activity
19932013
most citedXMM-Newton discovery of an X-ray filament in Coma

106 citations · 268 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2013★ 6 cited

A Large Scale Structure at Redshift 1.71 in the Lockman Hole

J. P. Henry, K. Aoki, A. Finoguenov +5

We previously identified LH146, a diffuse X-ray source in the Lockman Hole, as a galaxy cluster at redshift 1.753. The redshift was based on one spectroscopic value, buttressed by…

astro-ph.CO2011★ 51 cited

Photometry and Photometric Redshift catalogs for the Lockman Hole Deep Field

S. Fotopoulou, M. Salvato, G. Hasinger +8

We present broad band photometry and photometric redshifts for 187611 sources located in ~0.5deg^2 in the Lockman Hole area. The catalog includes 389 X-ray detected sources identif…

astro-ph.CO2010★ 38 cited

An X-ray Selected Galaxy Cluster in the Lockman Hole at Redshift 1.753

J. Patrick Henry, Mara Salvato, Alexis Finoguenov +12

We have discovered an X-ray selected galaxy cluster with a spectroscopic redshift of 1.753. The redshift is of the brightest cluster galaxy (BCG), which is coincident with the peak…

astro-ph2004★ 45 cited

Evolution of the Cluster X-ray Luminosity Function

C. R. Mullis, A. Vikhlinin, J. P. Henry +6

We report measurements of the cluster X-ray luminosity function out to z=0.8 based on the final sample of 201 galaxy systems from the 160 Square Degree ROSAT Cluster Survey. There…

astro-ph2003★ 106 cited

XMM-Newton discovery of an X-ray filament in Coma

A. Finoguenov, U. G. Briel, J. P. Henry

XMM-Newton observations of the outskirts of the Coma cluster of galaxies confirm the existence of a soft X-ray excess claimed previously and show it comes from warm thermal emissio…

astro-ph2000

Evolution of the cluster X-ray luminosity function from the WARPS survey

L. R. Jones, H. Ebeling, C. Scharf +5

The evolution of the X-ray luminosity function of clusters of galaxies has been measured to z=0.85 using over 150 X-ray selected clusters found in the WARPS survey. We find no evid…