SATELLITE QUENCHING and GALACTIC CONFORMITY at 0.3 < z < 2.5

Autor: Kawinwanichakij, L, Quadri, RF, Papovich, C, Kacprzak, GG, Labbé, I, Spitler, LR, Straatman, CMS, Tran, KVH, Allen, R, Behroozi, P, Cowley, M, Dekel, A, Glazebrook, K, Hartley, WG, Kelson, DD, Koo, DC, Lee, SK, Lu, Y, Nanayakkara, T, Persson, SE, Primack, J, Tilvi, V, Tomczak, AR, Van Dokkum, P

Publikováno v: Astrophysical Journal, vol 817, iss 1
Kawinwanichakij, L; Quadri, RF; Papovich, C; Kacprzak, GG; Labbé, I; Spitler, LR; et al.(2016). SATELLITE QUENCHING and GALACTIC CONFORMITY at 0.3 < z < 2.5. Astrophysical Journal, 817(1). doi: 10.3847/0004-637X/817/1/9. UC Santa Cruz: Retrieved from: http://www.escholarship.org/uc/item/0734s9bj

We measure the evolution of the quiescent fraction and quenching efficiency of satellites around star-forming and quiescent central galaxies with stellar mass $\log(M_{\mathrm{cen}}/M_{\odot})>10.5$ at $0.39.3$. Satellites for both star-forming and q

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bfa3bfe57e4ee974efd92737d8bb1d5e
https://escholarship.org/uc/item/0734s9bj