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II.</title><shortName>J/AJ/141/61</shortName><identifier>ivo://CDS.VizieR/J/AJ/141/61</identifier><altIdentifier>doi:10.26093/cds/vizier.51410061</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Caldwell N.</name></creator><creator><name>Schiavon R.</name></creator><creator><name>Morrison H.</name></creator><creator><name>Rose J.A.</name></creator><creator><name>Harding P.</name></creator><date role="Updated">2017-12-05T05:10:12Z</date><date role="Created">2012-08-15T11:32:22Z</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>galaxies</subject><subject>stellar-associations</subject><subject>metallicity</subject><subject>radial-velocity</subject><description>We present new high signal-to-noise spectroscopic data on the M31 globular cluster (GC) system, obtained with the Hectospec multifiber spectrograph on the 6.5m MMT. More than 300 clusters have been observed at a resolution of 5{AA} and with a median S/N of 75 per{AA}, providing velocities with a median uncertainty of 6km/s. The primary focus of this paper is the determination of mean cluster metallicities, ages, and reddenings. 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