Astronomy and Astrophysics – Astronomy
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21831901r&link_type=abstract
American Astronomical Society, AAS Meeting #218, #319.01; Bulletin of the American Astronomical Society, Vol. 43, 2011
Astronomy and Astrophysics
Astronomy
Scientific paper
We combine the CIRS (Cluster Infall Regions in SDSS) sample of 72 clusters at z<0.1 with the HeCS (Hectospec Cluster Survey) sample of 74 clusters in the redshift range 0.1-0.3. Both samples are X-ray flux limited. HeCS contains over 20,000 new redshifts obtained with Hectospec on the MMT. We apply the caustic technique to this full sample of 148 clusters to measure M200 directly and to derive the NFW concentration from the fits of the mass profile to each cluster. We derive the correlation between concentration and mass and its spread at fixed mass and compare these measurements with the expected results from numerical simulations. We also tested the conjecture from some weak lensing studies that cluster concentrations substantially exceed model predictions.
This work is supported in part by a Cottrell College Science Award from the Research Corporation.
Diaferio Antonaldo
Geller Margaret J.
Rines Kenneth J.
No associations
LandOfFree
Mass Profiles and Concentration Parameters for 148 Clusters at z<0.3 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Mass Profiles and Concentration Parameters for 148 Clusters at z<0.3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass Profiles and Concentration Parameters for 148 Clusters at z<0.3 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1742434