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The Herschel-ATLAS data release 1: I. Maps, catalogues and number counts

Valiante, E.; Smith, M.W.L.; Eales, S.; Maddox, S.J.; Ibar, E.; Hopwood, R.; Dunne, L.; Cigan, P.J.; Dye, S.; Pascale, E.; Rigby, E.E.; Bourne, N.; Furlanetto, C.; Ivison, R.J.

The Herschel-ATLAS data release 1: I. Maps, catalogues and number counts Thumbnail


Authors

E. Valiante

M.W.L. Smith

S. Eales

S.J. Maddox

E. Ibar

R. Hopwood

L. Dunne

P.J. Cigan

SIMON DYE Simon.Dye@nottingham.ac.uk
Associate Professor

E. Pascale

E.E. Rigby

N. Bourne

C. Furlanetto

R.J. Ivison



Abstract

We present the first major data release of the largest single key-project in area carried out in open time with the Herschel Space Observatory. The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) is a survey of 600 deg2 in five photometric bands – 100, 160, 250, 350 and 500 μm – with the Photoconductor Array Camera and Spectrometer and Spectral and Photometric Imaging Receiver (SPIRE) cameras. In this paper and the companion Paper II, we present the survey of three fields on the celestial equator, covering a total area of 161.6 deg2 and previously observed in the Galaxy and Mass Assembly (GAMA) spectroscopic survey. This paper describes the Herschel images and catalogues of the sources detected on the SPIRE 250 μm images. The 1σ noise for source detection, including both confusion and instrumental noise, is 7.4, 9.4 and 10.2 mJy at 250, 350 and 500 μm. Our catalogue includes 120 230 sources in total, with 113 995, 46 209 and 11 011 sources detected at >4σ at 250, 350 and 500 μm. The catalogue contains detections at >3σ at 100 and 160 μm for 4650 and 5685 sources, and the typical noise at these wavelengths is 44 and 49 mJy. We include estimates of the completeness of the survey and of the effects of flux bias and also describe a novel method for determining the true source counts. The H-ATLAS source counts are very similar to the source counts from the deeper HerMES survey at 250 and 350 μm, with a small difference at 500 μm. Appendix A provides a quick start in using the released data sets, including instructions and cautions on how to use them.

Journal Article Type Article
Acceptance Date Jul 21, 2016
Online Publication Date Jul 28, 2016
Publication Date Jul 28, 2016
Deposit Date Apr 27, 2017
Publicly Available Date Apr 27, 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 462
Issue 3
Pages 3146-3179
DOI https://doi.org/10.1093/mnras/stw1806
Keywords Data analysis, Catalogues, Surveys, Galaxies, Cosmology: observations, Submillimetre galaxies
Public URL https://nottingham-repository.worktribe.com/output/799113
Publisher URL https://doi.org/10.1093/mnras/stw1806
Additional Information This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2016 The authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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