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ivo-id="ivo://CDS">CDS</publisher><creator><name>Parisi M.C.</name></creator><creator><name>Geisler D.</name></creator><creator><name>Grocholski A.J.</name></creator><creator><name>Claria J.J.</name></creator><creator><name>Sarajedini A.</name></creator><date role="Updated">2012-09-11T14:00:17Z</date><date role="Created">2012-06-07T15:04:00Z</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>magellanic-clouds</subject><subject>stellar-associations</subject><subject>giant-stars</subject><subject>line-intensities</subject><description>We have obtained metallicities of ~360 red giant stars distributed in 15 Small Magellanic Cloud (SMC) fields from near-infrared spectra covering the CaII triplet lines using the VLT + FORS2.</description><source 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