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Field Area/deg2 Slim[cgs] N/deg2 N(zspec) zmed logLmed Ref. ... 6% CDFN. CLASXS. COSMOS. 5-8% Due to redshift spikes, cannot divide in z bins in the CDF-S/N ...
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Find 3:1 ratio, flat or increasing with redshift. HST ACS color image ... Treister & Urry 2006: meta-analysis shows obs/unobs ratio flat or increases with z ...
The X-ray background in the Chandra and XMM-Newton era. Andrea Comastri (INAF-OABologna-Italy) ... Deep X-ray surveys have resolved some 80% of the XRB (below a ...
Obscured AGN and the synthesis of the cosmic X-ray background ... isotropy suggests an. extragalactic origin. All sky X-ray maps. G a l a c t i c p l a n e ...
The two big scenarios. Early on. Strong galaxy interactions= violent star-bursts ... Magorrian (end 90') BH in local bulges, tight correlations MBH-Bulge properties ...
Corral 07 (see poster #1) Averaging AXIS XWAS (Tedds 07) ... Average spectra show narrow Fe lines in both BLAGN and NELGs (Amalia Corral's poster #1) ...
X-ray spectroscopy of bright AGN Giorgio Matt & Stefano Bianchi (Dipartimento di Fisica, Universit Roma Tre) Bright AGN Some open problems (which can be addressed ...
... in the most local bulges; tight correlation between MBH and bulge properties. ... Most bulges passed a phase of activity: Complete SMBH census, ...
Space Telescope Science Institute. and INAF-IRA. Alessandro Capetti INAF Torino Observatory ... THE HUBBLE SPACE TELESCOPE. 1. What is the origin for ...
Chandra Deep Field-North data. Source Redshifts. Diversity of X-ray selected sources ... Moderately deep Chandra surveys reported little overlap with the submm source ...
high-z type 2 quasar candidates. SED's of spectroscopically ID'd sources. 3. SEXSI Survey ... Many BLAGN fit a typical quasar SED (Elvis et al. 1994) ...
Stellar populations, star formation and their evolution over ... galaxies (Garching-MPA, Stephane Charlot, Jarle Brichmann, Simon White, Guinevere Kauffmann) ...
Fondamenti di Java Introduzione alla costruzione di GUI (graphic user interface) component - container - layout awt component hierarchy awt container hierarchy Swing ...
SED, radio-optical-X-ray luminosity correlations. Nature of accretion flow: thin disk? ... Supporting radio (VLA and VLBI) and optical (HST) data. e.g. 3C 452 ...
ExAO experiments can be done today. with a 'well-corrected sub-aperture' (WCS) ... oversized and off-centered Lyot stop and. inexact p phase-shift. measured 'ideal' ...
Dust-Obscured Gamma-Ray Bursts and the Cosmic Star-Formation Rate astro-ph/ 1301.5903 + A. J. Levan (Warwick), N. R. Tanvir (Leicester), S. B. Cenko, J. S. Bloom (UC ...
Strong constraints to models for the formation and evolution of structure in the Universe ... Miss most highly obscured AGN. La Franca et al. 2005. 2-10 keV ...
The Chandra Multi-wavelength Project (ChaMP) PIs: Paul Green & Belinda Wilkes X-ray: Dong-Woo Kim Imaging: Rob Cameron, Wayne Barkhouse Spectroscopy: John Silverman
Boston, November 2006. Extragalactic X-ray surveys. Paolo Tozzi ... Pascual et al. 2001. Tresse et al. 2002. Sullivan et al. 2000. Lilly et al. 1996. Lines from 60 ...
Distributed Ray Tracing CIS 681 CIS 681 Anti-Aliasing Graphics as signal processing Scene description: continuous signal Sample digital representation Reconstruction ...
Geoffrey McLennan,2 Eric A. Hoffman,2 Roderick Swift1 ... Blue line in Projections view indicates the airway branch viewed as a virtual endoscopic movie. ...
manual for the standardization of colposcopy for the evaluation of vaginal products world health organization steps to be carried out when performing colposcopy
Astrophysical Gravitational Wave Backgrounds Cosmological supernovae as neutrino and gravitational wave sources mHz gravitational wave background from inspiral of ...
NASA Goddard Space Flight Center, Exploration of the Universe Division & Joint Center for Astrophysics, ... public data, imager IBIS/ISGRI, 20 - 40 keV ...
for the first time, to compare high-redshift & low-redshift samples ... There is an astonishing amount of agreement---we understand the X-ray samples very well! ...
WHIM Backlight Scaling relation fudge factor Point source contaminant Cooling problem get-out clause AGN/GALAXY COEVOLUTION Kirpal Nandra Imperial College London
Wave Background for LISA. G nter Sigl. GReCO, Institut d'Astrophysique de Paris, CNRS et ... This gravitational wave background may be observable by LISA. ...
Robust identification of distant Compton-thick AGNs. IR AGN ... First insight into AGN activity in a Distant Protocluster. Lehmer, Alexander, et al., in prep ...
... selection of the most bolometrically luminous far-IR galaxies in Universe ... Before SCUBA2, submm will miss hot ultraluminous sources. Hughes et al. (1998) ...
Interpretation: AGN obscured at their birth (Fabian 1998, Hopkins 06) Number of C-thick AGN: largely unknown but see talks by Fabian & Comastri. 2-3:1. 4:1 ...