MWSC Star Cluster Extension 2014aMWSC-e14a cluivo://org.gavo.dc/mwsc-e14a/q/cluThe 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 Center TeamMönchhofstrasse 12-14, D-69120 Heidelberggavo@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/formhttps://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/infoIsServedByGAVO Data Center TAP servicehttp://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/formhttps://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/formhttp://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/scs.xml?https://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealrecnoMWSC sequential number (cluster catalog number).meta.id;meta.maincharot_certainTrue if the object type is confirmed, false if object type has candidate status.meta.code;src.classcharnameNGC, IC or other common designationmeta.idcharobject_typeObject typesrc.classcharrclusterAngular radius of the clusterdegphys.angSize;srcrealdistDistance from the Sunpcpos.distance;pos.heliocentricreallogtLogarithm of average agelog(yr)time.age;stat.meanrealfe_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.FerealresponseformatFile format requested for output.meta.code.mimecharmaxrecMaximum number of records returned. Pass 0 to retrieve service parameters.integerverbExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integer180100000true4.298086.1830.001http://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/availabilityhttps://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/availabilityhttp://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/capabilitieshttps://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/capabilitieshttp://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/tableMetadatahttps://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/tableMetadatahttp://dc.zah.uni-heidelberg.de/taphttps://dc.zah.uni-heidelberg.de/tap4/21,28-29,48,143,152,166,255,305,309,313,384,387,396,420,443,447,501,510,776,794,796,799,838,853,941,950,994,1014,1070,1213,1284,1286,1337,1372,1436,1439,1461-1462,1514,1540,1545,1575,1643,1666,1673,1696,1723,1860,1873,1875,1878,1920,1922,1926,1929,1932,1938,1948-1949,1951,1992,2010,2016-2017,2019,2024,2041,2044,2050,2057,2154,2308,2310,2314,2316,2337,2340,2391,2399,2420,2422,2444,2474,2551-2552,2560-2561,2563,2568,2577,2581,2686,2714,2738,2740,2744,2753,2756-2757,2759,2768,2772,2775,2778,2782-2783,2793,2825-2826,2862,2944,2953,2958,2966,2983,2994,3004,3007,3050,3052,3054-3055https://dc.zah.uni-heidelberg.de/mwsc-e14a/q/clu/coveragemwsce14aGlobal Survey of Star Clusters in the Milky Way. III. 139 new open
clusters at high Galactic latitudes
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/form
output
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/formmembersLink to stars that are candiadate members of this clustermeta.ref.urlcharnullable_rDistance to cone centerdegpos.distancedoublenullablerecnoMWSC sequential number (cluster catalog number).meta.id;meta.maincharnameNGC, IC or other common designationmeta.idcharnullableconfirmation_flagIs this object a stellar cluster? 'dupe' indicates the object coincides with another cluster.charobject_typeObject typesrc.classcharnullablesourceSource for MWSC list and input parametersmeta.refcharnullablesource_typeObject type from sourcesrc.classcharnullablen_starNumber of stars in MWSC sky area.meta.numberintraj2000Adopted cluster centre in RA J2000.0degpos.eq.ra;meta.maindoublenullabledej2000Adopted cluster centre in Dec J2000.0degpos.eq.dec;meta.maindoublenullableglonGalactic longitudedegpos.galactic.londoublenullableglatGalactic latitudedegpos.galactic.latdoublenullablercoreAngular radius of the coredegphys.angSize;srcfloatnullablercenterAngular radius of the central partdegphys.angSize;srcfloatnullablerclusterAngular radius of the clusterdegphys.angSize;srcfloatnullablepmraAverage proper motion in RA*cos(DE)deg/yrpos.pm;pos.eq.ra;stat.meanfloatnullablepmdeAverage proper motion in Declinationdeg/yrpos.pm;pos.eq.dec;stat.meanfloatnullablee_pmError of proper motiondeg/yrstat.error;pos.pm;pos.eq.ra;stat.meanfloatnullablervAverage radial velocitykm/sspect.dopplerVeloc;pos.heliocentric;stat.meanfloatnullablee_rvError of RVkm/sstat.error;spect.dopplerVeloc;pos.heliocentric;stat.meanfloatnullablen1s_coreNumber of most probable (1sigma) members within R(core)meta.numberintnullablen1s_centerNumber of most probable (1sigma) members within R(center); these are the stars used to compute the average proper motion.meta.numberintnullablen1s_clusterNumber of most probable (1sigma) members within R(cluster)meta.numberintnullabledistDistance from the Sunpcpos.distance;pos.heliocentricfloatnullablecol_ex_optColour excess in (B-V)magphot.color.excess;phot.color;em.opt.B;em.opt.VfloatnullablelogtLogarithm of average agelog(yr)time.age;stat.meanfloatnullablercKing core radiuspcphys.size.radiusfloatnullablertKing tidal radiuspcphys.size.radiusfloatnullablekingkKing normalization factor (a measure of the central density of the cluster, see 2007A&A...468..151Ppc**-2stat.fit.paramfloatnullablefe_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.Fefloatnullablenote_textThe text of the note for an object.meta.notecharnullable