic;pos.galactocentricdoubleYY coordinate in galactocentric galactic coordinatespcpos.cartesian.y;pos.galactocentric;pos.galacticdoubleZZ coordinate in galactocentric galactic coordinatespcpos.cartesian.z;pos.galactocentric;pos.galacticdoubleRV? Mean Gaia DR3 radial velocitykm/sphys.veloc;pos.heliocentricdoublenullables_RV? Standard deviation of radial velocitykm/sstat.stdev;spect.dopplerVelocdoublenullablee_RV? Standard error of radial velocitykm/sstat.errordoublenullablen_RVNumber of member stars with a radial velocitymeta.noteintCMDCl2.5[0/1] 2.5th percentile of CMD classmeta.codedoubleCMDCl16[0/1] 16th percentile of CMD classmeta.codedoubleCMDCl50[0/1] 50th percentile of CMD classmeta.codedoubleCMDCl84[0/1] 84th percentile of CMD classmeta.codedoubleCMDCl97.5[0/1] 97.5th percentile of CMD classmeta.codedoublelogAge1616th percentile of logarithm of cluster agelog(yr)time.agedoublelogAge5050th percentile of logarithm of cluster agelog(yr)time.agedoublelogAge8484th percentile of logarithm of cluster agelog(yr)time.agedoubleAV1616th percentile of V-band cluster extinctionmagphys.absorptiondoubleAV5050th percentile of V-band cluster extinctionmagphys.absorptiondoubleAV8484th percentile of V-band cluster extinctionmagphys.absorptiondoublediffAV1616th percentile of approximate V-band differential extinctionmagphys.absorption;arith.diffdoublediffAV5050th percentile of approximate V-band differential extinctionmagphys.absorption;arith.diffdoublediffAV8484th percentile of approximate V-band differential extinctionmagphys.absorption;arith.diffdoubleMOD1616th percentile of photometrically estimated distance modulusmagphot.mag.distModdoubleMOD5050th percentile of photometrically estimated distance modulusmagphot.mag.distModdoubleMOD8484th percentile of photometrically estimated distance modulusmagphot.mag.distModdoubleminClSize[-1/80] HDBSCAN parameter used to construct cluster membership list (-1 for membership lists not made with HDBSCAN)meta.code.member;instr.setupintisMerged[0/1] Flag indicating manually merged cluster membership listmeta.codeintisGMMMemb[0/1] Flag indicating cluster membership list constructed using additional Gaussian mixture model post-processing stepmeta.codeintNXmatches[0/2] Number of unique crossmatches to this clustermeta.numberintXmatchTypeType of crossmatch (G3)meta.codecharisMC[0/1] Flag indicating cluster is believed to be in Magellanic cloudsmeta.codeintisStream[0/1] Flag indicating cluster is believed to be a component of a stellar streammeta.codeintNameMain accepted cluster namemeta.id;meta.maincharAllNamesComma separated list of all crossmatched cluster namesmeta.idcharType[omg] Type of object (o: open cluster, m: moving group, g: globular cluster)src.classcharCMDClHumanHuman-assigned CMD class (where available) (G2)meta.codechar
J/A+A/673/A114/membrejMember stars of rejected clusters_RA.icrsRight ascension (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.raindexed_DE.icrsDeclination (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.decindexedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[7167/7787] Internal cluster IDmeta.idintGaiaDR3Gaia DR3 source IDmeta.id;meta.maininrt[0/1] Flag indicating if cluster is within tidal radius (i.e. is a good member)meta.codeintProb[0/1] Membership probabilitystat.probabilitydoubleRA_ICRSRight ascension of star (ICRS) at