Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies
- Department of Physics and Astronomy, University of Wyoming, Laramie WY (United States)
- Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena CA (United States)
- Institut d’Astrophysique de Paris, Sorbonne Universités, Paris (France)
- Spitzer Science Center, California Institute of Technology, Pasadena, CA (United States)
- Department of Astronomy, University of Maryland, College Park, MD (United States)
- Unidad de Astronomía, Universidad de Antofagasta, Antofagasta (Chile)
- School of Physics and Astronomy, Monash University, Victoria 3800 (Australia)
- Department of Astronomy, University of Massachusetts, Amherst MA (United States)
- Sterrenkundig Observatorium, Universiteit Gent, Gent (Belgium)
- European Southern Observatory, Garching (Germany)
- Space Telescope Science Institute, Baltimore MD (United States)
- Research School of Astronomy and Astrophysics, Australian National University, Canberra (Australia)
- Astronomy Department, University of Capetown, Rondebosch (South Africa)
- Max-Planck-Institut für Extraterrestrische Physik, Garching (Germany)
- Steward Observatory, University of Arizona, Tucson AZ (United States)
- INAF—Osservatorio Astrofisico di Arcetri, Firenze (Italy)
- Institute of Astronomy, University of Cambridge, Cambridge (United Kingdom)
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 BVR {sub C} I {sub C} and KINGFISH far-infrared/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.
- OSTI ID:
- 22663734
- Journal Information:
- Astrophysical Journal, Vol. 837, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
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