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相关论文: Groups of galaxies in the SDSS Data Release 5. A g…

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Aims. We intend to compile a new galaxy group and cluster sample of the latest available SDSS data, adding several parameter for the purpose of studying the supercluster network, galaxy and group evolution, and their connection to the…

宇宙学与河外天体物理 · 物理学 2012-02-29 E. Tempel , E. Tago , L. J. Liivamägi

We create a new catalogue of groups and clusters for the 2dF GRS final release sample. We show that the variable linking length friends-of-friends (FoF) algorithms used so far yield groups with sizes that grow systematically with distance…

天体物理学 · 物理学 2009-11-10 E. Tago , J. Einasto , M. Einasto , E. Saar

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…

宇宙学与河外天体物理 · 物理学 2014-06-04 E. Tempel , A. Tamm , M. Gramann , T. Tuvikene , L. J. Liivamägi , I. Suhhonenko , R. Kipper , M. Einasto , E. Saar

We identify galaxy groups and clusters in volume-limited samples of the SDSS redshift survey, using a redshift-space friends-of-friends algorithm. We optimize the friends-of-friends linking lengths to recover galaxy systems that occupy the…

In this work we introduce a new method to perform the identification of groups of galaxies and present results of the identification of galaxy groups in the Seventh Data Release of the Sloan Digital Sky Survey (SDSS-DR7). Our methodology…

宇宙学与河外天体物理 · 物理学 2012-03-23 J. C. Muñoz-Cuartas , Volker Mueller

We apply a friends-of-friends algorithm to an enhanced SDSS DR12 spectroscopic catalog including redshift from literature to construct a catalog of $1588~N\ge3$ compact groups of galaxies containing 5179 member galaxies and covering the…

星系天体物理 · 物理学 2016-08-17 Jubee Sohn , Margaret J. Geller , Ho Seong Hwang , H. Jabran Zahid , Myung Gyoon Lee

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 combination of two methods is used to identify the centers of…

天体物理学 · 物理学 2009-07-28 Xiaohu Yang , H. J. Mo , Frank C. van den Bosch , Anna Pasquali , Cheng Li , Marco Barden

We present a catalogue of galaxy groups and clusters selected using a friends-of-friends algorithm with a dynamic linking length from the 2dF-SDSS and QSO (2SLAQ) luminous red galaxy survey. The linking parameters for the code are chosen…

宇宙学与河外天体物理 · 物理学 2015-05-28 S. Farrens , F. B. Abdalla , E. S. Cypriano , C. Sabiu , C. Blake

We present a large catalog of loose groups of galaxies in the Southern Galactic Hemisphere, selected from the Perseus-Pisces redshift Survey (PPS). Particular care is taken in order to obtain group samples as homogeneous as possible to…

天体物理学 · 物理学 2009-10-30 Roberto Trasarti-Battistoni

I review here past and present research on clusters and groups of galaxies within the Sloan Digital Sky Survey (SDSS). In particular, I discuss the C4 algorithm which is designed to search for clusters within a 7-dimensional data-space,…

天体物理学 · 物理学 2007-05-23 Robert C. Nichol

We present a new sample of galaxy groups identified in the Sloan Digital Sky Survey Data Release 3. Following previous works we use the well tested friend-of-friend algorithm developed by Huchra & Geller which take into account the number…

天体物理学 · 物理学 2014-09-26 Manuel Merchan , Ariel Zandivarez

Recent large-scale galaxy spectroscopic surveys, such as the Sloan Digital Sky Survey (SDSS), enable us to execute a systematic, relatively-unbiased search for galaxy clusters. Such surveys make it possible to measure the 3-d distribution…

天体物理学 · 物理学 2009-11-13 Joo H. Yoon , Kevin Schawinski , Yun-Kyeong Sheen , Chang H. Ree , Sukyoung K. Yi

We present an automated method to detect populations of groups in galaxy redshift catalogs. This method uses both analysis of the redshift distribution along lines of sight in fixed cells to detect elementary structures and a…

天体物理学 · 物理学 2009-11-07 C. Adami , A. Mazure

Galaxy groups and clusters are the main tools used to test cosmological models and to study the environmental effect of galaxy formation. This work provides a catalogue of galaxy groups and clusters, as well as potentially merging systems…

宇宙学与河外天体物理 · 物理学 2017-06-21 Elmo Tempel , Taavi Tuvikene , Rain Kipper , Noam I. Libeskind

Clusters of galaxies in most previous catalogs have redshifts z<0.3. Using the photometric redshifts of galaxies from the Sloan Digital Sky Survey Data Release 6 (SDSS DR6), we identify 39,668 clusters in the redshift range 0.05< z <0.6…

宇宙学与河外天体物理 · 物理学 2014-11-20 Z. L. Wen , J. L. Han , F. S. Liu

A ``friends-of-friends'' percolation algorithm has been used to extract a catalogue of dn/n = 80 density enhancements (groups) from the six slices of the Las Campanas Redshift Survey (LCRS). The full catalogue contains 1495 groups and…

We present the largest publicly available catalogue of compact groups of galaxies identified using the original selection criteria of Hickson, selected from the Sixth Data Release (DR6) of the Sloan Digital Sky Survey (SDSS). We identify…

天体物理学 · 物理学 2009-11-13 Alan McConnachie , David Patton , Sara Ellison , Luc Simard

We have constructed a set of supercluster catalogues for the galaxies from the SDSS survey main and luminous red galaxy (LRG) flux-limited samples. To delineate superclusters, we calculated luminosity density fields using the B3-spline…

宇宙学与河外天体物理 · 物理学 2012-01-17 L. J. Liivamägi , E. Tempel , E. Saar

Context. Friends-of-friends algorithms are a common tool to detect galaxy groups and clusters in large survey data. In order to be as precise as possible, they have to be carefully calibrated using mock catalogues. Aims. We create an…

宇宙学与河外天体物理 · 物理学 2016-11-23 Christoph Saulder , Eelco van Kampen , Igor V. Chilingarian , Steffen Mieske , Werner W. Zeilinger

We use the Updated Zwicky Catalog of galaxies (Falco et al. 1999) to generate a catalog of groups, by means of a friend-of-friend algorithm. The correlation length of the total sample is well fitted with a power law $ \xi(r)=(r/r_0)^\gamma…

天体物理学 · 物理学 2009-10-31 Manuel E. Merchan , Marcio A. G. Maia , Diego G. Lambas
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