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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 1.

Full LIRG SEDs and defining photometric points. Between 5 and 36 μm the SEDs are based on IRS spectra rather than the photometry. The curves have been offset for clarity; from top to bottom the galaxies and offset factors are: (1) NGC 1614 (2); (2) NGC 4194 (0.2); (3) NGC 3256 (0.003); (4) NGC 2369 (0.001); (5) ESO 0320-g030 (0.0001); and (6) Zw 049.057 (0.00005).

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