Flux- and volume-limited groups/clusters for the SDSS galaxies: catalogues and mass estimation
arXiv:1402.1350 · doi:10.1051/0004-6361/201423585
Abstract
We provide flux-limited and volume-limited galaxy group and cluster catalogues, based on the spectroscopic sample of the SDSS data release 10 galaxies. We used a modified friends-of-friends (FoF) method with a variable linking length in the transverse and radial directions to identify as many realistic groups as possible. The flux-limited catalogue incorporates galaxies down to m_r = 17.77 mag. It includes 588193 galaxies and 82458 groups. The volume-limited catalogues are complete for absolute magnitudes down to M_r = -18.0, -18.5, -19.0, -19.5, -20.0, -20.5, and -21.0; the completeness is achieved within different spatial volumes, respectively. Our analysis shows that flux-limited and volume-limited group samples are well compatible to each other, especially for the larger groups/clusters. Dynamical mass estimates, based on radial velocity dispersions and group extent in the sky, are added to the extracted groups. The catalogues can be accessed via http://cosmodb.to.ee and the Strasbourg Astronomical Data Center (CDS).
16 pages, 18 figures, 2 tables, accepted for publication in A&A
References in corpus (15)
- K-corrections and filter transformations in the ultraviolet, optical, and near infrared
- Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
- Concentration, Spin and Shape of Dark Matter Haloes as a Function of the Cosmological Model: WMAP1, WMAP3 and WMAP5 results
- A GMBCG Galaxy Cluster Catalog of 55,424 Rich Clusters from SDSS DR7
- CIRS: Cluster Infall Regions in the Sloan Digital Sky Survey I. Infall Patterns and Mass Profiles
- Galaxy And Mass Assembly (GAMA): The large scale structure of galaxies and comparison to mock universes
- The dependence of the galaxy mass-metallicity relation on environment and the implied metallicity of the IGM
- Galaxy Cluster Mass Reconstruction Project: I. Methods and first results on galaxy-based techniques
- Groups of galaxies in the SDSS Data Release 5. A group-finder and a catalogue
- SDSS superclusters: morphology and galaxy content
- Anatomy of luminosity functions: the 2dFGRS example
- How well does the Friends-of-Friends algorithm recover group properties from galaxy catalogs limited in both distance and luminosity?
- The Virial Mass Function of Nearby SDSS Galaxy Clusters
- First Galaxy-Galaxy Lensing Measurement of Satellite Halo Mass in the CFHT Stripe-82 Survey
- Central galaxies in different environments: Do they have similar properties?
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