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20042009
most citedA Catalog of Galaxy Clusters Observed by XMM-Newton

399 citations · 474 across the 5 of their papers we have counts for

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astro-ph200819 cited

OMCat: Catalogue of Serendipitous Sources Detected with the XMM-Newton Optical Monitor

K. D. Kuntz, Ilana Harrus, Thomas A. McGlynn +2

The Optical Monitor Catalogue of serendipitous sources (OMCat) contains entries for every source detected in the publicly available XMM-Newton Optical Monitor (OM) images taken in…

astro-ph2007399 cited

A Catalog of Galaxy Clusters Observed by XMM-Newton

S. L. Snowden, R. M. Mushotzky, K. D. Kuntz +1

Aims: We present a uniform catalog of the images and radial profiles of the temperature, abundance, and brightness for 70 clusters of galaxies observed by XMM-Newton. Methods: We u…

astro-ph200750 cited

Chandra ACIS Survey of M33 (ChASeM33): A First Look

Paul P. Plucinsky, Benjamin Williams, Knox S. Long +22

We present an overview of the Chandra ACIS Survey of M33 (ChASeM33): A Deep Survey of the Nearest Face-on Spiral Galaxy. The 1.4 Ms survey covers the galaxy out to $R \approx 18\ar…

astro-ph20064 cited

Discovery of an eclipsing X-ray binary with a 32.69 hour period in M101: an analog of Her X-1 or LMC X-4?

Jifeng Liu, Rosanne di Stefano, Jeffrey McClintock +3

We report the discovery of an eclipsing X-ray binary in M101, the first such system to be discovered outside the Local Group. Based on a sequence of 25 Chandra observations that sa…

astro-ph2005

One-Up On L1: Can X-rays Provide Longer Advanced Warning of Solar Wind Flux Enhancements Than Upstream Monitors?

M. R. Collier, T. E. Moore, S. L. Snowden +1

Observations of strong solar wind proton flux correlations with ROSAT X-ray rates along with high spectral resolution Chandra observations of X-rays from the dark Moon show that so…

astro-ph2004

G65.2+5.7: A Thermal Composite Supernova Remnant With a Cool Shell

R. L. Shelton, K. D. Kuntz, R. Petre

This paper presents archival ROSAT PSPC observations of the G65.2+5.7 supernova remnant (also known as G65.3+5.7). Little material obscures this remnant and so it was well observed…