MC extinctionsivo://org.gavo.dc/mcextinct/q/conedoi:10.21938/AvlnaD4AvIeK9nIscpF.YAThe GAVO DC teamHaschke, R.Grebel, E.K.Duffau, S.2012-04-05T00:00:00ZGAVO Data Centre Team

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gavo@ari.uni-heidelberg.de+49 6221 54 1837large-magellanic-cloudinterstellar-extinctioninterstellar-dust A catalogue of E(V-I) extinction values is presented for 3174 (LMC) and 693 (SMC) fields within the Magellanic Clouds. The extinction values were computed by determining the (V-I) colour difference of the red clump from Optical Gravitational Microlensing Experiment (OGLE III) observations in the V and I bands and theoretical values for unreddend red clump colours.2011AJ....141..158Hhttps://dc.g-vo.org/mcextinct/q/cone/infoIsServedByGAVO Data Center TAP service If you use this data, please cite Haschke, R., Grebel, E., Duffau, S., 2011: "New Optical Reddening Maps of the Large and Small Magellanic Clouds", AJ 141, 158, `2011AJ....141..158H <http://adsabs.harvard.edu/abs/2011AJ....141..158H>`_ The photometric data of the red clump is provided by the OGLE collaboration. Part of this research was supported by SFB 881 "The Milky Way System".http://dc.g-vo.org/mcxhttps://dc.g-vo.org/mcxhttp://dc.g-vo.org/mcextinct/q/cone/scs.xml?https://dc.g-vo.org/mcextinct/q/cone/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealev_iReddening (color difference between observation and theory, V-I)magphot.color.excess;em.opt.V;em.opt.Ireal_ADDITEMCheck bands you want extinctions forcharresponseformatFile 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.integer180100000true93.5257-72.80050.001http://dc.g-vo.org/mcextinct/q/cone/capabilitieshttps://dc.g-vo.org/mcextinct/q/cone/capabilitieshttp://dc.g-vo.org/mcextinct/q/cone/availabilityhttps://dc.g-vo.org/mcextinct/q/cone/availabilityhttp://dc.g-vo.org/mcextinct/q/cone/tableMetadatahttps://dc.g-vo.org/mcextinct/q/cone/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/tap4/2068 5/8263,8268-8269,8271,8280,8323,8326,8329,9376,9378 6/33045-33047,33049,33051,33069,33080-33081,33083,33104-33106,33112,33124-33126,33128-33130,33287,33289,33291,33297-33299,33313,33315,33323-33326,33328-33330,37416,37418,375361.986e-19 6.02e-19https://dc.g-vo.org/mcextinct/q/cone/coverageOpticalInfrared0.02mcextinct A catalogue of E(V-I) extinction values is presented for 3174 (LMC) and 693 (SMC) fields within the Magellanic Clouds. The extinction values were computed by determining the (V-I) colour difference of the red clump from Optical Gravitational Microlensing Experiment (OGLE III) observations in the V and I bands and theoretical values for unreddend red clump colours.output A catalogue of E(V-I) extinction values is presented for 3174 (LMC) and 693 (SMC) fields within the Magellanic Clouds. The extinction values were computed by determining the (V-I) colour difference of the red clump from Optical Gravitational Microlensing Experiment (OGLE III) observations in the V and I bands and theoretical values for unreddend red clump colours.row_idArtificial key for this rowmeta.id;meta.mainfloatnullablecenteralphaArea center RA ICRSdegpos.eq.ra;meta.main5.3051710.347779.30488.743294.52271floatnullablecenterdeltaArea center Declination ICRSdegpos.eq.dec;meta.main-74.6606-73.7765-69.919-67.6284-66.72681floatnullableev_iReddening (color difference between observation and theory, V-I)magphot.color.excess;em.opt.V;em.opt.I-0.010.020.070.180.431floatnullablesig_ev_iDifferential reddening calculated as FWHM of the red clump star distributionmagstat.stdev;phot.color.excess0.0610.0680.09150.14150.21951floatnullablebboxBounding box for the extinction datapos.outline;obs.fielddoublenullable