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ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance

Oteo, I.; Zwaan, M.A.; Ivison, R.J.; Smail, I.; Biggs, A.D.

ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance Thumbnail


Authors

I. Oteo

M.A. Zwaan

R.J. Ivison

Profile image of Ian Smail

Ian Smail ian.smail@durham.ac.uk
Emeritus Professor

A.D. Biggs



Abstract

We have exploited ALMA calibration observations to carry out a novel, wide, and deep submillimeter (submm) survey, almacal. These calibration data comprise a large number of observations of calibrator fields in a variety of frequency bands and array configurations. By gathering together data acquired during multiple visits to many ALMA calibrators, it is possible to reach noise levels which allow the detection of faint, dusty, star-forming galaxies (DSFGs) over a significant area. In this paper, we outline our survey strategy and report the first results. We have analyzed data for 69 calibrators, reaching depths of ~25 μJy beam−1 at sub-arcsec resolution. Adopting a conservative approach based on ≥5σ detections, we have found 8 and 11 DSFGs in ALMA bands 6 and 7, respectively, with flux densities S 1.2 mm ≥ 0.2 mJy. The faintest galaxies would have been missed by even the deepest Herschel surveys. Our cumulative number counts have been determined independently at 870 μm and 1.2 mm from a sparse sampling of the astronomical sky, and are thus relatively free of cosmic variance. The counts are lower than reported previously by a factor of at least 2×. Future analyses will yield large, secure samples of DSFGs with redshifts determined via the detection of submm spectral lines. Uniquely, our strategy then allows for morphological studies of very faint DSFGs—representative of more normal star-forming galaxies than conventional submm galaxies—in fields where self-calibration is feasible, yielding milliarcsecond spatial resolution.

Citation

Oteo, I., Zwaan, M., Ivison, R., Smail, I., & Biggs, A. (2016). ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance. Astrophysical Journal, 822(1), Article 36. https://doi.org/10.3847/0004-637x/822/1/36

Journal Article Type Article
Acceptance Date Feb 17, 2016
Online Publication Date May 2, 2016
Publication Date May 2, 2016
Deposit Date Jun 21, 2016
Publicly Available Date Jun 22, 2016
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 822
Issue 1
Article Number 36
DOI https://doi.org/10.3847/0004-637x/822/1/36
Public URL https://durham-repository.worktribe.com/output/1380691
Related Public URLs http://adsabs.harvard.edu/abs/2016ApJ...822...36O

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Copyright Statement
© 2016. The American Astronomical Society. All rights reserved.






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