Figure 16 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 16.

Comparison of L(60) and L(TIR). The line is a linear fit given in the text. There are no outliers (not surprisingly because 60 μm is close to the maximum of the SED) but the slope differs somewhat from unity ( L(TIR) = 740 L(60) ^0.943). Symbols are as for Figure 13.

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