Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0 postprint

Author: Rongjun Huang Andrew J. Battisti Kathryn Grasha Elisabete da Cunha Claudia del P Lagos Sarah K. Leslie Emily Wisnioski
Submit Time:2023-02-19 20:58:59

Abstract: Previous studies have shown that the normalization and scatter of the galaxy 'main sequence' (MS), the relation between star formation rate (SFR) and stellar mass ($M_*$), evolves over cosmic time. However, such studies often rely on photometric redshifts and/or only rest-frame UV to near-IR data, which may underestimate the SFR and $M_*$ uncertainties. We use MAGPHYS+photo-z to fit the UV to radio spectral energy distributions of 12,380 galaxies in the COSMOS field at $0.5

Subject: Astronomy >> Astrophysical processes
Cite as: ChinaXiv:202303.02580 (or this version ChinaXiv:202303.02580V1)
DOI:10.12074/202303.02580V1
CSTR:32003.36.ChinaXiv.202303.02580.V1
TXID： df28fc46-e389-450e-8a93-7053805fc245
Recommended references： Rongjun Huang,Andrew J. Battisti,Kathryn Grasha,Elisabete da Cunha,Claudia del P Lagos,Sarah K. Leslie,Emily Wisnioski.Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0.中国科学院科技论文预发布平台.[ChinaXiv:202303.02580V1] (Click&Copy)

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Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0 postprint

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