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Êîäèðîâêà: Mac-cyrillic
CV
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Curriculum vitae
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Research Position ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ European Southern Observatory ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠStaff astronomer since 09/2008 Interests ƒŠ ƒŠ ƒŠ ƒŠ AGN evolution and host galaxy properties ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠAGN feedback ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠAGN obscuration and SED ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠX-ray, optical, IR, sub-mm instrumentation 09/2006- ƒŠ ƒŠ ƒŠ ƒŠ Fellow at ESO 08/2008 04/2003- ƒŠ ƒŠ ƒŠ ƒŠ Postdoc at ƒŠMPE 07/2006 07/2000- ƒŠ ƒŠ ƒŠ ƒŠ Student at ESO 03/2003 Education 2000-2003 ƒŠ ƒŠ ƒŠUniversity of Roma TREƒŠ(Rome, Italy) ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠPhD in Physics (Advisor: Prof. Rosati and Prof. Matt) ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ "A new view of Active Galactic Nuclei with the X-ray satellitesƒŠXMM-Newton and Chandra" 1993-1999 ƒŠ ƒŠ University of Roma Tor VergataƒŠ (Rome, Italy) ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠLaurea in Physics (Advisors: Prof. Scaramella and Prof. Vittorio) ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ ƒŠ "Dynamical Evolution of Large Scale Structures in theƒŠUniverse:ƒŠdetectability by means of redshift surveysâÀÝ http://www.eso.org/public/http://www.mpe.mpg.de/indexhttp://www.uniroma3.it/http://web.uniroma2.it/shapeimage_2_link_0shapeimage_2_link_1shapeimage_2_link_2shapeimage_2_link_3