D-Net

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   <oaf:dateofacceptance>2012-02-28</oaf:dateofacceptance>

   <oaf:description>Using the photometric redshifts of galaxies from the Sloan Digital Sky

                    Survey III (SDSS-III), we identify 132,684 clusters in the redshift range of.

                    Monte Carlo simulations show that the false detection rate is less than 6% for

                    the whole sample. The completeness is more than 95% for clusters with a mass of

                    M_{200}>1.0*10^{14} M_{\\odot} in the redshift range of , while clusters of

                    z>0.42 are less complete and have a biased smaller richness than the real one

                    due to incompleteness of member galaxies. We compare our sample with other

                    cluster samples, and find that more than 90% of previously known rich clusters

                    of 0.052 are matched with clusters in our sample. Richer clusters tend to have

                    more luminous brightest cluster galaxies (BCGs). Correlating with X-ray and the

                    Planck data, we show that the cluster richness is closely related to the X-ray

                    luminosity, temperature and Sunyaev-Zel'dovich measurements. Comparison of the

                    BCGs with the SDSS luminous red galaxy (LRG) sample shows that 25% of LRGs are

                    BCGs of our clusters and 36% of LRGs are cluster member galaxies. In our cluster

                    sample, 63% of BCGs of r_{petro} satisfy the SDSS LRG selection

                    criteria.</oaf:description>

   <oaf:language code="eng">English</oaf:language>

   <oaf:resulttype>publication</oaf:resulttype>

   <oaf:subject type="arxiv" provenance="inference">Astrophysics::Galaxy Astrophysics</oaf:subject>

   <oaf:subject type="arxiv" provenance="inference">Astrophysics::Cosmology and Extragalactic Astrophysics</oaf:subject>

   <oaf:subject type="keyword">Astrophysics - Cosmology and

                    Nongalactic Astrophysics</oaf:subject>

   <oaf:resulttitle>A catalog of 132,684 clusters of galaxies

                    identified from Sloan Digital Sky Survey III</oaf:resulttitle>

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   <oaf:originalId>oai:arXiv.org:1202.6424</oaf:originalId>

   <oaf:pid type="doi">10.1088/0067-0049/199/2/34</oaf:pid>

   <oaf:bestaccessrights code="OPEN">Open Access</oaf:bestaccessrights>

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   <oaf:creator rank="3">Liu, F. S.</oaf:creator>

   <oaf:creator rank="2">Han, J. L.</oaf:creator>

   <oaf:creator rank="1">Wen, Z. L.</oaf:creator>

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            <oaf:url>http://arxiv.org/abs/1202.6424</oaf:url>

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