Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies
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Author
Dale, D. A.Cook, D. O.
Roussel, H.

Turner, J. A.
Armus, L.
Bolatto, A. D.

Boquien, M.
Brown, M. J. I.
Calzetti, D.

Looze, I. De
Galametz, M.

Gordon, K. D.

Groves, B. A.
Jarrett, T. H.

Helou, G.
Herrera-Camus, R.

Hinz, J. L.

Hunt, L. K.
Kennicutt, R. C.
Murphy, E. J.
Rest, A.
Sandstrom, K. M.

Smith, J.-D. T.

Tabatabaei, F. S.
Wilson, C. D.
Affiliation
Univ Arizona, Steward ObservIssue Date
2017-03-07
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IOP PUBLISHING LTDCitation
Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies 2017, 837 (1):90 The Astrophysical JournalJournal
The Astrophysical JournalRights
© 2017. The American Astronomical Society. All rights reserved.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We present an update to the ultraviolet-to-radio database of global broadband photometry for the 79 nearby galaxies that comprise the union of the KINGFISH (Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel) and SINGS (Spitzer Infrared Nearby Galaxies Survey) samples. The 34-band data set presented here includes contributions from observational work carried out with a variety of facilities including GALEX, SDSS, Pan-STARRS1, NOAO, 2MASS, Wide-Field Infrared Survey Explorer, Spitzer, Herschel, Planck, JCMT, and the VLA. Improvements of note include recalibrations of previously published SINGS BVRCIC and KINGFISH farinfrared/submillimeter photometry. Similar to previous results in the literature, an excess of submillimeter emission above model predictions is seen primarily for low-metallicity dwarf or irregular galaxies. This 33-band photometric data set for the combined KINGFISH+SINGS sample serves as an important multiwavelength reference for the variety of galaxies observed at low redshift. A thorough analysis of the observed spectral energy distributions is carried out in a companion paper.ISSN
1538-4357Version
Final published versionSponsors
Alfred P. Sloan Foundation; Participating Institutions; NSF; U.S. Department of Energy, NASA; Japanese Monbukagakusho; Max Planck Society; Higher Education Funding Council for England; NASAAdditional Links
http://stacks.iop.org/0004-637X/837/i=1/a=90?key=crossref.c8af1d7d861e20ce3e1e7d49c04d3707ae974a485f413a2113503eed53cd6c53
10.3847/1538-4357/aa6032