Abstract
The TeV emitting high-mass X-ray binary system LSI+61303 was observed with the Swift satellite from early September 2006 to early January 2007. Many of these observations were contemporaneous with TeV observations. The data consist of observations on 24 separate days with durations ranging between 700s and 4700s, and partially cover 4.5 orbital periods of the binary system. We present here an analysis of the 0.2 to 10keV X-ray data from the Swift-XRT instrument. Contemporaneous optical data from UVOT are also available.
| Original language | English (US) |
|---|---|
| Pages | 571-574 |
| Number of pages | 4 |
| State | Published - 2007 |
| Event | 30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico Duration: Jul 3 2007 → Jul 11 2007 |
Other
| Other | 30th International Cosmic Ray Conference, ICRC 2007 |
|---|---|
| Country/Territory | Mexico |
| City | Merida, Yucatan |
| Period | 7/3/07 → 7/11/07 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics