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20062009
most citedGalaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties

995 citations · 1.7k across the 6 of their papers we have counts for

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6 papers

astro-ph.CO2009136 cited

Structural Properties of Central Galaxies in Groups and Clusters

Yicheng Guo, Daniel H. McIntosh, H. J. Mo +6

Using a representative sample of 911 central galaxies (CENs) from the SDSS DR4 group catalogue, we study how the structure of the most massive members in groups and clusters depend…

astro-ph200830 cited

Alignments of Group Galaxies with Neighboring Groups

Yougang Wang, Changbom Park, Xiaohu Yang +2

Using a sample of galaxy groups found in the Sloan Digital Sky Survey Data Release 4, we measure the following four types of alignment signals: (1) the alignment between the distri…

astro-ph200830 cited

Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups

Ran Li, H. J. Mo, Zuhui Fan +4

We use galaxy groups selected from the Sloan Digital Sky Survey (SDSS) together with mass models for individual groups to study the galaxy-galaxy lensing signals expected from gala…

astro-ph2007172 cited

Ongoing Assembly of Massive Galaxies by Major Merging in Large Groups and Clusters from the SDSS

Daniel H. McIntosh, Yicheng Guo, Jen Hertzberg +4

We investigate the incidence of major mergers creating >10e11 Msun galaxies in present-day groups and clusters more massive than 2.5e13 Msun. We identify 38 pairs of massive galaxi…

astro-ph2007995 cited

Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties

Xiaohu Yang, H. J. Mo, Frank C. van den Bosch +3

We use a modified version of the halo-based group finder developed by Yang et al. to select galaxy groups from the Sloan Digital Sky Survey (SDSS DR4). In the first step, a combina…

astro-ph2006289 cited

Towards a Concordant Model of Halo Occupation Statistics

Frank C. van den Bosch, Xiaohu Yang, H. J. Mo +6

We use the conditional luminosity function (CLF) and data from the 2dFGRS to constrain the average relation between light and mass in a LCDM cosmology with Omega_m=0.23 and sigma_8…