July 29, 2015 to August 6, 2015
World Forum
Europe/Amsterdam timezone

Recent follow-up observations of GRBs in the very high energy band with the MAGIC Telescopes

Aug 3, 2015, 11:15 AM
15m
Word Forum Theater (World Forum)

Word Forum Theater

World Forum

Churchillplein 10 2517 JW Den Haag The Netherlands
Oral contribution GA-EX Parallel GA12 EGAL

Speaker

Alessandro Carosi (INAF-ASDC)

Description

Gamma-ray burst (GRBs) are primary targets for all modern IACT telescope. The MAGIC collaboration has identified the detection of GRBs in the VHE regime as one of its multi-year key observational programs (KOP). However, the transient and unpredictable nature of GRBs makes pointing and rapid follow-up observations to observe the prompt emission phase difficult for large ground-based Cherenkov facilities. Thanks to its fast pointing speed and low-energy sensitivity, MAGIC is particularly well suited for GRB studies in the VHE range below ~100 GeV during the prompt-to-early afterglow phase. Since beginning operation in 2005, MAGIC has performed 72 follow-up observations that, to date, have yielded no significant detections. However, in the last two years, the MAGIC system upgrade and an improved GRB observation procedure has made possible follow-up of GRBs within ~100s after the event onset, hence opening a new phase in MAGIC GRB monitoring. In this contribution, I will show the achieved MAGIC performance for prompt observations and transient source detection, and will also report results from some GRB MAGIC observations.
Registration number following "ICRC2015-I/" 444
Collaboration MAGIC

Primary author

Co-authors

Elena Moretti (MPI) Francesco Longo Koji Noda (Max-Planck-Institute for Physics) Lucio Angelo Antonelli (INAF) Markus Garczarczyk (DESY) Markus Gaug (Universitat Autònoma de Barcelona) Martin Will (IFAE) Masahiro Teshima (Max-Planck-Institute) Massimo Persic (INAF) Saverio Lombardi (INAF) Stefano Covino (INAF / Brera) Susumu Inoue (Institute for Cosmic Ray Research, University of Tokyo) Takeshi Toyama (MPI)

Presentation materials

There are no materials yet.