4.6 Article

AN ATLAS OF GALAXY SPECTRAL ENERGY DISTRIBUTIONS FROM THE ULTRAVIOLET TO THE MID-INFRARED

期刊

出版社

IOP PUBLISHING LTD
DOI: 10.1088/0067-0049/212/2/18

关键词

atlases; galaxies: general; galaxies: photometry; techniques: spectroscopic

资金

  1. Australian Research Council [FT100100280]
  2. Monash Research Accelerator Program (MRA)
  3. International Science Linkages Program
  4. NASA'
  5. Alfred P. Sloan Foundation
  6. National Science Foundation
  7. U.S. Department of Energy Office of Science
  8. SDSS-III Collaboration including the University of Arizona
  9. Brazilian Participation Group
  10. Brookhaven National Laboratory
  11. University of Cambridge
  12. University of Florida
  13. French Participation Group
  14. German Participation Group
  15. Instituto de Astrofisica de Canarias
  16. Michigan State/Notre Dame/JINA Participation Group
  17. Johns Hopkins University
  18. Lawrence Berkeley National Laboratory
  19. Max Planck Institute for Astrophysics
  20. New Mexico State University
  21. New York University
  22. Ohio State University
  23. Pennsylvania State University
  24. University of Portsmouth
  25. Princeton University
  26. Spanish Participation Group
  27. University of Tokyo
  28. University of Utah
  29. Vanderbilt University
  30. University of Virginia
  31. University of Washington
  32. Yale University
  33. NASA Astrophysics Data Analysis Program [08-ADP08-0072]
  34. NSF [AST-1211644]
  35. National Aeronautics and Space Administration
  36. NASA
  37. JPL
  38. [22012006]
  39. Grants-in-Aid for Scientific Research [23540273] Funding Source: KAKEN
  40. Australian Research Council [FT100100280] Funding Source: Australian Research Council

向作者/读者索取更多资源

We present an atlas of 129 spectral energy distributions for nearby galaxies, with wavelength coverage spanning from the ultraviolet to the mid-infrared. Our atlas spans a broad range of galaxy types, including ellipticals, spirals, merging galaxies, blue compact dwarfs, and luminous infrared galaxies. We have combined ground-based optical drift-scan spectrophotometry with infrared spectroscopy from Spitzer and Akari with gaps in spectral coverage being filled using Multi-wavelength Analysis of Galaxy Physical Properties spectral energy distribution models. The spectroscopy and modelswere normalized, constrained, and verified with matched-aperture photometry measured from Swift, Galaxy Evolution Explorer, Sloan Digital Sky Survey, Two Micron All Sky Survey, Spitzer, and Wide-field Infrared Space Explorer images. The availability of 26 photometric bands allowed us to identify and mitigate systematic errors present in the data. Comparison of our spectral energy distributions with other template libraries and the observed colors of galaxies indicates that we have smaller systematic errors than existing atlases, while spanning a broader range of galaxy types. Relative to the prior literature, our atlas will provide improved K-corrections, photometric redshifts, and star-formation rate calibrations.

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