Periodic very high energy gamma-ray emission from LS I +61 303 observed with the MAGIC telescope

Details Periodic very high energy gamma-ray emission from LS I +61 303 observed with the MAGIC telescope Periodic very high energy gamma-ray emission from LS I +61 303 observed with the MAGIC telescope

2008-06-11

arxiv.org/abs/0806.1865v1

Astrophys.J.693:303-310,2009

Astronomy and Astrophysics

Astrophysics

7 pages, 8 figures, submitted to ApJ

Scientific paper

10.1088/0004-637X/693/1/303

The MAGIC collaboration has recently reported the discovery of gamma-ray emission from the binary system LS I +61 303 in the TeV energy region. Here we present new observational results on this source in the energy range between 300 GeV and 3 TeV. In total 112 hours of data were taken between September and December 2006 covering 4 orbital cycles of this object. This large amount of data allowed us to produce an integral flux light curve covering for the first time all orbital phases of LS I +61 303. In addition, we also obtained a differential energy spectrum for two orbital phase bins covering the phase range 0.5

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