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SUMMARY:A view from the window\, birth and growth of X-Ray Astronomy
DTSTART;VALUE=DATE-TIME:20030129T100000Z
DTEND;VALUE=DATE-TIME:20030129T110000Z
DTSTAMP;VALUE=DATE-TIME:20130525T124239Z
UID:indico-event-a03180@cern.ch
DESCRIPTION:The history and evolution of X-ray astronomy presented on the 
 occasion of the Nobel Prize 2002\, which was awarded to Riccardo Giacconi.
 \n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a03180
LOCATION:INTEGRAL Science Data Centre
URL:http://indico.cern.ch/conferenceDisplay.py?confId=a03180
END:VEVENT
BEGIN:VEVENT
SUMMARY:The CANGAROO Project - TeV gamma-ray observations by ground-based 
 telescopes in Australia
DTSTART;VALUE=DATE-TIME:20030131T100000Z
DTEND;VALUE=DATE-TIME:20030131T110000Z
DTSTAMP;VALUE=DATE-TIME:20130525T124239Z
UID:indico-event-a03181@cern.ch
DESCRIPTION:CANGAROO (the Collaboration of Australia and Nippon (Japan) \n
 for a GAmma Ray Observatory in the Outback) project has been \nexploring t
 he southern sky in the sub-TeV to multi-TeV energy range \nusing the groun
 d-based Cherenkov telescopes located in South Australia.\nSupernova remnan
 ts of non-thermal X-ray detection\, rotation-powered pulsars\nof large dE/
 dt over d2 value\, and other galactic unique objects \nincluding our Galac
 tic Center have been selected as observation targets\,\ntogether with some
  nearby X-ray selected BL Lacs and (starburst) galaxies.\nIntroduction of 
 the project and some recent results will be presented.\n\nhttp://indico.ce
 rn.ch/conferenceDisplay.py?confId=a03181
LOCATION:INTEGRAL Science Data Centre (isdc.unige.ch)
URL:http://indico.cern.ch/conferenceDisplay.py?confId=a03181
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BEGIN:VEVENT
SUMMARY:Spectro-temporal Studies of Microquasars in X-rays
DTSTART;VALUE=DATE-TIME:20030311T100000Z
DTEND;VALUE=DATE-TIME:20030311T110000Z
DTSTAMP;VALUE=DATE-TIME:20130525T124239Z
UID:indico-event-a03182@cern.ch
DESCRIPTION:Microquasars are binary systems in our Galaxy composed of a no
 rmal star\nand a stellar mass black hole (or a neutron star). Their name c
 omes from\nthe fact that the compact object ejects matter in powerful jets
  similar\nto those observed in distant quasars. This talk will be dedicate
 d to the\nstudy of three microquasars\, hosting a black hole\, mainly thro
 ugh the\nspectral and temporal properties of their soft (1-10 keV) and har
 d\n(10-100 keV) X-ray emissions.\n\nI will first briefly define and presen
 t the useful terms and the basic \nphysics underlying the phenomena occurr
 ing in the close vicinity of\nthese objects from both the spectral and tem
 poral point of view.\nI will then turn to the study of two microquasars\, 
 GRO J1655-40 and GRS\n1915+105 and present the link between quasi-periodic
  oscillations \n(QPO) and spectral parameters. I show how the spectro-temp
 oral behavior\nof both sources\, although different\, are in good agreemen
 t with the\ntheoretical predictions of the Accretion-Ejection Instability 
 (AEI).\n\nA third object\, XTE J1550-564\, will be then studied over a per
 iod of\noutbursts. I will  point out the presence of two different X-ray e
 mitting\nmedia\, which relative geometry may be changing through the outbu
 rst.\nI will also present the evolution of low frequency QPOs and compare 
 it\nto the theoretical predictions of some models of these features.\n\nAs
  a conclusion\, I will discuss all these results in the framework of\ntheo
 retical models compatible with the observations presented along this talk.
 \n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a03182
LOCATION:INTEGRAL Science Data Centre (isdc.unige.ch)
URL:http://indico.cern.ch/conferenceDisplay.py?confId=a03182
END:VEVENT
BEGIN:VEVENT
SUMMARY:SESAME Training Advisory Committee Meeting
DTSTART;VALUE=DATE-TIME:20110908T060000Z
DTEND;VALUE=DATE-TIME:20110909T160000Z
DTSTAMP;VALUE=DATE-TIME:20130525T124239Z
UID:indico-event-154672@cern.ch
DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=154672
LOCATION:International Center for Theoretical Physics (ICTP) Oppenheimer R
 oom
URL:http://indico.cern.ch/conferenceDisplay.py?confId=154672
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