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A direct calibration of thtae IRX–β relation in Lyman-break galaxies at z=3–5

Koprowski, M.P.; Coppin, K.E.K.; Geach, J.E.; McLure, R.J.; Almaini, Omar; Blain, A.W.; Bremer, M.; Bourne, N.; Chapman, S.C.; Conselice, Christopher; Dunlop, J.S.; Farrah, D.; Hartley, W.; Karim, A.; Knudsen, K.K.; Michałowski, M.J.; Scott, D.; Simpson, C.; Smith, D.J.B.; van der Werf, P.P.

Authors

M.P. Koprowski

K.E.K. Coppin

J.E. Geach

R.J. McLure

Omar Almaini

A.W. Blain

M. Bremer

N. Bourne

S.C. Chapman

Christopher Conselice

J.S. Dunlop

D. Farrah

W. Hartley

A. Karim

K.K. Knudsen

M.J. Michałowski

D. Scott

C. Simpson

D.J.B. Smith

P.P. van der Werf



Abstract

We use a sample of 4209 Lyman-break galaxies (LBGs) at z~ -3, 4, and 5 in the UKIRT Infrared Deep Sky Survey Ultra Deep Survey field to investigate the relationship between the observed slope of the stellar continuum emission in the ultraviolet, β , and the thermal dust emission, as quantified via the so-called ‘infrared excess’ (IRX≡LIR/LUV). Through a stacking analysis, we directly measure the 850-μm flux density of LBGs in our deep (0.9 mJy) James Clerk Maxwell Telescope SCUBA-2850-μm map as well as deep public Herschel/SPIRE 250-, 350-, and 500-μm imaging. We establish functional forms for the IRX–β relation to z∼5, confirming that there is no significant redshift evolution of the relation, and that the resulting average IRX–β curve is consistent with a Calzetti-like attenuation law. Comparing our results with recent works in the literature, we confirm that discrepancies in the slope of the IRX–β relation are driven by biases in the methodology used to determine the ultraviolet slopes. Consistent results are found when IRX–β is evaluated by stacking in bins of stellar mass, and we argue that the near-linear IRX–M* relationship is a better proxy for correcting observed ultraviolet luminosities to total star formation rates, provided an accurate handle on M* and also gives clues as to the physical driver of the role of dust-obscured star formation in high-redshift galaxies.

Journal Article Type Article
Publication Date Oct 1, 2018
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 479
Issue 4
APA6 Citation Koprowski, M., Coppin, K., Geach, J., McLure, R., Almaini, O., Blain, A., …van der Werf, P. (2018). A direct calibration of thtae IRX–β relation in Lyman-break galaxies at z=3–5. Monthly Notices of the Royal Astronomical Society, 479(4), https://doi.org/10.1093/mnras/sty1527
DOI https://doi.org/10.1093/mnras/sty1527
Keywords dust, extinction ; galaxies: high-redshift ; galaxies: ISM ; galaxies: star formation ; cosmology: observations.
Publisher URL http://dx.doi.org/10.1093/mnras/sty1527
Copyright Statement Copyright information regarding this work can be found at the following address: http://eprints.nottingh.../end_user_agreement.pdf

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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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