Ep=2016.0degpos.eq.ra;meta.mainindexede_RA_ICRSStandard error on RAarcsecstat.error;pos.eq.radoubleDE_ICRSDeclination of star (ICRS) at Ep=2016.0degpos.eq.dec;meta.mainindexede_DE_ICRSStandard error on DEarcsecstat.error;pos.eq.decdoubleGLONGalactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latdoublepmRAMean proper motion in right ascension multipled by cos(dec)mas/yrpos.pm;pos.eq.radoublee_pmRAStandard error of pmRAmas/yrstat.error;pos.pm;pos.eq.radoublepmDEMean proper motion in declinationmas/yrpos.pm;pos.eq.decdoublee_pmDEStandard error of pmDEmas/yrstat.error;pos.pm;pos.eq.decdoublePlxMean parallaxmaspos.parallax;stat.meandoublee_PlxStandard error of parallaxmasstat.error;pos.parallaxdoublepscol? Estimated pseudocolourum**-1stat.fit.paramdoublenullablee_pscol? Standard error on pseudocolorum**-1stat.errordoublenullablePlxpmRACorCorrelation between parallax and pmRAstat.correlationdoublePlxpmDECorCorrelation between parallax and pmDEstat.correlationdoublepmRApmDECorCorrelation between pmRA and pmDEstat.correlationdoublePlxpscolCor? Correlation between parallax and pseudocolourstat.correlationdoublenullablepmRApscolCor? Correlation between pmRA and pseudocolourstat.correlationdoublenullablepmDEpscolCor? Correlation between pmDE and pseudocolourstat.correlationdoublenullableSolved[31/95] Gaia DR3 flag indicating which parameters solved formeta.numberintELATEcliptic latitudedegpos.ecliptic.latdoublenueff? Effective wavenumber of source used in astrometric solutionum**-1em.freqdoublenullableRUWERenormalised unit weight errorstat.errordoubleFidelityV1Rybizki et al. (2022MNRAS.510.2597R) V1 fidelity parametermeta.codedoubleFGMean G-band fluxphot.flux.density;em.optdoublee_FGError on mean G-band fluxstat.errordoubleFBPMean BP-band fluxphot.flux.density;em.opt.Bdoublee_FBPError on mean BP-band fluxstat.errordoubleFRPMean RP-band fluxphot.flux.density;em.opt.Rdoublee_FRPError on mean RP-band fluxstat.errordoubleGmagMean G-band magnitudemagphot.mag;em.optdoubleBPmagMean BP-band magnitudemagphot.mag;em.opt.BdoubleRPmagMean RP-band magnitudemagphot.mag;em.opt.RdoubleBP-RPBP-RP colourmagphot.color;em.opt.B;em.opt.RdoubleBP-GBP-G colourmagphot.color;em.opt;em.optdoubleG-RPG-RP colourmagphot.color;em.opt;em.optdoubleRV? Mean Gaia DR3 radial velocitykm/sphys.veloc;pos.heliocentricdoublenullablee_RV? Standard error of radial velocitykm/sstat.errordoublenullablen_RV? Method used to obtain the RVmeta.notefloatnullableo_RV? Number of transits used to compute the RVmeta.numberfloatnullableo_RVd? Number of transits that underwent deblendingmeta.numberfloatnullableGRVSmag? Mean Grvs magnitudemagphot.mag;em.optdoublenullablee_GRVSmag? Error on mean Grvs magnitudemagstat.error;phot.magdoublenullableo_GRVSmag? Number of transits used to construct Grvs magnitudemeta.numberfloatnullableVbroad? Spectral line broadening parameterkm/sspect.line.broad;spect.linedoublenullablee_Vbroad? Error on the spectral line broadeningkm/sstat.errordoublenullableo_Vbroad? Number of transits used to compute vbroadmeta.numberfloatnullableNSS[0/6] Flag indicating source has additional information in the Gaia DR3 non single star tablesmeta.codeintRVS[0/1] Flag indicating the availability of mean RVS spectrum for this sourcemeta.codeintNameMain accepted cluster namemeta.id.parentcharVarFlagGaia DR3 photometric variability flagmeta.code;src.varchar