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Welcome on the residential home of ACCEPT, a challenge at Michigan State University by Kenneth Cavagnolo,office 2010 Professional Plus activation, Megan Donahue,office Standard 2010 activation, Mark Voit, and Ming Sun. The objective of this web site could be to distribute the science-ready info programs and finalized analysis outcomes for you -- the interested researcher. Updates and RSS Feed This website can be updated as new cluster observations become available in the CDA and as the challenge expands to include evaluation of XMM-Newton data. Stay up-to-date by subscribing to our RSS feed. A schedule of upcoming 'Clusters of Galaxies' Chandra observations to be made public is provided here. The typical timeline for new observations to be processed and added to this page is 1 day. Citation Request If you find a use in your work for that data or outcomes of ACCEPT, please cite our paper:
"Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters"
Cavagnolo, Kenneth W.; Donahue,office 2007 Professional Plus product key, Megan; Voit,windows 7 ultimate serial, G. Mark; Sun,microsoft office 2007 Enterprise activation key, Ming
ADS Listing
BibTeX Entry Useful Info and Figures 0) Download an ASCII version of the main table.
1) Download an ASCII file containing all of the data for ACCEPT.
2) Download a FITS file containing all of the info for ACCEPT (coming soon).
3) Download a FITS file for your HIFLUGCS subsample (coming soon).
4) Download a montage image of the ACCEPT clusters ordered by ascending core entropy (WARNING: 18Mb file). Explanation of Main Table Below is the main table which lists all the clusters in ACCEPT. To view an individual cluster click about the ObsID and a new tab will open with that clusterObsID's page. Each page contains: Wide-field Chandra image of cluster.
Image of the cluster core.
SDSSDSS image of the cluster core.
Light curve for the observation.
Surface brightness profile.
Image of temperature bins plus temperature profile.
Density profile.
Metal abundance profile.
Pressure profile.
Entropy profile.
Cooling time profile.
Gravitating mass profile (NOT THE CRUX OF THIS WORK, USE AT OWN RISK!).