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TeV and X-ray Monitoring of LS I +61 303 With VERITAS, Swift, and RXTE by VERITAS Collaboration; Smith, A. is a scholarly article available to read on EtoBox.

What is TeV and X-ray Monitoring of LS I +61 303 With VERITAS, Swift, and RXTE about?

Between September 2006 and February 2007, the galactic binary LS I +61 303 was monitored in the TeV band with the VERITAS array of imaging Cherenkov telescopes. These observations confirm LS I +61 303 as a variable TeV gamma-ray source, with emission peaking between orbital phase 0.6 and 0.7. During this observational period, monitoring in the X-ray regime was also carried out using both the RXTE and Swift detectors, which offered complementary coverage of the source. Outbursts in the 0.2-10 keV band were observed by both satellites at close to the same orbital phase as the TeV peak during the 2 orbital cycles covered simultaneously in both bands. While this source has been extensively studied in the X-ray band in the past, this is the first observational campaign to utilize contemporaneous X-ray and TeV data on LS I +61 303.

Author
VERITAS Collaboration; Smith, A.
Published
2007
Language
EN

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