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Cosmic Web of Galaxies in the COSMOS Field: Public Catalog and Different Quenching for Centrals and Satellites

  • Authors: Behnam Darvish, Bahram Mobasher, D. Christopher Martin, David Sobral, Nick Scoville, Andra Stroe, Shoubaneh Hemmati, and Jeyhan Kartaltepe

2017 The Astrophysical Journal 837 16.

  • Provider: AAS Journals

Caption: Figure 8.

Number of groups Ngroup as a function of the projected linking length in units of the median projected intergalaxy separation (b) for a fixed α = 1.5 (Section 3.5). The number of groups for small b values is low because only a small number of galaxies are too close to link together. On the other hand, for large values of b, Ngroup is also small because many galaxies link together to form percolated structures. By fixing α = 1.5, the number of selected groups maximizes at b ∼ 1.3 and we use it as a suitable trade-off linking length for our group selection.

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