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Infrared to millimetre spectral energy distributions have been obtained for41 bright ultra-luminous infrared galaxies. The observations were carried outwith ISOPHOT between 10 and 200 micron and supplemented for 16 sources withSCUBA at 450 and 850 micron and with SEST at 1.3 mm. In addition, seven sourceswere observed at 1.2 and 2.2 $\mu$m with the 2.2 m telescope on Calar Alto.These new SEDs represent the most complete set of infrared photometrictemplates obtained so far on ULIRGs in the local universe.Comment: 23 pages, 11 figures, accepted for publication in Astronomy &  Astrophysic

Infrared to millimetre photometry of ultra-luminous IR galaxies : New evidence favouring a 3-stage dust model