The high-redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: towards addressing the tension between observations and simulations (2020)
Attributed to:
DiRAC 2.5y Bridging Funding - UCL
funded by
STFC
Abstract
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Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa157
Publication URI: http://dx.doi.org/10.1093/mnras/staa157
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 4