PolCatSMCivo://org.gavo.dc/polcatsmc/q/coneThe GAVO DC teamLobo Gomes, A.Magalhães, A. M.Pereyra, A.Rodrigues, C. V.2014-12-11T00:00:00ZGAVO Data Centre Team

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gavo@ari.uni-heidelberg.de+49 6221 54 1837polarimetrydwarf-galaxiesmagnetic-fieldssmall-magellanic-cloud An optical polarimetric catalog for the Small Magelanic Cloud (SMC) is presented. It gives intrinsic and observed polarizations in the V-band for a total of 7207 stars located in the Northeast and Wing sections of the SMC and part of the Magellanic Bridge.2015ApJ...806...94Lhttp://dc.g-vo.org/polcatsmc/q/cone/infoIsServedByGAVO Data Center TAP servicehttp://dc.g-vo.org/polcatsmc/q/cone/scs.xml?https://dc.g-vo.org/polcatsmc/q/cone/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealpol_intIntrinsic polarisation in per cent of total flux, obtained by substracting the foreground polarization due to Milky Way dust from the observed polarization pol_obs. See paper, chapter 3, for details on foreground determination.realpol_obsObserved polarization in percent of total flux, obtained by determining the Q and U stokes parameters from V photometry in four different angles.realvmagV band magnitude obtained by summing up the flux of the image pair in one frame and calibrating against several published catalogs (see Table 3 in the paper).magphot.mag;em.opt.VrealresponseformatFile 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.integer180100000true26.322542-74.54141670.01http://dc.g-vo.org/polcatsmc/q/cone/formhttps://dc.g-vo.org/polcatsmc/q/cone/formhttp://dc.g-vo.org/polcatsmc/q/cone/capabilitieshttps://dc.g-vo.org/polcatsmc/q/cone/capabilitieshttp://dc.g-vo.org/polcatsmc/q/cone/availabilityhttps://dc.g-vo.org/polcatsmc/q/cone/availabilityhttp://dc.g-vo.org/polcatsmc/q/cone/tableMetadatahttps://dc.g-vo.org/polcatsmc/q/cone/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/tapCerro Tololo Inter-American Observatory (CTIO)6/32950-32951,32956-32958,33295,33297-33299,33304-33306,3332848939 48943http://dc.g-vo.org/polcatsmc/q/cone/coverageOpticalpolcatsmc An optical polarimetric catalog for the Small Magelanic Cloud (SMC) is presented. It gives intrinsic and observed polarizations in the V-band for a total of 7207 stars located in the Northeast and Wing sections of the SMC and part of the Magellanic Bridge.polcatsmc.data An optical polarimetric catalog for the Small Magelanic Cloud (SMC) is presented. It gives intrinsic and observed polarizations in the V-band for a total of 7207 stars located in the Northeast and Wing sections of the SMC and part of the Magellanic Bridge.7207ctObject running numbermeta.id;meta.main1217.179999999999983604.06990.8272071.0intraj2000Object Right Ascension ICRSdegpos.eq.ra;meta.main15.001715.051816.823430.324732.50431doubleindexednullabledej2000Object Declination ICRSdegpos.eq.dec;meta.main-74.6845-74.4829-72.6133-71.851-71.8081doubleindexednullablepol_obsObserved polarization in percent of total flux, obtained by determining the Q and U stokes parameters from V photometry in four different angles.0.0270.207180.9633.416645.1481floatnullablee_pol_obsError in observed polarization including pixel noise. The error is given in percent of the total flux.0.0010.0050.0860.627821.551floatnullablepa_pol_obsPosition angle of the observed polarizationdeg0.0712.67106.87170.87179.971floatnullablepol_intIntrinsic polarisation in per cent of total flux, obtained by substracting the foreground polarization due to Milky Way dust from the observed polarization pol_obs. See paper, chapter 3, for details on foreground determination.0.05240.1777220.96613.439665.40770.910087floatnullablee_pol_intError on the intrinsic polarisation, including errors on observed polarisation and the estimate of the polarization due to forground dust.0.01580.01730.08670.6288721.55020.910087floatnullablepa_pol_intPosition angle of the intrinsic polarisationdeg0.046.697.06173.623179.930.910087floatnullablevmagV band magnitude obtained by summing up the flux of the image pair in one frame and calibrating against several published catalogs (see Table 3 in the paper).magphot.mag;em.opt.V9.689914.532717.899519.508920.69861floatnullablee_vmagError in V band magnitude, including photon noise and dispersion in the magnitude calibration.magstat.error;phot.mag;em.opt.V0.00040.02190.11040.25020.27071floatnullable