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

Author(s):
Boogaard, L.A. (0000-0002-3952-8588); Brinchmann, J. (0000-0003-4359-8797); Bouché, N.; Paalvast, M. (0000-0002-7474-5393); Bacon, R.; Bouwens, R.J. (0000-0002-4989-2471); Contini, T.; Gunawardhana, M.L.P.; Inami, H.; Marino, R.A.; Maseda, M.V. (0000-0003-0695-4414); Mitchell, P.; Nanayakkara, T.; Richard, J.; Schaye, J. (0000-0002-0668-5560); Schreiber, C.; Tacchella, S.; Wisotzki, L.; Zabl, J.
Published
2018
Publication type
Article / Letter to editor
galaxies:star formationgalaxies:formationgalaxies:evolutiongalaxies:ISMmethods:statistical
Date issued
2018
Language
English
Is part of
Astronomy and Astrophysics (2018), Vol. 619, p. A27
hdl
1887/69495
doi
10.1051/0004-6361/201833136
URL
https://ui.adsabs.harvard.edu/#abs/2018A&A...619A..27B