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DTSTART;TZID=Europe/Rome:20190122T114500
DTEND;TZID=Europe/Rome:20190122T124500
DTSTAMP:20260407T185400
CREATED:20180725T070311Z
LAST-MODIFIED:20180725T070311Z
UID:4172-1548157500-1548161100@www.oa-roma.inaf.it
SUMMARY:colloquium - Viola Allevato
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-viola-allevato/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20190122T114500
DTEND;TZID=Europe/Rome:20190122T124500
DTSTAMP:20260407T185400
CREATED:20180725T070311Z
LAST-MODIFIED:20190108T105344Z
UID:4757-1548157500-1548161100@www.oa-roma.inaf.it
SUMMARY:Clustering dependence of X-ray AGN on host galaxy properties
DESCRIPTION:The presence of a super massive BH in almost all galaxies in the Universe is an accepted paradigm in astronomy. How these BHs form and how they co-evolve with the host galaxy is one of the most intriguing unanswered problems in modern Cosmology and of extreme relevance to understand the issue of galaxy formation. Clustering measurements can powerfully test theoretical model predictions of BH triggering scenarios and put constraints on the typical environment where AGN live in\, through the connection with their host dark matter halos. In this presentation I will talk about the clustering properties of X-ray AGN from both an observational and theoretical point of view\, using the new catalog of AGN detected by Chandra in COSMOS and semi-empirical models. The Chandra COSMOS-Legacy catalog is one of the largest available sample of X-ray AGN for clustering studies\, allowing clustering measurements as a function of obscuration\, luminosity and AGN host galaxy properties.
URL:https://www.oa-roma.inaf.it/event/colloquium-viola-allevato-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
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