Coppin, K. E. K. and Geach, J. E. and Almaini, O. and Arumugam, V. and Dunlop, J. S. and Hartley, W. G. and Ivison, R. J. and Simpson, C. J. and Smith, D. J. B. and Swinbank, A. M. and Blain, A. W. and Bourne, N. and Bremer, M. and Conselice, C. and Harrison, C. M. and Mortlock, A. and Chapman, S. C. and Davies, L. J. M. and Farrah, D. and Gibb, A. and Jenness, T. and Karim, A. and Knudsen, K. K. and Ibar, E. and Michałowski, M. J. and Peacock, J. A. and Rigopoulou, D. and Robson, E. I. and Scott, D. and Stevens, J. and van der Werf, P. P. (2015) 'The SCUBA-2 Cosmology Legacy Survey : the submillimetre properties of Lyman-break galaxies at z = 3-5.', Monthly notices of the Royal Astronomical Society., 446 (2). pp. 1293-1304.
We present detections at 850 μm of the Lyman-break galaxy (LBG) population at z ≈ 3, 4, and 5 using data from the Submillimetre Common User Bolometer Array 2 Cosmology Legacy Survey in the United Kingdom Infrared Deep Sky Survey ‘Ultra Deep Survey’ field. We employ stacking to probe beneath the survey limit, measuring the average 850 μm flux density of LBGs at z ≈ 3, 4, and 5 with typical ultraviolet luminosities of L1700 ≈ 1029 erg s−1 Hz−1. We measure 850 μm flux densities of (0.25 ± 0.03), (0.41 ± 0.06), and (0.88 ± 0.23) mJy, respectively, finding that they contribute at most 20 per cent to the cosmic far-infrared (IR) background at 850 μm. Fitting an appropriate range of spectral energy distributions to the z ∼ 3, 4, and 5 LBG stacked 24–850 μm fluxes, we derive IR luminosities of L8-1000 μm ≈ 3.2, 5.5, and 11.0 × 1011 L⊙ [and star formation rates (SFRs) of ≈50–200 M⊙ yr−1], respectively. We find that the evolution in the IR luminosity density of LBGs is broadly consistent with model predictions for the expected contribution of luminous-to-ultraluminous IR galaxies at these epochs. We observe a positive correlation between stellar mass and IR luminosity and confirm that, for a fixed mass, the reddest LBGs (UV slope β → 0) are redder due to dust extinction, with SFR(IR)/SFR(UV) increasing by about an order of magnitude over −2 < β < 0 with SFR(IR)/SFR(UV) ∼ 20 for the reddest LBGs. Furthermore, the most massive LBGs tend to have higher obscured-to-unobscured ratios, hinting at a variation in the obscuration properties across the mass range.
|Keywords:||Galaxies: evolution – galaxies: formation, Galaxies: high-redshift, Galaxies: star formation, Submillimetre: galaxies, Ultraviolet: galaxies.|
|Full text:||(VoR) Version of Record|
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|Publisher Web site:||http://dx.doi.org/10.1093/mnras/stu2185|
|Publisher statement:||This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.|
|Date accepted:||17 October 2014|
|Date deposited:||22 October 2015|
|Date of first online publication:||January 2015|
|Date first made open access:||No date available|
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