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19972008
most citedThe SCUBA HAlf Degree Extragalactic Survey (SHADES) - IV: Radio-mm-FIR photometric redshifts

109 citations · 128 across the 5 of their papers we have counts for

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17 papers · 1 filter

astro-ph2008

Galaxy formation & evolution: the far-ir/sub-mm view

M. Cirasuolo, J. S. Dunlop

We review our current knowledge of the population of high-redshift sub-mm/mm galaxies, with particular emphasis on recent results from the SCUBA HAlf Degree Extragalactic Survey (S…

astro-ph2007109 cited

The SCUBA HAlf Degree Extragalactic Survey (SHADES) - IV: Radio-mm-FIR photometric redshifts

Itziar Aretxaga, David H. Hughes, Kristen Coppin +28

We present the redshift distribution of the SHADES galaxy population based on the rest-frame radio-mm-FIR colours of 120 robustly detected 850um sources in the Lockman Hole East (L…

astro-ph200615 cited

A broadband spectroscopic search for CO line emission in HDF850.1: the brightest submillimetre object in the Hubble Deep Field North

J. Wagg, D. H. Hughes, I. Aretxaga +4

Using the 100-m Green Bank Telescope, we have conducted a cm-wavelength search for CO J=1-0 line emission towards the high-redshift, far-infrared luminous object, HDF850.1 over the…

astro-ph20034 cited

The formation of cluster elliptical galaxies as revealed by extensive star formation

J. A. Stevens, R. J. Ivison, J. S. Dunlop +6

The most massive galaxies in the present-day Universe are found to lie in the centres of rich clusters. They have old, coeval stellar populations suggesting that the bulk of their…

astro-ph2003

Quasar Hosts and the Black Hole-Spheroid Connection

James S. Dunlop

I review our current understanding of the structures and ages of the host galaxies of quasars, and the masses of their central black holes. At low redshift, due largely to the impa…

astro-ph2002

The near-infrared Hubble diagram for sub-mm galaxies

James S. Dunlop

Determing the nature of the bright sub-mm sources and their role in the process of galaxy formation is likely to be a major focus of extra-galactic research over the next few years…