4.7 Article

The 2MASS redshift survey galaxy group catalogue derived from a graph-theory based friends-of-friends algorithm

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/staa1946

关键词

catalogues; surveys; large-scale structure of Universe

资金

  1. SARChI grants
  2. National Research Foundation, under the South Africa Research Chair Initiative
  3. South African Research Chairs Initiative of the Department of Science and Technology
  4. National Research Foundation
  5. NASA
  6. National Science Foundation
  7. Jet Propulsion Laboratory, California Institute of Technology under NASA

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We present the galaxy group catalogue for the recently completed 2MASS Redshift Survey (2MRS; Macri et al. 2019) which consists of 44 572 redshifts, including 1041 new measurements for galaxies mostly located within the Zone of Avoidance. The galaxy group catalogue is generated by using a novel, graph-theory based, modified version of the friends-of-friends algorithm. Several graph-theory examples are presented throughout this paper, including a new method for identifying substructures within groups. The results and graph-theory methods have been thoroughly interrogated against previous 2MRS group catalogues and a Theoretical Astrophysical Observatory (TAO) mock by making use of cutting-edge visualization techniques including immersive facilities, a digital planetarium, and virtual reality. This has resulted in a stable and robust catalogue with on-sky positions and line-of-sight distances within 0.5 and 2 Mpc, respectively, and has recovered all major groups and clusters. The final catalogue consists of 3022 groups, resulting in the most complete 'whole-sky' galaxy group catalogue to date. We determine the 3D positions of these groups, as well as their luminosity and comoving distances, observed and corrected number of members, richness metric, velocity dispersion, and estimates of R-200 and M-200. We present three additional data products, i.e. the 2MRS galaxies found in groups, a catalogue of subgroups, and a catalogue of 687 new group candidates with no counterparts in previous 2MRS-based analyses.

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