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The z ~ 1.2 Galaxy Luminosity Function from The LCIR Survey
H. -W. Chen, P. J. McCarthy, R. O. Marzke +10
We present results from the Las Campanas Infrared Survey, designed to identify a statistically significant sample of z>=1 galaxies using photometric redshift techniques. Here we su…
Automated optical identification of a large complete northern hemisphere sample of flat spectrum radio sources with S_6cm > 200 mJy
Ignas Snellen, Richard McMahon, Isobel Hook +1
This paper describes the automated optical APM identification of radio sources from the Jodrell Bank - VLA Astrometric Survey (JVAS), as used for the search for distant radio-loud…
HST imaging of hyperluminous infrared galaxies
D. Farrah, A. Verma, S. Oliver +2
We present HST WFPC2 I band imaging for a sample of 9 Hyperluminous Infrared Galaxies spanning a redshift range 0.45 < z < 1.34. Three of the sample have morphologies showing evide…
The SCUBA Bright Quasar Survey (SBQS): 850micron observations of the z>4 sample
Kate G. Isaak, Robert S. Priddey, Richard G. McMahon +4
We present initial results of a new, systematic search for massive star-formation in the host galaxies of the most luminous and probably most massive z>=4 radio-quiet quasars (M(B)…
The Las Campanas IR Survey. II. Photometric redshifts, comparison with models and clustering evolution
A. E. Firth, R. S. Somerville, R. G. McMahon +15
The LCIR Survey, using the Cambridge IR Survey Instrument (CIRSI), reaches H \~ 20-21 over ~1 deg^2. We present results for 744 arcmin^2 in which public UBVRI data exist. We compar…
Statistical Properties of DLAs and sub-DLAs
Celine Peroux, Mike J. Irwin, Richard G. McMahon +1
Quasar absorbers provide a powerful observational tool with which to probe both galaxies and the intergalactic medium up to high redshift. We present a study of the evolution of th…