GOODS–Herschel: an infrared main sequence for star-forming galaxies

D. Elbaz; M. Dickinson; H. S. Hwang; T. Díaz-Santos; G. Magdis; B. Magnelli; D. Le Borgne; F. Galliano; M. Pannella; P. Chanial; L. Armus; V. Charmandaris; E. Daddi; H. Aussel; P. Popesso; J. Kartaltepe; B. Altieri; I. Valtchanov; D. Coia; H. Dannerbauer; K. Dasyra; R. Leiton; J. Mazzarella; D. M. Alexander; V. Buat; D. Burgarella; R.-R. Chary; R. Gilli; R. J. Ivison; S. Juneau; E. Le Floc’h; D. Lutz; G. E. Morrison; J. R. Mullaney; E. Murphy; A. Pope; D. Scott; M. Brodwin; D. Calzetti; C. Cesarsky; S. Charlot; H. Dole; P. Eisenhardt; H. C. Ferguson; N. Förster Schreiber; D. Frayer; M. Giavalisco; M. Huynh; A. M. Koekemoer; C. Papovich; N. Reddy; C. Surace; H. Teplitz; M. S. Yun; G. Wilson

doi:10.1051/0004-6361/201117239

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Volume 533 (September 2011)

A&A, 533 (2011) A119

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Fig. 8

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[IRAS] versus L₈ for local galaxies including only the ISO sample of galaxies used to build the CE01 library of template SEDs and converted from 6.75 μm to 8 μm using the SED of M82. The light blue line shows the position of the CE01 SED templates, built to follow two power laws in the – L₈ relation.

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