Andrew W. Blain
Published 1998-06-29, updated 1998-08-11Version 2
The population of distant dusty submm-luminous galaxies was first detected last year (Smail, Ivison and Blain 1997). Forms of evolution required to account for both this population and the intensity of background radiation have now been determined (Blain, Smail, Ivison and Kneib 1998), and are used to investigate the most efficient observing strategies for future surveys.
Comments: 4 pages, 3 figures. Revised version includes updated references and details of the SCUBA upgrades programme
Journal: Colombi S., Mellier Y. eds., `Wide Field surveys in cosmology', Editions Frontieres, p. 213-216
Multiple scattering of polarized radiation by non-spherical grains: first results
Source Counts and Background Radiation
Far-Ultraviolet Spectra of AGN: First Results from FUSE
