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The GISMO Two-millimeter Deep Field in GOODS-N

Staguhn, Johannes G. and Kovács, Attila and Arendt, Richard G. and Benford, Dominic J. and Decarli, Roberto and Dwek, Eli and Fixsen, Dale J. and Hilton, Gene C. and Irwin, Kent D. and Jhabvala, Christine A. and Karim, Alexander and Leclercq, Samuel and Maher, Stephen F. and Miller, Timothy M. and Moseley, S. Harvey and Sharp, Elmer H. and Walter, Fabian and Wollack, Edward J. (2014) The GISMO Two-millimeter Deep Field in GOODS-N. Astrophysical Journal, 790 (1). Art. No. 77. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20140815-140858231

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Abstract

We present deep continuum observations using the GISMO camera at a wavelength of 2 mm centered on the Hubble Deep Field in the GOODS-N field. These are the first deep field observations ever obtained at this wavelength. The 1σ sensitivity in the innermost ~4' of the 7' diameter map is ~135 μJy beam^(−1), a factor of three higher in flux/beam sensitivity than the deepest available SCUBA 850 μm observations, and almost a factor of four higher in flux/beam sensitivity than the combined MAMBO/AzTEC 1.2 mm observations of this region. Our source extraction algorithm identifies 12 sources directly, and another 3 through correlation with known sources at 1.2 mm and 850 μm. Five of the directly detected GISMO sources have counterparts in the MAMBO/AzTEC catalog, and four of those also have SCUBA counterparts. HDF850.1, one of the first blank-field detected submillimeter galaxies, is now detected at 2 mm. The median redshift of all sources with counterparts of known redshifts is med(z) = 2.91±0.94. Statistically, the detections are most likely real for five of the seven 2 mm sources without shorter wavelength counterparts, while the probability for none of them being real is negligible.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/790/1/77DOIArticle
http://iopscience.iop.org/0004-637X/790/1/77/articlePublisherArticle
http://arxiv.org/abs/1311.1485arXivDiscussion Paper
ORCID:
AuthorORCID
Arendt, Richard G.0000-0001-8403-8548
Dwek, Eli0000-0001-8033-1181
Karim, Alexander0000-0002-8414-9579
Walter, Fabian0000-0003-4793-7880
Additional Information:© 2014 The American Astronomical Society. Received 2013 February 22; accepted 2014 June 7; published 2014 July 7. We would like to thank Carsten Kramer, Santiago Navarro, David John, Albrecht Sievers, and the entire IRAM Granada staff for their support during the instrument installation and observations. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain). This work was supported through NSF ATI grants 1020981 and 1106284. Facility: IRAM:30m (GISMO) - Institute de Radioastronomie Millimetrique 30 meter telescope
Funders:
Funding AgencyGrant Number
Institut national des sciences de l'Univers (INSU)UNSPECIFIED
Max-Planck-GesellschaftUNSPECIFIED
Instituto Geográfico Nacional (IGN)UNSPECIFIED
NSF1020981
NSF1106284
Centre National de la Recherche Scientifique (CNRS)UNSPECIFIED
Subject Keywords:galaxies: evolution; galaxies: high-redshift; galaxies: luminosity function, mass function; galaxies: photometry; galaxies: starburst; infrared: galaxies
Record Number:CaltechAUTHORS:20140815-140858231
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20140815-140858231
Official Citation:The GISMO Two-millimeter Deep Field in GOODS-N Johannes G. Staguhn et al. 2014 ApJ 790 77
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:48626
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:15 Aug 2014 22:32
Last Modified:01 Dec 2017 20:06

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