Prof.
Phil Allport
(University of Liverpool)
27/09/2010, 09:00
Radiation hardness of semicomductor detectors
Prof.
Samo Korpar
(University of Maribor and Jožef Stefan Institute)
27/09/2010, 10:00
Detector processing
Michael Moll
(CERN, Geneve)
27/09/2010, 11:00
Radiation hardness of semicomductor detectors
Ioana Pintilie
(NIMP Bucharest)
27/09/2010, 11:45
Radiation hardness of semicomductor detectors
Prof.
Gian-Franco Dalla Betta
(University of Trento, FBK Trento)
27/09/2010, 14:10
Prof.
Manuel Lozano
(CNM-IMB Barcelona)
27/09/2010, 15:00
Prof.
Manuel Lozano
(Instituto de Microelectronica de Barcelona (CNM-IMB))
27/09/2010, 16:30
Christian Joram
(CERN)
28/09/2010, 08:40
Nicola PACIFICO
(CERN)
28/09/2010, 09:00
Tomas Balog
(GSI)
28/09/2010, 09:08
Jennifer Sibille
(PSI)
28/09/2010, 09:16
Jiaguo Zhang
(University of Hamburg)
28/09/2010, 09:24
Cristina Pirvutoiu
(University of Hamburg)
28/09/2010, 09:32
Marko Milovanović
(Jožef Stefan Institute)
28/09/2010, 09:40
Marco Villa
(CERN)
28/09/2010, 09:48
Jing Dong
(INFN Frascati)
28/09/2010, 09:56
Stefano Caiazza
(DESY)
28/09/2010, 10:30
Rolf Schön
(NIKHEF)
28/09/2010, 10:38
Rahul ARORA
(GSI)
28/09/2010, 10:46
Jonathan Aguilar
(AGH Cracow)
28/09/2010, 10:54
Olga Novgorodova
(DESY)
28/09/2010, 11:02
Dr
Paolo Beltrame
(CERN)
28/09/2010, 11:10
Ruben Verheyden
(JSI)
28/09/2010, 11:18
Francesco Zappon
(NIKHEF)
28/09/2010, 11:26
Mohammed Imran Ahmed
(AGH Cracow)
28/09/2010, 11:34
Prasoon AMBALATHANKANDY
(AGH-UST Crakow)
28/09/2010, 11:42
Name: Prasoon Ambalathankandy
Supervisor: Dr. Marek Idzik
Institution: WFiIS, AGH University of Science and Tech., Cracow.
Supervisor: Dr. Marek Idzik
Institution: WFiIS, AGH University of Science and Tech., Cracow.
Dr
Shahinur RAHMAN
(GSI)
28/09/2010, 11:50
Tsagri Marie
(CERN)
28/09/2010, 11:58
Filimon ROUKOUTAKIS
(INFN Frascati)
28/09/2010, 12:06
Seamus Hegarty
(CERN)
28/09/2010, 15:30
Prof.
Margherita Hack
(INAF Osservatorio Astronomico di Trieste)
29/09/2010, 12:45
The seminar will present the information which can be obtained from the stellar spectra- temperature, density, state of the matter, chemical composition, and how the internal structure can be derived, which are the source of energy and how the continuous emission of radiation modifies the stellar structure. The mass is the parameter which affects the whole evolution of a star.