Poster(s)

1
Poster(s)
Radio quieti SKA

Photos Marcella Brusa
2
Blue shift asymmetric profiles in high L/Le
sources
High ionization winds in the Broad Line Region
of QSO
Marziani et al.
3
Two set of lines shift of 2650 lm/s
SDSS (555) a candidate massive BH Binary
Montuori et al.
Monica Colpi talk
4
7 QSO physical pairs 50 - 500 kpc M dyn 8 x
1012Mhost 1.4 x 1012
Close by Quasars Pairs
Farina et al.
5
AGN is a galaxy with aflux in excess to that
predicted by its SF Two type of AGN red and
deadblue and alive
The environment of radio AGN and the quest for
feedback
Bardelli zCOSMOSVLACOSMOS
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Simultaneous data do not reduce scatterin the
relation(s)
A study of the X-ray to UV ratio of AGN with
simultaneous measurements from XMM
Antonucci et al.
7
X-ray detected EROs (R-K gt 5) z 1 High
fx/foptObscured AGN 10 of the X-ray population
5 of the EROs sample
On the nature of red galaxies the Chandra
perspective
Campisi et al.
8

Analysis of a LSS at z 0.3 with the Chandra
Observatory
Cazzoli et al.
Source counts logN-logS In between two
Clusters of galaxies Small but significant
Excess Need spectroscpy to Associate X-ray
sources To the LSS
9

The soft X-ray emission of Seyfert 2
galaxies
Tamborra et al.
Soft X-ray emission As a blend of emission
Lines Unresolved with CCD Resolution Photoioniz
ation from Nuclear continuum Small
contribution From collisional Excitation
10

Iron Line in the integrated spectra of high-z AGN
Brusa et al.
Rest frame Stacking in Chandra deep Fields (1
Ms CDFS 2 Ms CDFN Line is there No evidence
of broadening In progress
11

OIII EW and orientation effects in
quasars
Risaliti et al.
OIII EW as a measure of Accretion disk
inclination From 6000 SDSS QSO The distribution
is consistent with A random orientation Prove
of disk like structure Of ionizing radiation
12

Bolometric Luminosity of Type 2 AGN
Pozzi et al.
16 HELLAS2XMM Type 2 QSO Spitzer coverage
Nuclear luminosity from torus SED fitting MBH
from scaling relations Low Eddington ratio
sources Kbol correlates with Eddington ratio
13

Dust Distribution in AGN SMOOTH vs CLUMPY
Feltre et al.
SED of clumpy And smooth models Present similar
properties Good fits to IRS Spectra
14
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
Feedback in action in a z 1.6 obscured QSO
Brusa et al.
15

Newly discovered Compton Thick AGN in the local
Universe
Severgnini et al.
X-ray IR selection X-hard /Mid IR Vs HR4
(5-12/2-5) Candidate CT
16

Compton Thick quasars in the SDSS
Vignali et al.
CT QSO are selected from OIII luminosity and
Comparison with X-ray Luminosity or UL Weak
or absent in X Candidate CT Space densities
17

Discovering heavily obscured AGN in COSMOS via
NeV detection
Mignoli et al.
NeV in 10 k spectra visually inspected Need
hard ionizing cont. -- low NeV/X ratio observed
In NL - Gilli (2010) plot candidate CT
18

Square Kilometer Array
(SKA)
Giovannini
Factor 50 improvement in collecting area