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20042009
most citedSpectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey

877 citations · 1.2k across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2009★ 20 cited

Resolved Dust Emission in a Quasar at z=3.65

D. L. Clements, Glen Petitpas, D. Farrah +11

We present submillimetre observations of the z=3.653 quasar SDSS160705+533558 together with data in the optical and infrared. The object is unusually bright in the far-IR and submm…

astro-ph2008★ 65 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-ph2007★ 55 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-ph2007★ 138 cited

Obscuration in extremely luminous quasars

M. Polletta, D. Weedman, S. Hoenig +3

The spectral energy distributions and infrared (IR) spectra of a sample of obscured AGNs selected in the mid-IR are modeled with recent clumpy torus models to investigate the natur…

astro-ph2007

Ultraluminous Infrared Galaxies at 1.5<z<3 occupy dark matter haloes of mass ~6x10^13 solar masses

D. Farrah, C. J. Lonsdale, C. Borys +9

We present measurements of the spatial clustering of ultraluminous infrared galaxies in two redshift intervals, 1.5<z<2.0 and 2<z<3. Both samples cluster strongly, with r_0=14.40+/…

astro-ph2007★ 877 cited

Spectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey

M. Polletta, M. Tajer, L. Maraschi +18

We present the spectral energy distributions (SEDs) of a hard X-ray selected sample. The sample contains 136 sources with F(2-10 keV)>10^-14 erg/cm^2/s and 132 are AGNs. The source…