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Published online by Cambridge University Press: 03 August 2017
We have surveyed a sample of 40 ultraluminous (L60μm > 1012L using H0 = 50 km s−1 Mpc−1 and Ω0 = 1) and 7 high-luminosity (11.7 < log(L60μm) < 12.0) IRAS galaxies with the aim of obtaining a better estimate of the fraction of ultraluminous IRAS galaxies in interacting systems. This is the largest imaging survey of such high-luminosity galaxies. The galaxies were selected from the North Galactic Wedge (Lawrence et al. 1986) and QDOT (Rowan-Robinson et al. 1990 MN in press) area and flux limited IRAS galaxy samples with complete z information. Imaging observations were carried out at the Observatorio del Roque de los Muchachos (La Palma) using the CCD imaging system at the f/3 focus of the 2.5m Isaac Newton Telescope. The average total exposure time per galaxy was 2000s, reaching a limiting isophote of R=26.