<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2014-12-11T13:06:00Z" status="active" updated="2024-02-06T08:59:19Z" version="1.2" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://dc.g-vo.org/ColStats-1 http://vo.ari.uni-heidelberg.de/docs/schemata/Colstats.xsd http://www.ivoa.net/xml/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogResource"><title>Optical Polarimetric Catalog for the SMC</title><shortName>polcatsmc.data</shortName><identifier>ivo://org.gavo.dc/polcatsmc/q/data</identifier><curation><publisher>The GAVO DC team</publisher><creator><name>Lobo Gomes, A.</name></creator><creator><name>Magalhães, A. M.</name></creator><creator><name>Pereyra, A.</name></creator><creator><name>Rodrigues, C. V.</name></creator><date role="Updated">2014-12-11T00:00:00Z</date><contact><name>GAVO Data Centre Team</name><address>Mönchhofstrasse 12-14, D-69120 Heidelberg</address><email>gavo@ari.uni-heidelberg.de</email><telephone>+49 6221 54 1837</telephone></contact></curation><content><subject>polarimetry</subject><subject>dwarf-galaxies</subject><subject>magnetic-fields</subject><subject>small-magellanic-cloud</subject><description> 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.</description><source format="bibcode">2015ApJ...806...94L</source><referenceURL>http://dc.g-vo.org/tableinfo/polcatsmc.data</referenceURL></content><facility>Cerro Tololo Inter-American Observatory (CTIO)</facility><coverage><spatial>6/32950-32951,32956-32958,33295,33297-33299,33304-33306,33328</spatial><temporal>48939 48943</temporal><waveband>Optical</waveband></coverage><tableset><schema><name>polcatsmc</name><title>Optical Polarimetric Catalog for the SMC</title><description> 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.</description><table><name>polcatsmc.data</name><description> 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.</description><nrows>7207</nrows><column><name>ct</name><description>Object running number</description><ucd>meta.id;meta.main</ucd><stats><min>1</min><percentile03>217.17999999999998</percentile03><median>3604.0</median><percentile97>6990.82</percentile97><max>7207</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>raj2000</name><description>Object Right Ascension ICRS</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><stats><min>15.0017</min><percentile03>15.0518</percentile03><median>16.8234</median><percentile97>30.3247</percentile97><max>32.5043</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>dej2000</name><description>Object Declination ICRS</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><stats><min>-74.6845</min><percentile03>-74.4829</percentile03><median>-72.6133</median><percentile97>-71.851</percentile97><max>-71.808</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>pol_obs</name><description>Observed polarization in percent of total flux, obtained by determining the Q and U stokes parameters from V photometry in four different angles.</description><stats><min>0.027</min><percentile03>0.20718</percentile03><median>0.963</median><percentile97>3.41664</percentile97><max>5.148</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_pol_obs</name><description>Error in observed polarization including pixel noise. The error is given in percent of the total flux.</description><stats><min>0.001</min><percentile03>0.005</percentile03><median>0.086</median><percentile97>0.62782</percentile97><max>1.55</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pa_pol_obs</name><description>Position angle of the observed polarization</description><unit>deg</unit><stats><min>0.07</min><percentile03>12.67</percentile03><median>106.87</median><percentile97>170.87</percentile97><max>179.97</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pol_int</name><description>Intrinsic 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.</description><stats><min>0.0524</min><percentile03>0.177722</percentile03><median>0.9661</median><percentile97>3.43966</percentile97><max>5.4077</max><fillFactor>0.910087</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_pol_int</name><description>Error on the intrinsic polarisation, including errors on observed polarisation and the estimate of the polarization due to forground dust.</description><stats><min>0.0158</min><percentile03>0.0173</percentile03><median>0.0867</median><percentile97>0.628872</percentile97><max>1.5502</max><fillFactor>0.910087</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pa_pol_int</name><description>Position angle of the intrinsic polarisation</description><unit>deg</unit><stats><min>0.04</min><percentile03>6.6</percentile03><median>97.06</median><percentile97>173.623</percentile97><max>179.93</max><fillFactor>0.910087</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>vmag</name><description>V 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).</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><stats><min>9.6899</min><percentile03>14.5327</percentile03><median>17.8995</median><percentile97>19.5089</percentile97><max>20.6986</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_vmag</name><description>Error in V band magnitude, including photon noise and dispersion in the magnitude calibration.</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.V</ucd><stats><min>0.0004</min><percentile03>0.0219</percentile03><median>0.1104</median><percentile97>0.2502</percentile97><max>0.2707</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>