mwsce14a.mainivo://org.gavo.dc/mwsc-e14a/q/mainThe GAVO DC teamSchmeja, S.Kharchenko, N.V.Piskunov, A.E.Roeser, S.Schilbach, E.Froebrich, D.Scholz, R.-D.2021-07-20T11:23:30ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837surveysopen-star-clustersstellar-kinematicsgalaxy-structureproper-motions MWSC-e14a ("MWSC extension 2014a") is a catalogue of 139 new open clusters at high Galactic latitudes (\|b\|>20 deg) including lists of candidate members. It extends the Kharchenko et al. 'Catalog of Milky Way Star Clusters'. The target list was compiled as density enhancements found in the 2MASS point source catalogue. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, proper motion, distance, reddening, age, and tidal parameters. .. _Catalog of Milky Way Star Clusters: http://dc.g-vo.org/mwsc/q/clu/form2014A&A...568A..51Shttp://dc.g-vo.org/tableinfo/mwsce14a.main4/21,28-29,48,143,152,166,255,305,309,313,384,387,396,420,443,447,501,510,776,794,796,799,838,853,941,950,994,1014,1070,1213,1284,1286,1337,1372,1436,1439,1461-1462,1514,1540,1545,1575,1643,1666,1673,1696,1723,1860,1873,1875,1878,1920,1922,1926,1929,1932,1938,1948-1949,1951,1992,2010,2016-2017,2019,2024,2041,2044,2050,2057,2154,2308,2310,2314,2316,2337,2340,2391,2399,2420,2422,2444,2474,2551-2552,2560-2561,2563,2568,2577,2581,2686,2714,2738,2740,2744,2753,2756-2757,2759,2768,2772,2775,2778,2782-2783,2793,2825-2826,2862,2944,2953,2958,2966,2983,2994,3004,3007,3050,3052,3054-3055mwsce14a MWSC-e14a ("MWSC extension 2014a") is a catalogue of 139 new open clusters at high Galactic latitudes (\|b\|>20 deg) including lists of candidate members. It extends the Kharchenko et al. 'Catalog of Milky Way Star Clusters'. The target list was compiled as density enhancements found in the 2MASS point source catalogue. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, proper motion, distance, reddening, age, and tidal parameters. .. _Catalog of Milky Way Star Clusters: http://dc.g-vo.org/mwsc/q/clu/formmwsce14a.main MWSC-e14a ("MWSC extension 2014a") is a catalogue of 139 new open clusters at high Galactic latitudes (\|b\|>20 deg) including lists of candidate members. It extends the Kharchenko et al. 'Catalog of Milky Way Star Clusters'. The target list was compiled as density enhancements found in the 2MASS point source catalogue. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, proper motion, distance, reddening, age, and tidal parameters. .. _Catalog of Milky Way Star Clusters: http://dc.g-vo.org/mwsc/q/clu/form782recnoMWSC sequential number (cluster catalog number).meta.id;meta.maincharindexedprimarynameNGC, IC or other common designationmeta.idcharnullableconfirmation_flagIs this object a stellar cluster? 'dupe' indicates the object coincides with another cluster.charobject_typeObject typesrc.classcharnullableot_certainTrue if the object type is confirmed, false if object type has candidate status.meta.code;src.classbooleannullablesourceSource for MWSC list and input parametersmeta.refcharnullablesource_typeObject type from sourcesrc.classcharnullablen_starNumber of stars in MWSC sky area.meta.number00.011195.054257.1799999999716431931.0intraj2000Adopted cluster centre in RA J2000.0degpos.eq.ra;meta.main0.067519.4204167.11343.301359.7720.794397doublenullabledej2000Adopted cluster centre in Dec J2000.0degpos.eq.dec;meta.main-83.445-64.7943-12.325563.774585.2550.794397doublenullableglonGalactic longitudedegpos.galactic.lon0.0088.31210.733351.439359.7640.794397doublenullableglatGalactic latitudedegpos.galactic.lat-89.386-18.2523-0.34616.457384.4930.794397doublenullablercoreAngular radius of the coredegphys.angSize;src0.0090.010.0180.050.50.794397floatnullablercenterAngular radius of the