Col. (1) Exposure time; col. (2) right ascension of cluster center; col. (3) declination of cluster center; col. (4) Galactic absorbing column density, NH; col. (5) redshift; col. (6) maximum radius from cluster center, Rmax; col. (7) minimum counts used per TX annulus; col. (8) average cluster temperature; col. (9) average cluster metal abundance; and col. (10) bolometric luminosity;
Smoothed and binnd wide-field Chandra X-ray image of cluster
A gaussian smoothing kernel with size 2 was applied to the flare-cleaned, level-2 events file binned with a factor of 8 to produce this image. Point sources have not been excluded and no exposure correction has been applied to this image.
Smoothed and binned Chandra X-ray image of the cluster "core"
Same as the wide-field image above but the binning factor used here was 2.
SDSS/DSS footprint overlaid on cluster core
The SDSS/DSS footprint (white box) is centered on the cluster core.