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The Spitzer South Pole Telescope Deep Field: Survey Design and Infrared Array Camera Catalogs

Ashby, M. L. N. and Stanford, S. A. and Brodwin, M. and Gonzalez, A. H. and Martinez-Manso, J. and Bartlett, J. G. and Benson, B. A. and Bleem, L. E. and Crawford, T. M. and Dey, A. and Dressler, A. and Einsenhardt, P. R. M. and Galametz, A. and Jannuzi, B. T. and Marrone, D. P. and Mei, S. and Muzzin, A. and Pacaud, F. and Pierre, M. and Stern, D. and Vieira, J. D. (2013) The Spitzer South Pole Telescope Deep Field: Survey Design and Infrared Array Camera Catalogs. Astrophysical Journal Supplement Series, 209 (2). Art. No. 22. ISSN 0067-0049. https://resolver.caltech.edu/CaltechAUTHORS:20140107-085945350

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Abstract

The Spitzer South Pole Telescope Deep Field (SSDF) is a wide-area survey using Spitzer's Infrared Array Camera (IRAC) to cover 94 deg^2 of extragalactic sky, making it the largest IRAC survey completed to date outside the Milky Way midplane. The SSDF is centered at (α, δ) = (23:30, –55:00), in a region that combines observations spanning a broad wavelength range from numerous facilities. These include millimeter imaging from the South Pole Telescope, far-infrared observations from Herschel/SPIRE, X-ray observations from the XMM XXL survey, near-infrared observations from the VISTA Hemisphere Survey, and radio-wavelength imaging from the Australia Telescope Compact Array, in a panchromatic project designed to address major outstanding questions surrounding galaxy clusters and the baryon budget. Here we describe the Spitzer/IRAC observations of the SSDF, including the survey design, observations, processing, source extraction, and publicly available data products. In particular, we present two band-merged catalogs, one for each of the two warm IRAC selection bands. They contain roughly 5.5 and 3.7 million distinct sources, the vast majority of which are galaxies, down to the SSDF 5σ sensitivity limits of 19.0 and 18.2 Vega mag (7.0 and 9.4 μJy) at 3.6 and 4.5 μm, respectively.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0067-0049/209/2/22DOIArticle
http://iopscience.iop.org/0067-0049/209/2/22/PublisherArticle
http://arxiv.org/abs/1308.0201arXivDiscussion Paper
http://dx.doi.org/10.1088/0067-0049/212/1/16ErrataErratum
ORCID:
AuthorORCID
Ashby, M. L. N.0000-0002-3993-0745
Brodwin, M.0000-0002-4208-798X
Gonzalez, A. H.0000-0002-0933-8601
Benson, B. A.0000-0002-5108-6823
Dey, A.0000-0002-4928-4003
Galametz, A.0000-0002-1504-8117
Jannuzi, B. T.0000-0002-1578-6582
Marrone, D. P.0000-0002-2367-1080
Mei, S.0000-0002-2849-559X
Muzzin, A.0000-0002-9330-9108
Stern, D.0000-0003-2686-9241
Alternate Title:The Spitzer-South Pole Telescope Deep Field: Survey Design and IRAC Catalogs
Additional Information:© 2013 American Astronomical Society. Received 2013 July 12; accepted 2013 October 8; published 2013 November 13. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under contract with the National Aeronautics and Space Administration (NASA). Support was provided by NASA through contract number 1439357 issued by JPL/Caltech. IRAF is distributed by the National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation. Lawrence Livermore National Laboratory is operated by Lawrence Livermore National Security, LLC, for the U.S. Department of Energy, National Nuclear Security Administration under Contract DE-AC52-07NA27344. F.P. acknowledges support from grant 50 OR 1117 of the Deutches Zenturm für Luft- und Raumfahrt (DLR). We thank Dave Nair for his efforts in characterizing a preliminary reduction of the SSDF images. We also thank Richard G. Arendt, who kindly computed the Milky Way star count models shown in Figure 8. Facility: Spitzer (IRAC)
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
NASA1439357
Department of Energy (DOE)DE-AC52-07NA27344
Deutches Zenturm für Luft- und Raumfahrt (DLR)50 OR 1117
Subject Keywords: catalogs; galaxies: clusters: general; infrared: galaxies; surveys
Issue or Number:2
Record Number:CaltechAUTHORS:20140107-085945350
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140107-085945350
Official Citation:The Spitzer South Pole Telescope Deep Field: Survey Design and Infrared Array Camera Catalogs M. L. N. Ashby et al. 2013 ApJS 209 22
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:43242
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:07 Jan 2014 17:31
Last Modified:02 Nov 2019 19:09

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