The MUSE Hubble Ultra Deep Field Survey. XI. Constraining the low-mass end of the stellar mass - star formation rate relation at z < 1

The MUSE Hubble Ultra Deep Field Survey. XI. Constraining the low-mass end of the stellar mass - star formation rate relation at z < 1

Star-forming galaxies have been found to follow a relatively tight relation between stellar mass (M*) and star formation rate (SFR), dubbed the “star formation sequence”. A turnover in the sequence has been observed, where galaxies with M* <  1010 M⊙ follow a steeper relation than their highe...

Full description

Bibliographic Details
Main Authors: Boogaard, L, Brinchmann, J, Bouché, N, Paalvast, M, Bacon, R, Bouwens, R, Contini, T, Gunawadhana, M, Inami, H, Marino, R, Maseda, M, Mitchell, P, Nanayakkara, T, Richard, J, Schaye, J, Schreiber, C, Tacchella, S, Wisotzki, L, Zabl, J
Format: Journal article
Published: EDP Sciences 2018

Similar Items