An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: source catalogue and properties
Date
Authors
Stach, Stuart M.
Dudzeviciute, U
Smail, Ian
Swinbank, A M
Geach, J. E.
Simpson, J M
An, Fangxia
Almaini, O
Arumugam, Vinodiran
Blain, A. W.
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Oxford University Press
Abstract
We present the catalogue and basic properties of sources in AS2UDS, an 870-μm continuum
survey with the Atacama Large Millimetre/sub-millimetre Array (ALMA) of 716 single-dish
sub-millimetre sources detected in the UKIDSS/UDS field by the SCUBA-2 Cosmology
Legacy Survey. In our sensitive ALMA follow-up observations, we detect 708 sub-millimetre
galaxies (SMGs) at >4.3σ significance across the ∼1◦-diameter field. We combine our precise
ALMA positions with the extensive multiwavelength coverage in the UDS field which yields
spectral energy distributions for our SMGs and a median redshift of zphot = 2.61 ± 0.09.
This large sample reveals a statistically significant trend of increasing sub-millimetre flux with
redshift suggestive of galaxy downsizing. 101 ALMA maps do not show a > 4.3σ SMG, but
we demonstrate from stacking Herschel SPIRE observations at these positions, that the vast
majority of these blank maps correspond to real single-dish sub-millimetre sources. We further
show that these blank maps contain an excess of galaxies at zphot = 1.5–4 compared to random
fields, similar to the redshift range of the ALMA-detected SMGs. In addition, we combine
X-ray and mid-infrared active galaxy nuclei activity (AGN) indicators to yield a likely range
for the AGN fraction of 8–28 per cent in our sample. Finally, we compare the redshifts of
this population of high-redshift, strongly star-forming galaxies with the inferred formation
redshifts of massive, passive galaxies being found out to z ∼ 2, finding reasonable agreement
– in support of an evolutionary connection between these two classes of massive galaxy
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Monthly Notices of the Royal Astronomical Society
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