The specific star formation rate function at different mass scales and quenching: a comparison between cosmological models and SDSS (2021)
Attributed to:
DiRAC 2.5y Bridging Funding - UCL
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa3236
Publication URI: http://dx.doi.org/10.1093/mnras/staa3236
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 2