19–22 Jun 2012
Lecce
Europe/Rome timezone

Session

The gamma-ray sky

04
21 Jun 2012, 15:15
Lecce

Lecce

Officine Cantelmo

Presentation materials

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  1. Ms Maja Llena Garde (Oskar Klein Centre, Stockholm University)
    21/06/2012, 15:15
    Dwarf spheroidal galaxies are considered very promising targets for dark matter searches in the gamma-ray band due to their large mass-to-light ratio and low astrophysical background. The gamma-ray signal is expected to be very faint, but a combined analysis of a set of dwarf galaxies improves the Fermi-LAT sensitivity to gamma-ray sources and yields enhanced constraints on the dark matter...
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  2. Dr Eugenio Bottacini (Stanford University)
    21/06/2012, 15:40
    In the view of the so-called Active Galactic Nuclei (AGN) unified model the nuclear activity is powered by a super-massive black hole (SMBH) at the center of the AGN. An optically thick gas-dust structure surrounding the SMBH absorbs efficiently the nuclear radiation. Current surveys of the INTEGRAL Soft-Gamma Ray Imager (IBIS/ISGRI) and of the Burst Alert Telescope (BAT) on board the...
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  3. Silvia Vernetto (INAF Torino and INFN)
    21/06/2012, 16:05
    ARGO-YBJ is an extensive air shower detector located in Tibet at 4300 m a.s.l. The detector features and location allow the study of gamma-ray sources with a few hundreds GeV energy threshold and very large duty cycle. Results so fare obtained will be reviewed.
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  4. Carlotta Pittori (INAF-OAR/ASDC)
    21/06/2012, 16:30
  5. Lorenzo Amati (INAF-IASF Bologna)
    21/06/2012, 16:55
    GRB emission: status and questions
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