AGN in Clusters of Galaxies - Berkeley Cosmology Group

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AGN Fraction Measurement Abell 3128 (z=0.06) fA = NX (L>LX; MR
AGN Fraction vs. Environment >95% probability they are different Sivakoff et al. (2008)
Page 1 and 2: AGN in Clusters of Galaxies Paul Ma
Page 3 and 4: Cluster Physics & the Cool Core Pro
Page 5 and 6: Black Hole Evolution Rapid black ho
Page 7 and 8: Galaxy Evolution in Clusters Do the
Page 9: Demographics Berlind et al. (2006)
Page 12 and 13: Mock Catalogs Create a mock catalog
Page 14 and 15: Radio Power at 1.4 GHz [w/Hz/sr] Lu
Page 16 and 17: Fraction of Sources < Projected Jet
Page 18: Distribution of AGN within Clusters
Page 21 and 22: Spectroscopic Confirmation Identifi
Page 23 and 24: AGN Identification LMXBs Hot Gas Jo
Page 25 and 26: Centrally Concentrated AGN Luminous
Page 27: Centrally Concentrated AGN Implicat
Page 31 and 32: Field AGN Downsizing Silverman et a
Page 33 and 34: AGN in z>0.5 clusters
Page 35 and 36: Comparison to Field AGN More pronou
Page 37: Summary The FRII lifetime is ~10 7

AGN in Clusters of Galaxies - Berkeley Cosmology Group

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