期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 505, 期 1, 页码 540-567出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab1294
关键词
galaxies: evolution; galaxies: general; galaxies: star formation; galaxies: stellar content
资金
- Australian Government Research Training Program (RTP) Scholarship
- Australian Research Council's Future Fellowship scheme [FT200100375, FT200100055]
- Australian Research Council [DP180103740]
- European Union's Horizon 2020 research and innovation programme under the Maria Sklodowska-Curie [754510]
- National Science Centre of Poland [UMO2016/23/N/ST9/02963]
- Spanish Ministry of Science and Innovation through Juan de la Cierva-formacion program [FJC2018-038792-I]
- European Research Council [770935]
- Australian Research Council
- STFC (UK)
- ARC (Australia)
- AAO
- Pawsey Supercomputing Centre
- Australian Government
- Government of Western Australia
- Australian Research Council [FT200100055, FT200100375] Funding Source: Australian Research Council
This study presents high-quality galaxy data from the DEVILS survey, showing the evolution of the galaxy stellar mass function and the SFR-M-star relation to reveal insights about star formation and metallicity evolution. The results indicate significant systematic effects on inferred stellar masses due to improvements in metallicity evolution assumptions. The combination of DEVILS measurements with values from the GAMA survey demonstrates the power of consistent treatment for galaxies at all redshifts.
We present catalogues of stellar masses, star formation rates (SFRs), and ancillary stellar population parameters for galaxies spanning 0 < z < 9 from the Deep Extragalactic VIsible Legacy Survey (DEVILS). DEVILS is a deep spectroscopic redshift survey with very high completeness, covering several premier deep fields including COSMOS (D10). Our stellar mass and SFR estimates are self-consistently derived using the spectral energy distribution (SED) modelling code ProSpect, using well-motivated parametrizations for dust attenuation, star formation histories, and metallicity evolution. We show how these improvements, and especially our physically motivated assumptions about metallicity evolution, have an appreciable systematic effect on the inferred stellar masses, at the level of similar to 0.2 dex. To illustrate the scientific value of these data, we map the evolving galaxy stellar mass function (SMF) and the SFR-M-star relation for 0 < z < 4.25. In agreement with past studies, we find that most of the evolution in the SMF is driven by the characteristic density parameter, with little evolution in the characteristic mass and low-mass slopes. Where the SFR-M-star relation is indistinguishable from a power law at z > 2.6, we see evidence of a bend in the relation at low redshifts (z < 0.45). This suggests evolution in both the normalization and shape of the SFR-M-star relation since cosmic noon. It is significant that we only clearly see this bend when combining our new DEVILS measurements with consistently derived values for lower redshift galaxies from the Galaxy And Mass Assembly (GAMA) survey: this shows the power of having consistent treatment for galaxies at all redshifts.
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