activity
19982009
most citedThe ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy Cluster Survey. V. The cluster catalogue

653 citations · 1k across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2009

Million Degree Plasmas in Extreme Ultraviolet (EUV) Astrophysics

Michael P. Kowalski, Martin Barstow, Frederick Bruhweiler +12

Million degree plasmas are ubiquitous in the Universe, and examples include the atmospheres of white dwarfs; accretion phenomena in young stars, cataclysmic variables and active ga…

astro-ph2004★ 653 cited

The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy Cluster Survey. V. The cluster catalogue

H. Boehringer, P. Schuecker, L. Guzzo +11

We present the catalogue of the REFLEX Cluster Survey providing information on the X-ray properties, redshifts, and some identification details of the clusters in the REFLEX sample…

astro-ph2002★ 4 cited

The Joint astrophysical Plasmadynamic EXperiment (J-PEX): A high-resolution rocket spectrometer

M. A. Barstow, N. P. Bannister, R. G. Cruddace +10

We report on the successful sounding rocket flight of the high resolution (R=3000-4000) J-PEX EUV spectrometer. J-PEX is a novel normal incidence instrument, which combines the foc…

astro-ph2001★ 19 cited

High-Resolution Spectroscopy of G191-B2B in the Extreme Ultraviolet

R. G. Cruddace, M. P. Kowalski, D. J. Yentis +14

We report a high-resolution (R=3000-4000) spectroscopic observation of the DA white dwarf G191-B2B in the extreme ultraviolet band 220-245 A. A low- density ionised He component is…

astro-ph2001★ 2 cited

The REFLEX Galaxy Cluster Survey IV: The X-ray Luminosity Function

H. Boehringer, C. A. Collins, L. Guzzo +10

The X-ray galaxy cluster sample from the REFLEX Cluster Survey, which covers the X-ray brightest galaxy clusters detected in the ROSAT All-Sky Survey in the southern sky, is used t…

astro-ph2001★ 50 cited

Non-Gaussian morphology on large scales: Minkowski functionals of the REFLEX cluster catalogue

M. Kerscher, K. Mecke, P. Schuecker +6

In order to quantify higher-order correlations of the galaxy cluster distribution we use a complete family of additive measures which give scale-dependent morphological information…