central partdegphys.angSize;src0.020.0350.070.249252.510.794397floatnullablerclusterAngular radius of the clusterdegphys.angSize;src0.040.0650.130.484256.20.794397floatindexednullablepmraAverage proper motion in RA*cos(DE)deg/yrpos.pm;pos.eq.ra;stat.mean-1.12361e-05-2.92736e-06-5.90278e-071.10833e-069.94444e-060.794397floatnullablepmdeAverage proper motion in Declinationdeg/yrpos.pm;pos.eq.dec;stat.mean-1.27778e-05-2.21625e-06-4.05556e-072.03111e-067.61111e-060.794397floatnullablee_pmError of proper motiondeg/yrstat.error;pos.pm;pos.eq.ra;stat.mean8.33333e-095.55556e-081.52778e-074.02778e-078.88889e-070.794397floatnullablervAverage radial velocitykm/sspect.dopplerVeloc;pos.heliocentric;stat.mean-411.4-123.815-4.57113.6474940.25185floatnullablee_rvError of RVkm/sstat.error;spect.dopplerVeloc;pos.heliocentric;stat.mean0.010.12.414.7138570.203488floatnullablen_rvNumber of stars used for RVkm/smeta.number;spect.dopplerVeloc;pos.heliocentric;stat.mean11.02.023.2799999999999731060.1915962intnullablen1s_coreNumber of most probable (1sigma) members within R(core)meta.number01.03.018.01470.7943975intnullablen1s_centerNumber of most probable (1sigma) members within R(center); these are the stars used to compute the average proper motion.meta.number28.030.0185.84999999999999500.7943975intnullablen1s_clusterNumber of most probable (1sigma) members within R(cluster)meta.number717.081.0513.042620.7943975intnullabledistDistance from the Sunpcpos.distance;pos.heliocentric87502.052069.58921.35825350.794397floatindexednullablecol_ex_optColour excess in (B-V)magphot.color.excess;phot.color;em.opt.B;em.opt.V00.0310.572.0823.7270.794397floatnullabledist_modApparent distance modulus in Ksmagphot.mag.distMod4.6988.568411.815.034219.610.794397floatnullablecol_ex_jColour excess in (J-Ks)magphot.color.excess;phot.color;em.ir.J;em.ir.K00.0150.27411.790.794397floatnullablecol_ex_hColour excess in (J-H)magphot.color.excess;phot.color;em.ir.J;em.ir.H00.010.1830.6671.1940.794397floatnullabledelta_hCorrection to H mag of fitted isochrone, empirically introduced to achieve a better fit in the Ks vs. J-H CMD. (see 2012A&A...543A.156K).magphot.mag;arith.diff-0.12-0.0425500.050.120.794397floatnullablelogtLogarithm of average agelog(yr)time.age;stat.mean66.28.6410.110.10.794397floatindexednullablee_logtError in logarithm of average agelog(yr)stat.error;time.age0.0010.0030.040.173920.3430.16834floatnullablentNumber of stars used for log(T) calculationmeta.number01.03.031.6499999999999771490.22357294intnullablercKing core radiuspcphys.size.radius0.080.31.246.62239.10.782505floatnullablee_rcError of King core radiuspcstat.error;phys.size.radius0.030.090.322.31424.090.782505floatnullablertKing tidal radiuspcphys.size.radius0.843.0568.5836.212178.830.782505floatnullablee_rtError of King tidal radiuspcstat.error;phys.size.radius0.140.542.2810.692137.370.782505floatnullablekingkKing normalization factor (a measure of the central density of the cluster, see 2007A&A...468..151Ppc**-2stat.fit.param0.010.245.0950.8552384.030.781977floatnullablee_kingkError of King normalization factorpc**-2stat.error;stat.fit.param0.010.081.1312.4908197.690.781448floatnullablefe_hMetallicity [Fe/H]; this is copied from 2013arXiv1309.4325C or 2012A&A...539A.125D. Data for globular clusters is taken from the revised Harris (1996) catalogue, edition 2010, or newly determined.phys.abund.Fe-2.155-1.887-0.3340.2014290.1280.102273floatindexednullablee_fe_hError of Metallicitystat.error;phys.abund.Fe0.010.010.0950.20.30.0486258floatnullablen_fe_hNumber of objects in [Fe/H] calculation.meta.number11.010.0134.38000000000015800.08192389shortnullablenote_textThe text of the note for an object.meta.notecharnullable