activity
19962005
most citedStar Formation History since z = 1.5 as Inferred from Rest-Frame Ultaviolet Luminosity Density Evolution

102 citations · 441 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph2005★ 56 cited

X-ray Cluster Associated with the z=1.063 CSS Quasar 3C 186: The Jet is NOT Frustrated

Aneta Siemiginowska, C. C. Cheung, Stephanie LaMassa +6

We report the Chandra discovery of an X-ray cluster at redshift z = 1.063 associated with the Compact Steep Spectrum radio loud quasar 3C 186 (Q0740+380). Diffuse X-ray emission is…

astro-ph2003★ 57 cited

The XMM--NEWTON Omega Project: I. The X-ray Luminosity - Temperature Relation at z>0.4

D. H. Lumb, J. G. Bartlett, A. K. Romer +9

(abridged) We describe XMM-Newton Guaranteed Time observations of a sample of eight high redshift (0.45<z<0.62) clusters. The goal of these observations was to measure the luminosi…

astro-ph2003★ 10 cited

A serendipitous survey for galaxy clusters by the XMM-Newton Survey Science Center

A. D. Schwope, G. Lamer, D. Burke +5

We describe the initial results of a programme to detect and identify extended X-ray sources found serendipitously in XMM-Newton observations. We have analysed 186 EPIC-PN images a…

astro-ph2002★ 102 cited

Star Formation History since z = 1.5 as Inferred from Rest-Frame Ultaviolet Luminosity Density Evolution

Gillian Wilson, Lennox L. Cowie, Amy J. Barger +1

We investigate the evolution of the universal rest-frame ultraviolet luminosity density from z = 1.5 to the present. We analyze an extensive sample of multicolor data (U', B, V = 2…

astro-ph2001★ 55 cited

Galaxy colours in high redshift X-ray selected clusters - I: Blue galaxy fractions in eight clusters

B. W. Fairley, L. R. Jones, D. A. Wake +4

We present initial results from a wide-field, multi-colour imaging project, designed to study galaxy evolution in X-ray selected clusters at intermediate (z~0.25) and high redshift…

astro-ph1999★ 38 cited

The Bright SHARC Survey: The X-ray Cluster Luminosity Function

R. C. Nichol, A. K. Romer, B. P. Holden +6

We present here initial results on the X-ray Cluster Luminosity Function (XCLF) from the Bright SHARC sample of distant X-ray clusters of galaxies. This sample is 97% complete in i…