Mid- to far-infrared properties of star-forming galaxies and active galactic nuclei

G. E. Magdis; D. Rigopoulou; G. Helou; D. Farrah; P. Hurley; A. Alonso-Herrero; J. Bock; D. Burgarella; S. Chapman; V. Charmandaris; A. Cooray; Y. Sophia Dai; D. Dale; D. Elbaz; A. Feltre; E. Hatziminaoglou; J.-S. Huang; G. Morrison; S. Oliver; M. Page; D. Scott; Y. Shi

doi:10.1051/0004-6361/201322226

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Volume 558 (October 2013)

A&A, 558 (2013) A136

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Fig. 11

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Correlation between L_IR and rest-frame luminosities at observed 10, 18, 21-, and 25.5 μm. The choice of the rest-frame luminosity wavelengths corresponds to the central wavelengths of the JWST-MIRI filters. Each IRS spectrum was shifted to the rest-frame and convolved with MIRI filters. The best-fit regression line and the associated plot are shown in each panel and are summarised in Table 3.

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