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Title: Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies

Journal Article · · Astrophysical Journal
;  [1];  [2];  [3]; ;  [4];  [5];  [6];  [7];  [8];  [9];  [10];  [11];  [12];  [13];  [14];  [15];  [16];  [17];
  1. Department of Physics and Astronomy, University of Wyoming, Laramie WY (United States)
  2. Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena CA (United States)
  3. Institut d’Astrophysique de Paris, Sorbonne Universités, Paris (France)
  4. Spitzer Science Center, California Institute of Technology, Pasadena, CA (United States)
  5. Department of Astronomy, University of Maryland, College Park, MD (United States)
  6. Unidad de Astronomía, Universidad de Antofagasta, Antofagasta (Chile)
  7. School of Physics and Astronomy, Monash University, Victoria 3800 (Australia)
  8. Department of Astronomy, University of Massachusetts, Amherst MA (United States)
  9. Sterrenkundig Observatorium, Universiteit Gent, Gent (Belgium)
  10. European Southern Observatory, Garching (Germany)
  11. Space Telescope Science Institute, Baltimore MD (United States)
  12. Research School of Astronomy and Astrophysics, Australian National University, Canberra (Australia)
  13. Astronomy Department, University of Capetown, Rondebosch (South Africa)
  14. Max-Planck-Institut für Extraterrestrische Physik, Garching (Germany)
  15. Steward Observatory, University of Arizona, Tucson AZ (United States)
  16. INAF—Osservatorio Astrofisico di Arcetri, Firenze (Italy)
  17. 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