C. Scharf

Details der Publikationsliste

Zeitraum

1997 - 2009

Anzahl

13

Co-Autoren

A 100 kpc inverse Compton x-ray halo around 4C 60.07 at z = 3.79. (2009)

Smail, I., Lehmer, B.D., Ivison, R.J., Alexander, D.M., Bower, R., Stevens, J. A., ...

Original article can be found at: http://www.iop.org/EJ/journal/apjl Copyright American Astronomical Society. DOI: 10.1088/0004-637X/702/2/L114 [Full text of this article is not available in the UHRA]

An XMM-Newton observation of the massive, relaxed galaxy cluster ClJ1226.9+3332 at z=0.89 (2004)

Maughan, B. J., Jones, L. R., Ebeling, H., Scharf, C.

A detailed X-ray analysis of an XMM-Newton observation of the high-redshift (z=0.89) galaxy cluster ClJ1226.9+3332 is presented. The X-ray temperature is found to be 11.5{+1.1}{-0.9}keV, the highest...

An XMM and Chandra view of massive clusters of galaxies to z=1 (2003)

Jones, L. R., Maughan, B. J., Ebeling, H., Scharf, C., Perlman, E., Lumb, D., ...

The X-ray properties of a sample of high redshift (z>0.6), massive clusters observed with XMM-Newton and Chandra are described, including two exceptional systems. One, at z=0.89, has an X-ray...

Discovery of a very X-ray luminous galaxy cluster at z=0.89 in the WARPS survey (2000)

Ebeling, H., Jones, L. R., Fairley, B. W., Perlman, E., Scharf, C., Horner, D.

We report the discovery of the galaxy cluster ClJ1226.9+3332 in the Wide Angle ROSAT Pointed Survey (WARPS). At z=0.888 and L_X=1.1e45 erg/s (0.5-2.0 keV, h_0=0.5) ClJ1226.9+3332 is the most distant...

The X-ray evolution of clusters of galaxies to z=0.9 (2000)

Jones, L. R., Ebeling, H., Scharf, C., Perlman, E., Horner, D., Fairley, B. W., ...

The evolution of the X-ray luminosity function of clusters of galaxies has been measured to z=0.9 using over 150 X-ray selected clusters discovered in the WARPS survey. We find no evidence for...

The WARPS survey - IV: The X-ray luminosity-temperature relation of high redshift galaxy clusters (2000)

Fairley, B. W., Jones, L. R., Scharf, C., Ebeling, H., Perlman, E., Horner, D., ...

We present a measurement of the cluster X-ray luminosity-temperature relation out to high redshift (z~0.8). Combined ROSAT PSPC spectra of 91 galaxy clusters detected in the Wide Angle ROSAT Pointed...

Evolution of the cluster X-ray luminosity function from the WARPS survey (2000)

Jones, L. R., Ebeling, H., Scharf, C., Perlman, E., Horner, D., Fairley, B., ...

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 evidence for evolution...

The WARPS survey: III. The discovery of an X-ray luminous galaxy cluster at z=0.833 and the impact of X-ray substructure on cluster abundance measurements (1999)

Ebeling, H., Jones, L. R., Perlman, E., Scharf, C., Horner, D., Wegner, G., ...

The WARPS team reviews the properties and history of discovery of ClJ0152.7-1357, an X-ray luminous, rich cluster of galaxies at z=0.833. At L_X = 8 x 10^44 h^(-2) erg/s (0.5-2.0 keV) ClJ0152.7-1357...

The WARPS survey - II: The Log(N)-Log(S) relation and the X-ray evolution of low luminosity Clusters of Galaxies (1997)

Jones, L. R., Scharf, C., Ebeling, H., Perlman, E., Wegner, G., Malkan, M., ...

X-ray selected surveys of clusters of galaxies can distinguish between hierarchical models of the growth of structure in the Universe. Here we present the first results from an X-ray selected, flux...