Office Professional ACCEPT Archive of Chandra Clu

Welcome to your house of ACCEPT Microsoft Office 2007, a venture at Michigan State University by Kenneth Cavagnolo Office 2007 Professional Key, Megan Donahue, Mark Voit, and Ming Sun. The goal of this web site could be to distribute the science-ready info merchandise and finalized evaluation benefits to you personally -- the interested researcher. Updates and RSS Feed This online site will undoubtedly be updated as new cluster observations become available in the CDA and as the undertaking expands to include analysis 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 your data or success of ACCEPT, please cite our paper:
"Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters"
Cavagnolo Office 2010 Professional, Kenneth W.; Donahue Office 2010 Professional Plus, Megan; Voit, G. Mark; Sun, 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 information for ACCEPT.
2) Download a FITS file containing all of the data for ACCEPT (coming soon).
3) Download a FITS file for the 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 on 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 Office Professional!).