As a service to the astronomical community, we are recalibrating all archival Hubble Space Telescope Faint Object Spectrograph UV and optical spectrophotometry of active galaxies and quasars in order to extract uniformly calibrated spectrophotometric...
... which combines all the main spectral features of AGN/quasars into a single structure ... AGN Physics with the SDSS' astro-ph/03346 . Latest Update: . Video: . ... 2003 astro-ph/0311436 , to be published in AGN and the SDSS, eds. G. Richards and P ...
... THE STUDY OF AGN FROM UV to X-RAYS . ... Emission Line Properties of AGN from a post-COSTAR FOS HST Spectral Atlas" . ... for a Strong NV/CIV Correlation Between Emission and Absorption Lines in AGN ...
... AGN from the AEGIS/Chandra survey and QSOs from SDSS, I present the cross ... mass of AGN/QSOs as a function of X-ray luminosity, which constrains AGN formation ... AGN/host-galaxy co-evolution Link between AGN and environment differences among AGN ...
... Type I and II AGN, Absorption, XBONGs, Tuesday: AGN correlation functions, LSS ... role of AGN in galaxy evolution: how can observations help? statistics of AGN in ... AGN synthesis models for the XRB I will discuss the multiwavelength properties of ...
... AGN Populations beyond Redshifts 6 - 7 using Large X-ray Surveys Tozzi Spectral analysis of X-ray sources in the CDFS Steffen Extending alpha_OX studies to include the numerous low- to-moderate luminosity AGNs 1037am COFFEE BREAK & POSTERS (Rooms 2-3 and ...
... XMS team : M. Garcia April 14, 2010 XMS high/mid/low resolution event rates for bright AGN mrg-2010-02v2 This memo arises out of the concern that the bright AGN that will be used to observed strong gravity effects in particular those for which time ...
[
Текст
]
Ссылки http://hea-www.harvard.edu/~garcia/ixo/high_rate_agn_v3.pdf -- 204.4 Кб -- 31.01.2012 Похожие документы
... and X-ray (top, right) spectra of a typical quasar or AGN (Active Galactic Nucleus ... Broad Emission Lines ("BELs") [seen in 100% of AGN], . ... Narrow Absorption Lines ("NALs") [seen in 50% of AGN], . ...