Figure 10 from Determining Star Formation Rates for Infrared Galaxies

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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 10.

Trends with redshift of the intercept A and slope B for the relation between SFR and infrared flux, log(SFR) = A + B(log(4π D ² _L f _ν) − 53), for several infrared bands: Spitzer/MIPS 24 μm (heavy black line); Herschel/PACS 70 and 100 μm (green and red lines); JWST/MIRI 18, 21, and 25 μm (magenta, blue, and cyan lines).

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