The stellar mass function of galaxies in Planck -selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching (2018)
Attributed to:
Astrophysics at the University of Birmingham: Consolidated Grant 2016-2019
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201833572
Publication URI: http://dx.doi.org/10.1051/0004-6361/201833572
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics