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<dri:objIdentifier>od________18::003d7b0e3c03f1501356d87b54b05185</dri:objIdentifier>
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<dri:dateOfCollection>2015-06-27T13:09:14.91Z</dri:dateOfCollection>
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<dri:dateOfTransformation>2017-08-22T08:16:32.855Z</dri:dateOfTransformation>
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<oaf:result>
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<dateofacceptance>2012-02-28</dateofacceptance>
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<description>Using the photometric redshifts of galaxies from the Sloan Digital Sky
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Survey III (SDSS-III), we identify 132,684 clusters in the redshift range of.
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Monte Carlo simulations show that the false detection rate is less than 6% for
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the whole sample. The completeness is more than 95% for clusters with a mass of
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M_{200}>1.0*10^{14} M_{\\odot} in the redshift range of , while clusters of
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z>0.42 are less complete and have a biased smaller richness than the real one
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due to incompleteness of member galaxies. We compare our sample with other
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cluster samples, and find that more than 90% of previously known rich clusters
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of 0.052 are matched with clusters in our sample. Richer clusters tend to have
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more luminous brightest cluster galaxies (BCGs). Correlating with X-ray and the
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Planck data, we show that the cluster richness is closely related to the X-ray
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luminosity, temperature and Sunyaev-Zel'dovich measurements. Comparison of the
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BCGs with the SDSS luminous red galaxy (LRG) sample shows that 25% of LRGs are
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BCGs of our clusters and 36% of LRGs are cluster member galaxies. In our cluster
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sample, 63% of BCGs of r_{petro} satisfy the SDSS LRG selection
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criteria.</description>
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schemename="dnet:languages"/>
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<subject classid="arxiv" classname="arxiv"
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schemeid="dnet:subject_classification_typologies"
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schemename="dnet:subject_classification_typologies" inferred="true"
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inferenceprovenance="iis::document_classes" provenanceaction="iis" trust="0.891"
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>Astrophysics::Galaxy Astrophysics</subject>
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<subject classid="arxiv" classname="arxiv"
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schemeid="dnet:subject_classification_typologies"
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schemename="dnet:subject_classification_typologies" inferred="true"
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inferenceprovenance="iis::document_classes" provenanceaction="iis" trust="0.891"
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>Astrophysics::Cosmology and Extragalactic Astrophysics</subject>
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schemeid="dnet:subject_classification_typologies"
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schemename="dnet:subject_classification_typologies">Astrophysics - Cosmology and
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Nongalactic Astrophysics</subject>
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<title classid="main title" classname="main title" schemeid="dnet:dataCite_title"
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schemename="dnet:dataCite_title">A catalog of 132,684 clusters of galaxies
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identified from Sloan Digital Sky Survey III</title>
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id="opendoar____::6f4922f45568161a8cdf4ad2299f6d23"/>
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<originalId>oai:arXiv.org:1202.6424</originalId>
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<pid classid="doi" classname="doi" schemeid="dnet:pid_types"
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schemename="dnet:pid_types">10.1088/0067-0049/199/2/34</pid>
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<fullname>Liu, F. S.</fullname>
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<ranking>2</ranking>
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<fullname>Han, J. L.</fullname>
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provenanceaction="sysimport:crosswalk:repository">
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<fullname>Wen, Z. L.</fullname>
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<url>http://arxiv.org/abs/1202.6424</url>
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