Poster(s)
Radio quieti + SKA
Photos : Marcella Brusa
AGN9 - FERRARA
Blue shift asymmetric profiles in high L/Le sources Marziani et al. High ionization winds in the Broad Line Region of QSO
AGN9 - FERRARA
Two set of lines shift of 2650 lm/s Montuori et al. SDSS (555) : a candidate massive BH BinaryMonica Colpi talk
AGN9 - FERRARA
7 QSO physical pairs 50 - 500 kpc M dyn ~ 8 x 1012
Mhost ~ 1.4 x 1012Farina et al. Close by Quasars Pairs
AGN9 - FERRARA
AGN is a galaxy with aflux in excess to that predicted by its SF
Two type of AGN red and deadblue and alive Bardelli & zCOSMOS+VLACOSMOS The environment of radio AGN and the quest for feedback
AGN9 - FERRARA
Simultaneous data do not reduce scatterin the relation(s)
Antonucci et al. A study of the X-ray to UV ratio of AGN with simultaneous measurements from XMM
AGN9 - FERRARA
X-ray detected EROs (R-K > 5) z ~ 1 High fx/foptObscured AGN 10% of the X-ray population
5% of the EROs sample
Campisi et al.On the nature of red galaxies : the Chandra perspective
AGN9 - FERRARA
Cazzoli et al. Analysis of a LSS at z ~ 0.3 with the Chandra Observatory Source counts logN-logS In between two Clusters of galaxies
Small but significant Excess
Need spectroscpy to Associate X-ray sourcesTo the LSS
AGN9 - FERRARA
Tamborra et al. The soft X-ray emission of Seyfert 2 galaxies Soft X-ray emissionAs a blend of emission LinesUnresolved with CCD Resolution
Photoionization from Nuclear continuum
Small contribution From collisional Excitation
AGN9 - FERRARA
Brusa et al. Iron Line in the integrated spectra of high-z AGN Rest frame Stacking in Chandra deep Fields (1 Ms CDFS + 2 Ms CDFN
Line is there No evidence of broadening In progress
AGN9 - FERRARA
Risaliti et al. [OIII] EW and orientation effects in quasars [OIII] EW as a measure ofAccretion disk inclination From 6000 SDSS QSO The distribution is consistent withA random orientation
Prove of disk like structure Of ionizing radiation
AGN9 - FERRARA
Pozzi et al. Bolometric Luminosity of Type 2 AGN16 HELLAS2XMM Type 2 QSO + Spitzer coverage Nuclear luminosity from torus SED fitting + MBH from scaling relationsLow Eddington ratio sources Kbol correlates with Eddington ratio
AGN9 - FERRARA
Feltre et al. Dust Distribution in AGN SMOOTH vs CLUMPY SED of clumpyAnd smooth models Present similar properties
Good fits to IRS Spectra
AGN9 - FERRARA
Keck/DEIMOS spectrum: red, early type continuum plus strong AGNemission lines ([NeV] doublet) and SF features (OII, SFR ~ 103 M_sun /yr)Evidence of outflowing material (~300 km/s) from the blueshiled MgIand MgII complex absorpOon.
Caught in the act
Brusa et al. Feedback in action in a z ~ 1.6 obscured QSO
AGN9 - FERRARA
Severgnini et al. Newly discovered Compton Thick AGN in the local UniverseX-ray + IR selection
X-hard /Mid IR
Vs
HR4 (5-12/2-5)
Candidate CT
AGN9 - FERRARA
Vignali et al. Compton Thick quasars in the SDSSCT QSO are selected from[OIII] luminosity and Comparison with X-ray Luminosity or UL
Weak or absent in X Candidate CT
Space densities
AGN9 - FERRARA
Mignoli et al. Discovering heavily obscured AGN in COSMOS via [NeV] detection [NeV] in ~10 k spectra visually inspectedNeed hard ionizing cont. -- low NeV/X ratio observed In NL - Gilli (2010) plot candidate CT
AGN9 - FERRARA
Giovannini Square Kilometer Array (SKA) Factor 50 improvement in collecting area
AGN9 - FERRARA
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