1. Non-linearity and environmental dependence of the star-forming galaxies main sequence
- Author
-
Erfanianfar, G, Popesso, P, Finoguenov, A, Wilman, D, Wuyts, S, Biviano, A, Salvato, M, Mirkazemi, M, Morselli, L, Ziparo, F, Nandra, K, Lutz, D, Elbaz, D, Dickinson, M, Tanaka, M, Altieri, MB, Aussel, H, Bauer, F, Berta, S, Bielby, RM, Brandt, N, Cappelluti, N, Cimatti, A, Cooper, MC, Fadda, D, Ilbert, O, Le Floch, E, Magnelli, B, Mulchaey, JS, Nordon, R, Newman, JA, Poglitsch, A, and Pozzi, F
- Subjects
Space Sciences ,Particle and High Energy Physics ,Astronomical Sciences ,Physical Sciences ,Galaxy: evolution ,Galaxy: structure ,galaxies: groups: general ,galaxies: haloes ,galaxies: star formation ,infrared: galaxies ,astro-ph.GA ,Astronomical and Space Sciences ,Astronomy & Astrophysics ,Astronomical sciences ,Particle and high energy physics ,Space sciences - Abstract
Using data from four deep fields (COSMOS, AEGIS, ECDFS, and CDFN), we studythe correlation between the position of galaxies in the star formation rate(SFR) versus stellar mass plane and local environment at $z10^{10.4-10.6}$ $M_{\odot}$), across all environments. At high redshift ($0.5
- Published
- 2016