Observational signatures of gas flows toward the center of galaxies
COSMOS 24 / 100 / 160 μ m
The merger-AGN connection since z~1: causal or circumstantial?
Observational signatures of gas flows toward the center of galaxies Thaisa Storchi Bergmann Instituto de Física, UFRGS, Brazil Collaborators: Barbosa,
HST Workshop Bologna Jan 31, 2008 Heavily obscured SMBH at high redshift Andrea Comastri INAF - OABologna C. Vignali, R. Gilli, K. Iwasawa, F. Civano,
AEGIS-X: Results from the Chandra survey of the Extended Groth Strip
What can emission lines tell us? lecture 2 Grażyna Stasińska
Galaxies and AGNs
Impact of Jet Feedback on H 2 and Star Formation in Radio Galaxies
Heavily obscured SMBH at high redshift