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
| Image |  |
|---|---|
| Description | scholarly article |
| Author/s |
author: Maarten Baes Marko Stalevski Claudia Lagos Joop Schaye |
| Publication date | January 20, 2020 |
| Language | English |
| Country of origin | |
| Wikipedia link | |
| Access work | |
| Copyright status | |
| Missing/wrong data? | Edit Wikidata item |