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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