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19932009
most citedThe SCUBA HAlf Degree Extragalactic Survey (SHADES) - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies

317 citations · 1.9k across the 33 of their papers we have counts for

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Showing 2006Show all

10 papers · 1 filter

astro-ph2006

A 15um selected sample of high-z starbursts and AGNs

A. Hernan-Caballero, I. Perez-Fournon, M. Rowan-Robinson +19

We report results from a Spitzer GO-1 program of IRS spectroscopy of a large sample of Luminous Infrared Galaxies and quasars selected from the European Large Area ISO Survey (ELAI…

astro-ph2006

Extragalactic Science with Herschel-SPIRE

M. J. Griffin, J. J. Bock, A. Franceschini +9

SPIRE, the Spectral and Photometric Imaging Receiver, is one of three instruments to fly on ESA's Herschel Space Observatory. It contains a three-band imaging photometer operating…

astro-ph2006

Deep GMOS Spectroscopy of Faint SWIRE Populations

M. Trichas, M. Rowan-Robinson, I. Waddington +1

We have carried out a deep (21.5<R<23.9) systematic survey of galaxies selected from SWIRE using GMOS to target X-ray sources, AGN and galaxies with photometric redshifts greater t…

astro-ph200626 cited

Optical and Infrared Diagnostics of SDSS galaxies in the SWIRE Survey

Payam Davoodi, Francesca Pozzi, Seb Oliver +14

We present the rest-frame optical and infrared colours of a complete sample of 1114 z<0.3 galaxies from the Spitzer Wide-area InfraRed Extragalactic Legacy Survey (SWIRE) and the S…

astro-ph2006145 cited

Luminosity functions for galaxies and quasars in the Spitzer Wide-Area Infrared Extra-galactic (SWIRE) Legacy survey

T. S. R. Babbedge, M. Rowan-Robinson, M. Vaccari +18

We construct rest-frame luminosity functions at 3.6, 4.5, 5.8, 8 and 24 microns over the redshift range 0<z<2 for galaxies and 0<z<4 for optical QSOs, using optical and infrared da…

astro-ph200612 cited

Parametric modelling of the 3.6um to 8um colour distributions of galaxies in the SWIRE Survey

Payam Davoodi, Seb Oliver, Maria del Carmen Polletta +15

We fit a parametric model comprising a mixture of multi-dimensional Gaussian functions to the 3.6 to 8um colour and optical photo-z distribution of galaxy populations in the ELAIS-…