Calendar
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The shape of the cutoff in the synchrotron emission of SN 1006 observed with XMM-Newton | Marco Miceli ( INAF – Osservatorio Astronomico di Palermo)
15:30
The shape of the cutoff in the synchrotron emission of SN 1006 observed with XMM-Newton | Marco Miceli ( INAF – Osservatorio Astronomico di Palermo)
@ Aula OAPA
May 16 @ 15:30 – 16:30
Synchrotron X-ray emission from the rims of young supernova remnants allows us to study the high-energy tail of the electrons accelerated at the shock front. The analysis of X-ray spectra can provide information on the physical mechanisms that limit the energy achieved by the electrons in the acceleration process. We analzsed the deep observations of the XMM-Newton SN 1006 Large
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ngCFHT: a 10-m class survey spectroscopic facility on Mauna Kea | Paolo Spanò ( National Research Council of Canada – Herzberg Institute of Astrophysics )
15:30
ngCFHT: a 10-m class survey spectroscopic facility on Mauna Kea | Paolo Spanò ( National Research Council of Canada – Herzberg Institute of Astrophysics )
@ Aula OAPA
May 30 @ 15:30 – 16:30
Many forefront astrophysical studies are based on imaging survey data. There is a clear need to complement them with dedicated spectroscopic surveys, especially at medium and high resolution. While some 4-m class instruments exist or have been planned, a real gain can be obtained by transforming the CFHT in a 10-m telescope to perform wide-field, high-multiplexing, multi object spectroscopy by
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