@inproceedings{f67365744c0b438a862422bb839bdba2,
title = "Whipple telescope observations of LS I+61 303: 2004-2006",
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 2005-2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0 - 0.1 and 0.8 - 1, phases which are not included in the MAGIC data set.",
keywords = "Cherenkov detectors, Gamma-ray sources, X-ray binary stars",
author = "Gary Gillanders",
year = "2007",
month = jun,
doi = "10.1007/s10509-007-9473-0",
language = "English (Ireland)",
isbn = "0004-640X",
volume = "309",
series = "Astrophysics and Space Science",
publisher = "Springer",
pages = "299--303",
booktitle = "ASTROPHYSICS AND SPACE SCIENCE",
edition = "1-4",
}