Project overview:
XBACs, a sample comprising the 242 X-ray brightest Abell (ACO)
clusters of galaxies in the extragalactic sky (|b| > 20 deg) was the
first X-ray flux limited sample of clusters of galaxies to be compiled
from ROSAT
All-Sky Survey data. Although not X-ray selected (all XBACs
clusters were initially discovered by George Abell and collaborators)
the sample has proven tremendously useful for studies of the local (z
< 0.2) cluster population.
The compilation and characterization of the XBACs sample was the subject
of my PhD thesis (MPE Report 250, ISSN 0178-0719).
The sample:
Unabridged and complete electronic table that combines Tables 3 and 4 of the paper listed below.
(LaTeX to ASCII conversion and merging Of both tables by Heinz Andernach)
XBACs publications (by the XBACs team):
- Ebeling H., Voges W., Böhringer H., Edge A.C., Huchra J.P., Briel U.G.
Properties of the X-ray-brightest Abell-type clusters of galaxies (XBACs)
from ROSAT All-Sky Survey data - I. The sample, 1996,
MNRAS, 281, 799
There is a lot more science to be extracted from this sample, and one
day I hope to get around to writing some of it up...
Note that the table published in the above paper lacks 6 clusters
which were omitted from page 823 due to a typesetting error. We are
grateful to Heinz Andernach for pointing this out to us. An erratum has been published in MNRAS
(1996, 283, 1103).
(page last updated by H. Ebeling, January 9, 2001)