activity
20042007
most citedThe UKIRT Infrared Deep Sky Survey Early Data Release

221 citations · 331 across the 4 of their papers we have counts for

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6 papers · 1 filter

astro-ph200755 cited

Galaxy Counts at 24 Microns in the SWIRE Fields

David L. Shupe, Michael Rowan-Robinson, Carol J. Lonsdale +21

This paper presents galaxy source counts at 24 microns in the six Spitzer Wide-field InfraRed Extragalactic (SWIRE) fields. The source counts are compared to counts in other fields…

astro-ph20071 cited

The UKIRT Infrared Deep Sky Survey Second Data Release

S. J. Warren, N. J. G. Cross, S. Dye +26

The UKIRT Infrared Deep Sky Survey (UKIDSS) is a set of five large near-infrared surveys, covering a complementary range of areas, depths, and Galactic latitudes. The UKIDSS Second…

astro-ph200654 cited

New members in the Upper Sco association from the UKIDSS Early Data Release

N. Lodieu, N. C. Hambly, R. F. Jameson

We present the results of a 9.3 square degree infrared (ZYJHK) survey in the Upper Scorpius association extracted from the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Cluster…

astro-ph2006221 cited

The UKIRT Infrared Deep Sky Survey Early Data Release

S. Dye, S. J. Warren, N. C. Hambly +11

This paper defines the UKIRT Infrared Deep Sky Survey (UKIDSS) Early Data Release (EDR). UKIDSS is a set of five large near-infra-red surveys defined by Lawrence et al. (2006), bei…

astro-ph2005

The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- I. Survey motivation, design and data processing

A. M. J. Mortier, S. Serjeant, J. S. Dunlop +2

The SCUBA HAlf Degree Extragalactic Survey (SHADES) is a major blank-field extragalactic sub-mm survey underway at the James Clerk Maxwell telescope.SHADES aims to cover half a squ…

astro-ph2004

The European Large Area ISO Survey IX: the 90 micron luminosity function from the Final Analysis sample

S. Serjeant, A. Carraminana, E. Gonzales-Solares +18

We present the 90 micron luminosity function of the Final Analysis of the European Large Area ISO Survey (ELAIS), extending the sample size of our previous analysis (paper IV) by a…