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 9.

Tracks of the average template SEDs vs. redshift, as would be observed at 24 μm. The even spacing at any given redshift implies that a power-law fit is a good approximation to the dependence of SFR on 24 μm flux.

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