Summary and discussion of some projects to use SCUBA to target sources selected at other wavebands, as well as to find new sub-mm galaxies in ‘blank fields’. 1

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ULIRG at intermediate (z=0.4) and high redshift (z=1 − 2) can be observed by the Hubble Space Telescope (HST) in order to present a plausible explanation for the origin of some host galaxies of the faint SCUBA sources recently observed by Smail et al. (1998). The results of our numerical simulations

Studies of galaxy properties in the infrared (IR) have added much to our understanding of how and when galaxies form

of the extragalactic background radiation field are described briefly, especially in the context of the SCUBA lens survey. 1 The potential problems caused by source confusion in the large 15-arcsec SCUBA observing beam for the identification and follow up of the results are discussed. The effects of confusion

The luminous high-redshift dust sources discovered by the

A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are:

of the ratio Mhalo/Msph between the mass of the dark halos hosting such galaxies and the mass in stars produced at the end of the major star-formation burst. SCUBA sources are predicted to be strongly clustered, with a clustering strength increasing with mass. Comparisons with the best available measurements

of the ratio Mhalo/Msph between the mass of the dark halos hosting such galaxies and the mass in stars produced at the end of the major star-formation burst. SCUBA sources are predicted to be strongly clustered, with a clustering strength increasing with mass. Comparisons with the best available measurements

to the anisotropy of the microwave sky. We review results from several submillimetre surveys started during SCUBA’s first year of operation, and discuss their future development, together with other projects that will greatly improve our understanding of the extragalactic point source contribution