Galaxy counts at 24 μm in the SWIRE fields
- Creators
- Shupe, David L.
- Rowan-Robinson, Michael
- Lonsdale, Carol J.
- Masci, Frank J.
- Evans, Tracey
- Fang, Fan
- Oliver, Sebastian
- Vaccari, Mattia
- Rodighiero, Giulia
- Padgett, Deborah
- Surace, Jason A.
- Xu, C. Kevin
- Berta, Stefano
- Pozzi, Francesca
- Franceschini, Alberto
- Babbedge, Thomas
- Gonzales-Solares, Eduardo
- Siana, Brian D.
- Farrah, Duncan
- Frayer, David T.
- Smith, H. E.
- Polletta, Maria del Carmen
- Owen, Frazer
- Pérez-Fournon, Ismael
Abstract
This paper presents galaxy source counts at 24 μm in the six Spitzer Wide-field InfraRed Extragalactic (SWIRE) fields. The source counts are compared to counts in other fields, and to model predictions that have been updated since the launch of Spitzer. This analysis confirms a very steep rise in the Euclidean-normalized differential number counts between 2 mJy and 0.3 mJy. Variations in the counts between fields show the effects of sample variance in the flux range of 0.5-10 mJy, up to 100% larger than Poisson errors. Nonetheless, a "shoulder" in the normalized counts persists at around 3 mJy. The peak of the normalized counts at 0.3 mJy is higher and narrower than most models predict. In the ELAIS N1 field, the 24 μm data are combined with Spitzer-IRAC data and five-band optical imaging, and these band-merged data are fit with photometric redshift templates. Above 1 mJy the counts are dominated by galaxies at z < 0.3. By 300 μJy, about 25% are between z ~ 0.3 and 0.8, and a significant fraction are at z ~ 1.3-2. At low redshifts the counts are dominated by spirals, and starbursts rise in number density to outnumber the spirals' contribution to the counts below 1 mJy.
Additional Information
© 2008 The American Astronomical Society. Received 2006 June 27; accepted 2007 November 3; published 2008 February 14. We are grateful to the referees for their comments, which have led to substantial improvement of this paper. 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 a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. SB was supported by a Fondazione Ing. Aldo Gini 2006 grant.Attached Files
Published - SHUaj08.pdf
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Additional details
- Eprint ID
- 14101
- Resolver ID
- CaltechAUTHORS:20090428-130122358
- NASA
- Fondazione Ing. Aldo Gini
- Created
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2009-07-09Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)