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most citedThe SCUBA Half-Degree Extragalactic Survey (SHADES) - VIII. The Nature of Faint Submm Galaxies in SHADES, SWIRE and SXDF Surveys

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astro-ph200865 cited

The SCUBA Half-Degree Extragalactic Survey (SHADES) - VIII. The Nature of Faint Submm Galaxies in SHADES, SWIRE and SXDF Surveys

D. L. Clements, M. Vaccari, T. Babbedge +46

We present the optical-to-submm spectral energy distributions for 33 radio & mid-IR identified submillimetre galaxies discovered via the SHADES 850 micron SCUBA imaging in the Suba…

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-ph2003

The environments of hyperluminous infrared galaxies at 0.44<z<1.55

D. Farrah, J. Geach, M. Fox +5

We present deep wide-field K-band observations of six Hyperluminous Infrared Galaxies (HLIRGs) spanning a redshift range 0.44<z<1.55. The sample resides in a wide variety of enviro…

astro-ph2003

Sub-millimeter emission from type Ia supernova host galaxies at z=0.5

D. Farrah, M. Fox, M. Rowan-Robinson +2

We present deep sub-millimetre observations of seventeen galaxies at z=0.5, selected through being hosts of a type 1a supernova. Two galaxies are detected directly, and the sample…

astro-ph2003

SWIRE: The SIRTF Wide-area InfraRed Extragalactic Survey

Carol J. Lonsdale, Harding E. Smith, Michael Rowan-Robinson +16

The SIRTF Wide-area InfraRed Extragalactic survey (SWIRE), the largest SIRTF Legacy program, is a wide-area, imaging survey to trace the evolution of dusty, star-forming galaxies,…

astro-ph2003

Starburst and AGN activity in ultraluminous infrared galaxies

D. Farrah, J. Afonso, A. Efstathiou +3

(Abridged) We examine the power source of 41 local Ultraluminous Infrared Galaxies using archival infrared and optical photometry. We fit the observed Spectral Energy Distributions…