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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
| Title: | 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 | Authors: | Katsianis, A; Gonzalez, V; Barrientos, D; Yang, X; Lagos, C D P; Schaye, J; Camps, P; Trčka, A; Baes, M; Stalevski, Marko   ; |
Issue Date: | 2020 | Publication: | Monthly Notices of the Royal Astronomical Society | ISSN: | 0035-8711 Monthly Notices of the Royal Astronomical Society Search Idenfier |
Type: | Article | Collation: | vol. 492 br. 4 str. 5592-5606 | DOI: | 10.1093/mnras/staa157 | WoS-ID: | 000518148000071 | Scopus-ID: | 2-s2.0-85099605821 | URI: | https://enauka.gov.rs/handle/123456789/150593 | Project: | Shanghai Natural Science Foundation CONICYT/FONDECYT fellowship [3160049] Shanghai Jiao Tong University Tsung-Dao Lee Institute Fellowship National Natural Science Foundation of China [11833005, 11890692, 11621303] |
Metadata source: | (Preuzeto iz Nasi u WoS) Migrirano iz RIS podataka |
M-category: | 21aM21a |
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