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<ri:Resource created="2014-02-27T15:32:52Z" status="active" updated="2025-06-13T15:25:00Z" 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>Metallicity and kinematics in Galactic bar</title><shortName>J/A+A/563/A15</shortName><identifier>ivo://CDS.VizieR/J/A+A/563/A15</identifier><altIdentifier>doi:10.26093/cds/vizier.35630015</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Babusiaux C.</name></creator><creator><name>Katz D.</name></creator><creator><name>Hill V.</name></creator><creator><name>Royer F.</name></creator><creator><name>Gomez A.</name></creator><creator><name>Arenou F.</name></creator><creator><name>Combes F.,Di Matteo P.</name></creator><creator><name>Gilmore G.</name></creator><creator><name>Haywood M.</name></creator><creator><name>Robin A.C.</name></creator><creator><name>Rodriguez-Fernandez N.,Sartoretti P. Schultheis M.</name></creator><date role="Updated">2014-08-23T18:23:47Z</date><date role="Created">2014-02-27T15:32:52Z</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>galaxy-planes</subject><subject>milky-way-galaxy</subject><subject>metallicity</subject><subject>radial-velocity</subject><description>We observe red clump stars in four fields along the Galactic bar major axis (l=10{deg}, -6{deg}, 6{deg} and b=0{deg}, plus a field at l=0{deg}, b=1{deg}) with low-resolution spectroscopy from FLAMES/GIRAFFE (setup LR08) at the VLT, observing around the CaII triplet. We developed robust methods to extract radial velocity and metallicity estimates from these low signal-to-noise spectra. Results have been derived by fixing atmospheric parameters typical of a red clump star (Teff=4750K, logg=2.5). For some targets, the metallicity could not be derived.</description><source format="bibcode">2014A&amp;A...563A..15B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/563/A15</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/349/1059">J/MNRAS/349/1059 : OGLE variables in Galactic bar (Wray+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/691/1387">J/ApJ/691/1387 : Spectroscopy of the Galactic bar. I. 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