The Space Density of Luminous Dusty Star-forming Galaxies at z > 4: SCUBA-2 and LABOCA Imaging of Ultrared Galaxies from Herschel-ATLAS

Author(s)

Rob J. Ivison, A. J. R. Lewis, Alexander Weiss, V. Arumugam, James M. Simpson, Helmut Dannerbauer

Abstract

Until recently, only a handful of dusty, star-forming galaxies (DSFGs) were known at z > 4, most of them significantly amplified by gravitational lensing. Here, we have increased the number of such DSFGs substantially, selecting galaxies from the uniquely wide 250, 350, and 500 μm Herschel-ATLAS imaging survey on the basis of their extremely red far-infrared colors and faint 350 and 500 μm flux densities, based on which, they are expected to be largely unlensed, luminous, rare, and very distant. The addition of ground-based continuum photometry at longer wavelengths from the James Clerk Maxwell Telescope and the Atacama Pathfinder Experiment allows us to identify the dust peak in their spectral energy distributions (SEDs), with which we can better constrain their redshifts. We select the SED templates that are best able to determine photometric redshifts using a sample of 69 high-redshift, lensed DSFGs, then perform checks to assess the impact of the CMB on our technique, and to quantify the systematic uncertainty associated with our photometric redshifts, σ = 0.14 (1 + z), using a sample of 25 galaxies with spectroscopic redshifts, each consistent with our color selection. For Herschel-selected ultrared galaxies with typical colors of S 500/S 250 ∼ 2.2 and S 500/S 350 ∼ 1.3 and flux densities, S 500 ∼ 50 mJy, we determine a median redshift, z_phot = 3.66, an interquartile redshift range, 3.30-4.27, with a median rest-frame 8-1000 μm luminosity, L_IR, of 1.3 · 10¹³ L_⊙. A third of the galaxies lie at z > 4, suggesting a space density, ρ_{z > 4}, of ≈ 6 · 10^-7 Mpc^-3. Our sample contains the most luminous known star-forming galaxies, and the most overdense cluster of starbursting proto-ellipticals found to date.

Organisation(s)

Department of Astrophysics

External organisation(s)

European Southern Observatory (Germany), The Royal Observatory, Edinburgh, Max-Planck-Institut für Radioastronomie, Durham University

Journal

The Astrophysical Journal

Volume

832

Pages

24

No. of pages

24

ISSN

0004-637X

DOI

https://doi.org/10.3847/0004-637X/832/1/78

Publication date

11-2016

Peer reviewed

Yes

Austrian Fields of Science 2012

103003 Astronomy, 103004 Astrophysics

Keywords

ASJC Scopus subject areas

Astronomy and Astrophysics, Space and Planetary Science

Portal url

https://ucrisportal.univie.ac.at/en/publications/d241ad9c-632f-48ea-a0eb-6cd23745a894