By Raul Mujica, Roberto Maiolino
ISBN-10: 9812560491
ISBN-13: 9789812560490
ISBN-10: 9812702431
ISBN-13: 9789812702432
The massive volume of information got by means of surveys in all wavebands, from radio to X-rays, has allowed significant growth within the knowing of energetic Galactic Nuclei and in their cosmic evolution. This publication comprises the court cases of a convention meant to provide a wide review of the new effects acquired by means of contemporary AGN surveys over the full electromagnetic spectrum. subject matters which have been mentioned through the convention and are integrated during this quantity are: AGN evolution, contribution to the cosmic historical past, AGN luminosity capabilities in several wavebands, multiwavelength houses of AGN, unified version and unconventional AGN, reference to the host galaxies, co-evolution of AGN and galaxies, implications for the neighborhood density of supermassive black holes. destiny AGN surveys deliberate with coming near near new observational amenities also are incorporated.
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Additional info for Multiwavelength AGN Surveys: Proceedings Of The Guillermo Haro Conference 2003, Cozumel, Mexico 8 12 December 2003
Example text
Results, the reader is directed to the s u i t e of papers focused on the X-ray sample1, the optical imaging2, and the optical spectroscopy3. References 1. A. E. H. J. Helfand & D. Stern, A p J 596, 944 (2003). 2. E. S. H. J. A. Harrison, submitted t o A p J (2004). 3. E. , in preparation, (2004). PRELIMINARY RESULTS FROM THE XMM MEDIUM DEEP SURVEY L. MAR AS CHI^, M. TAJER', G. TRINCHIERI~,L. CHIAPPETTI~,L. PAIOR02, D. MACCAGN12, M. PIERRE3, J. SURDEJ4 AND 0. LE FEVRE5 I N A F Osservatorio Astronomic0 di Brera, via Brera 28, Milano, Italy, IASF via Bassini 15, Milano, Italy, C E A / D S M / D A P N I A S k v i c e d 'Astrophysique, Saclay, France, Institut d'Astrophysique et Ge'ophysique, Universite' de LiBge, Belgium, 5 L A M , Marseille, France The XMM Medium Deep Survey (XMDS) is a joint program that involves three XMM hardware institutes (in Milan, Italy; Saclay, France; Likge, Belgium) and the VIMOS VLT Deep Survey consortium (VVDS).
A. , A p J 564, 190 (2002). EXPLORING THE HARD X-RAY SKY WITH XMM-NEWTON E. PICONCELLIl, M. CAPP12, L. BASSAN12, G. DI COCC02 AND M. esa. es We report on a spectroscopic study of 90 hard X-ray sources observed with XMMNewton. This work provides the first step in the detailed study of the X-ray spectral properties of hard X-ray selected sources detected at faint fluxes (Fz-10 2 erg cm-' s-') near the knee of the LogN-Logs distribution. Our results illustrate well how a wide-angle survey allows population studies to be made as well as enabling tight constraints to be placed on some parameters of synthesis models of the Cosmic X-ray Background.
Not showing broad emission lines (Fig. 2a). The dispersion along the correlation in Fig. 40 dex in luminosity. Note 13 100 10 bu P g 1 U 0 1 2 Redshift 3 4 ,o-,e 10-14 1043 2-10 keV Flux cgs 10-~6 Figure 1. Left: The L(a-lOkeV)-z plane for the source samples in Table 1 (symbols as in Table 1). e. e. Chandra deep surveys) and LAS2XMM survey) respectively. Right: The flux-area diagram for several 2-10 keV surveys. e. it is mostly thank to this sample that it is possible to extend and validate the correlation at high X/O values, and therefore at high luminosities.
Multiwavelength AGN Surveys: Proceedings Of The Guillermo Haro Conference 2003, Cozumel, Mexico 8 12 December 2003 by Raul Mujica, Roberto Maiolino
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