mcextinct.extsivo://org.gavo.dc/mcextinct/q/extsdoi: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 Extinction values within certain areas in the Magellanic clouds.2011AJ....141..158Hhttp://dc.g-vo.org/tableinfo/mcextinct.exts4/2068 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-19OpticalInfrared0.02mcextinct 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.mcextinct.exts Extinction values within certain areas in the Magellanic clouds.3867bboxBounding box for the extinction datapos.outline;obs.fielddoublenullablecenteralphaArea center RA ICRSdegpos.eq.ra;meta.main5.3051710.347779.30488.743294.52271floatindexednullablecenterdeltaArea center Declination ICRSdegpos.eq.dec;meta.main-74.6606-73.7765-69.919-67.6284-66.72681floatindexednullableev_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.excess0.0610.0680.09150.14150.21951floatnullable