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McMahon R. G.
McMahon Richard G.
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McMahon, Richard G.
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of
Near-infrared colors of minor planets recovered from VISTA-VHS survey (MOVIS)
Observations of the Hubble Deep Field with the Infrared Space Observatory - I. Data reduction, maps and sky coverage
Observations of the Hubble Deep Field with the Infrared Space Observatory - V. Spectral energy distributions, starburst models and star formation history
A homogeneous sample of sub-damped Lyman α systems — I. Construction of the sample and chemical abundance measurements
Submillimetre observations of z > 6 quasars
The luminosity function evolution of soft X-ray-selected active galactic nuclei in the RIXOS survey
Optical and X-ray properties of the RIXOS active galactic nuclei — I.
The extreme X-ray luminosity of the z = 4.72 radio-loud quasar GB 1428+4217
The Las Campanas Infrared Survey - II. Photometric redshifts, comparison with models and clustering evolution
Quasars as probes of the submillimetre cosmos at z> 5 — I. Preliminary SCUBA photometry
Submillimetre observations of luminous z> 4 radio-quiet quasars and the contribution of AGN to the submm source population
Lyman break galaxies and the star formation rate of the Universe at z≈ 6
A homogeneous sample of sub-damped Lyman α systems - IV. Global metallicity evolution
A new large sample of ultraluminous IRAS galaxies
The star formation rate of the Universe at z≈ 6 from the Hubble Ultra-Deep Field
Eight new T4.5-T7.5 dwarfs discovered in the UKIDSS Large Area Survey Data Release 1
Observations of the Hubble Deep Field with the Infrared Space Observatory - II. Source detection and photometry
The UKIRT Infrared Deep Sky Survey (UKIDSS)
PMN J0525-3343: soft X-ray spectral flattening in a blazar at z = 4.4
The SCUBA Bright Quasar Survey (SBQS) — II. Unveiling the quasar epoch at submillimetre wavelengths
A homogeneous sample of sub-damped Lyman α systems — II. Statistical, kinematic and chemical properties
Large-scale structure in a new deep IRAS galaxy redshift survey
The PSCz catalogue
Optical imaging of ultraluminous IRAS galaxies: how many are mergers?
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