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Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey

Bourne, N.; Dunlop, J.S.; Merlin, E.; Parsa, S.; Schreiber, C.; Castellano, M.; Conselice, Christopher J.; Coppin, K.E.K.; Farrah, D.; Fontana, A.; Geach, J.E.; Halpern, M.; Knudsen, K.K.; Michałowski, M.J.; Mortlock, A.; Santini, P.; Scott, D.; Shu, X.W.; Simpson, C.; Simpson, J.M.; Smith, D.J.B.; van der Werf, P.P.

Authors

N. Bourne

J.S. Dunlop

E. Merlin

S. Parsa

C. Schreiber

M. Castellano

Christopher J. Conselice

K.E.K. Coppin

D. Farrah

A. Fontana

J.E. Geach

M. Halpern

K.K. Knudsen

M.J. Michałowski

A. Mortlock

P. Santini

D. Scott

X.W. Shu

C. Simpson

J.M. Simpson

D.J.B. Smith

P.P. van der Werf



Abstract

We present a new exploration of the cosmic star formation history and dust obscuration in massive galaxies at redshifts 0.5 < z < 6. We utilize the deepest 450- and 850-μm imaging from SCUBA-2 CLS, covering 230 arcmin2 in the AEGIS, COSMOS and UDS fields, together with 100–250 μm imaging from Herschel. We demonstrate the capability of the t-phot deconfusion code to reach below the confusion limit, using multiwavelength prior catalogues from CANDELS/3D-HST. By combining IR and UV data, we measure the relationship between total star formation rate (SFR) and stellar mass up to z ∼ 5, indicating that UV-derived dust corrections underestimate the SFR in massive galaxies. We investigate the relationship between obscuration and the UV slope (the IRX–β relation) in our sample, which is similar to that of low-redshift starburst galaxies, although it deviates at high stellar masses. Our data provide new measurements of the total SFR density (SFRD) in M∗>1010M⊙ galaxies at 0.5 < z < 6. This is dominated by obscured star formation by a factor of >10. One third of this is accounted for by 450-μm-detected sources, while one-fifth is attributed to UV-luminous sources (brighter than L∗UV), although even these are largely obscured. By extrapolating our results to include all stellar masses, we estimate a total SFRD that is in good agreement with previous results from IR and UV data at z ≲ 3, and from UV-only data at z ∼ 5. The cosmic star formation history undergoes a transition at z ∼ 3–4, as predominantly unobscured growth in the early Universe is overtaken by obscured star formation, driven by the build-up of the most massive galaxies during the peak of cosmic assembly.

Citation

Bourne, N., Dunlop, J., Merlin, E., Parsa, S., Schreiber, C., Castellano, M., …van der Werf, P. (2017). Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey. Monthly Notices of the Royal Astronomical Society, 467(2), https://doi.org/10.1093/mnras/stx031

Journal Article Type Article
Acceptance Date Jan 5, 2017
Publication Date Jan 9, 2017
Deposit Date Jun 15, 2017
Publicly Available Date Jun 15, 2017
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 467
Issue 2
DOI https://doi.org/10.1093/mnras/stx031
Keywords methods: statistical, galaxies: high-redshift, submillimetre: diffuse background, submillimetre: galaxies
Public URL https://nottingham-repository.worktribe.com/output/841096
Publisher URL https://academic.oup.com/mnras/article/467/2/1360/2877230/Evolution-of-cosmic-star-formation-in-the-SCUBA-2
Additional Information This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf





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