Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Determining Star Formation Rates for Infrared Galaxies

  • Authors: G. H. Rieke, A. Alonso-Herrero, B. J. Weiner, P. G. Pérez-González, M. Blaylock, J. L. Donley, and D. Marcillac

RIEKE et al. 2009 The Astrophysical Journal 692 556.

  • Provider: AAS Journals

Caption: Figure 5.

Family of average spectral templates in the 5 to 37 μm range. These templates are used for K-correction to 24 μm rest band. The templates are keyed to the log( L(TIR)) of the galaxies, calculated as by Sanders et al. (2003). They are normalized at 14 μm. The templates for the three highest luminosities are extrapolated and therefore are only indicative.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions