Whipple telescope observations of LS I +61 303: 2004–2006

@article{Smith2007WhippleTO,
  title={Whipple telescope observations of LS I +61 303: 2004–2006},
  author={Aaron Drake Smith and Robert W. Atkins and Simon Bradbury and {\"O}zg{\"u}r Yaþar Çelik and Y. C. K. Chow and Peter Cogan and C. Dowdall and Stephen Fegan and Pascal D. Fortin and Daniel Gall and G. H. Gillanders and Jeffrey Grube and Kristopher Gutierrez and Tony A. Hall and D. S. Hanna and Jamie Holder and Diane Horan and Stephen B. Hughes and Thomas Brian Humensky and I. Jung and Phil Kaaret and Gary Kenny and M. Kertzman and David B. Kieda and Alexander Konopelko and Henric S. Krawczynski and Frank Krennrich and Matthew J Lang and S. Le Bohec and Gernot Maier and Joy Millis and Philip Moriarty and Rene A. Ong and Jimmye Shannon Perkins and K. Ragan and G. H. Sembroski and John A Toner and Lorea Valcarcel and V. V. Vassiliev and Robert Gene Wagner and Scott Patrick Wakely and Trevor C. Weekes and Russel Joseph White and D A Williams},
  journal={Astrophysics and Space Science},
  year={2007},
  volume={309},
  pages={299-303}
}
Abstract In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the… CONTINUE READING

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