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I THE IMPACT OF EVOLVING INFRARED SPECTRAL ENERGY DISTRIBUTIONS OF GALAXIES ON STAR FORMATION RATE ESTIMATESNORDON, R; LUTZ, D; CEPA, J et al.The Astrophysical journal. 2012, Vol 745, Num 2, issn 0004-637X, 182.1-182.24, 1Article

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Aéraulique des chantiers d'amiante : étude et analyse des écoulements de ventilation, par simulation numérique avec EOL3D, du sas d'accès du personnel = Asbestos site ventilation: Study and analysis of the ventilation airflows of personnel locks by numerical simulation with EOL3DRAPP, R; DANET, J. P; DUBERNET, F et al.Les Cahiers de notes documentaires - Institut national de sécurité. 2003, Vol 190, pp 13-22, issn 0007-9952, 10 p.Article

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NO EVOLUTION IN THE IR-RADIO RELATION FOR IR-LUMINOUS GALAXIES AT z < 2 IN THE COSMOS FIELDSARGENT, M. T; SCHINNERER, E; SALVATO, M et al.The Astrophysical journal. 2010, Vol 714, Num 2, issn 0004-637X, L190-L195, 2Article

DECOMPOSING STAR FORMATION AND ACTIVE GALACTIC NUCLEUS WITH SPITZER MID-INFRARED SPECTRA: LUMINOSITY FUNCTIONS AND CO-EVOLUTIONHAI FU; LIN YAN; SANDERS, D. B et al.The Astrophysical journal. 2010, Vol 722, Num 1, pp 653-667, issn 0004-637X, 15 p., 1Article

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