(20) link to Smithsonian/NASA Astrophysics Data System (ADS). (19) link to NASA/IPAC Extragalactic Database (NED) and col. (18) link to National Virtual Observatory (NVO) col. Entropy tables Chemists have found it possible to assign a numerical quantity for the entropy of each substance. (17) link to Chandra Data Archive (CDA) col. (10) best-fit entropy profile power-law index col. (9) best-fit entropy profile normalization at 100 kpc col. (5) right ascension of cluster center col. (3) observation identification number col. Values listed for K 0, K 100, and α are best-fit values of the model K(r) = K 0+K 100(r/100 kpc) α.īolometric luminosities are taken from a hetergeneous set of apertures new values for homogeneous apertures are being generated. Hence, low-redshift objects with upper limits may have a WAT radio source. Our NVSS and SUMSS search criteria miss large, amorphous sources like WATs. Gravitating mass profile (NOT THE CRUX OF THIS WORK, USE AT OWN RISK!).ĪCCEPT Main Table The table below is sortable by column, just click the column head to sort.Image of temperature bins plus temperature profile. Character Tables Links Standard Heats and Free Energies of Formation and Absolute Entropies of Elements and Inorganic Compounds.To view an individual cluster click on the ObsID and a new tab will open with that cluster/ObsID's page. Mark Sun, MingĠ) Download an ASCII version of the main table.ġ) Download an ASCII file containing all of the data for ACCEPT.Ģ) Download a FITS file containing all of the data for ACCEPT (coming soon).ģ) Download a FITS file for the HIFLUGCS subsample (coming soon).Ĥ) Download a montage image of the ACCEPT clusters ordered by ascending core entropy (WARNING: 18Mb file).īelow is the main table which lists all the clusters in ACCEPT. "Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters"Ĭavagnolo, Kenneth W. If you find a use in your work for the data or results of ACCEPT, Observations to be processed and added to this page is 1 day. Of Galaxies' Chandra observations to be made public is This site will be updated as new cluster observations becomeĪvailable in the CDA and as the project expands to includeĪnalysis of XMM-Newton data. Science-ready data products and finalized analysis results to The purpose of this web site is to distribute the University by Kenneth Cavagnolo, Megan Donahue, Mark Welcome to the home of ACCEPT, a project at Michigan State ACCEPT: Archive of Chandra Cluster Entropy Profile Tables
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