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<ri:Resource created="2017-12-18T07:21:56Z" status="active" updated="2025-09-17T20:00:36Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.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:CatalogService"><title>Southern Hemisphere ISM FORS2 spectropolarimetry</title><shortName>J/A+A/608/A146</shortName><identifier>ivo://CDS.VizieR/J/A+A/608/A146</identifier><altIdentifier>doi:10.26093/cds/vizier.36080146</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bagnulo S.</name></creator><creator><name>Cox N.L.J.</name></creator><creator><name>Cikota A.</name></creator><creator><name>Siebenmorgen R.</name></creator><creator><name>Voshchinnikov N.V.,Patat F.</name></creator><creator><name>Smith K.T.</name></creator><creator><name>Smoker J.V.</name></creator><creator><name>Tautenberger S.</name></creator><creator><name>Kaper L.</name></creator><creator><name>Cami J.</name></creator><date role="Updated">2025-09-17T20:00:36Z</date><date role="Created">2017-12-18T07:21:56Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>interstellar-medium</subject><subject>polarimetry</subject><description>Polarimetric studies of light transmitted through interstellar clouds may give constraints on the properties of the interstellar dust grains. Traditionally, broadband linear polarisation (BBLP) measurements have been considered an important diagnostic tool for the study of the interstellar dust, while comparatively less attention has been paid to spectropolarimetric measurements. However, spectropolarimetry may offer stronger constraints than BBLP, for example by revealing narrowband features, and by allowing us to distinguish the contribution of dust from the contribution of interstellar gas. Therefore, we have decided to carry out a Large Interstellar Polarisation Survey (LIPS) using spectropolarimetric facilities in both hemispheres. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Obs</name><description>Observation date</description><unit>s</unit><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>P(B)</name><description>? Polarisation in the B filter</description><unit>%</unit><ucd>phys.polarization.linear</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>theta(B)</name><description>? Position angle of the polarisation in the B filter</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>P(V)</name><description>Polarisation in the V filter</description><unit>%</unit><ucd>phys.polarization.linear</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>theta(V)</name><description>Position angle of the polarisation in the V filter</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>P(R)</name><description>Polarisation in the R filter</description><unit>%</unit><ucd>phys.polarization.linear</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>theta(R)</name><description>Position angle of the polarisation in the R filter</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>P(I)</name><description>Polarisation in the I filter</description><unit>%</unit><ucd>phys.polarization.linear</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>theta(I)</name><description>Position angle of the polarisation in the I filter</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>K</name><description>? Parameter K of the Serkowski curve</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_K</name><description>? Error on the parameter K of the Serkowski curve</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lmax</name><description>? Wavelength at which polarisation is maximum</description><unit>nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Lmax</name><description>? Error on wavelength at which polarisation is maximum</description><unit>nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Pmax</name><description>? Maximum of the polarisation</description><unit>%</unit><ucd>phys.polarization;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Pmax</name><description>? Error on maximum of polarisation</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dT/dl</name><description>Gradient of the polarisation position angle in degree/100nm</description><unit>0.01deg.nm**-1</unit><ucd>arith.grad;pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dT/dl</name><description>Error on gradient of the polarisation position angle in degree/100nm</description><unit>0.01deg.nm**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TARFILE</name><description>Name of the tar file with the data in subdirectory sp (1)</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="30*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>