4.7 Article

CHARACTERIZING DUST ATTENUATION IN LOCAL STAR-FORMING GALAXIES: UV AND OPTICAL REDDENING

期刊

ASTROPHYSICAL JOURNAL
卷 818, 期 1, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.3847/0004-637X/818/1/13

关键词

dust, extinction; galaxies: evolution; galaxies: general; galaxies: ISM

资金

  1. NASA, via the Jet Propulsion Laboratory Euclid Project Office, as part of the Science Investigations as Members of the Euclid Consortium
  2. Euclid Science Team program
  3. NASA [NAS5-98034]
  4. Alfred P. Sloan Foundation
  5. National Science Foundation
  6. US Department of Energy
  7. National Aeronautics and Space Administration
  8. Japanese Monbukagakusho
  9. Max Planck Society
  10. Higher Education Funding Council for England

向作者/读者索取更多资源

The dust attenuation for a sample of 10,000 local (z less than or similar to 0.1) star-forming galaxies is constrained as a function of their physical properties. We utilize aperture-matched multiwavelength data available from the Galaxy Evolution Explorer and the Sloan Digital Sky Survey to ensure that regions of comparable size in each galaxy are being analyzed.

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