X-ray observations of LSI+61303 with swift

J. Holder, Abraham David Falcone, D. Morris

Research output: Contribution to conferencePaper

1 Citation (Scopus)

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 languageEnglish (US)
Pages571-574
Number of pages4
StatePublished - Jan 1 2007
Event30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico
Duration: Jul 3 2007Jul 11 2007

Other

Other30th International Cosmic Ray Conference, ICRC 2007
CountryMexico
CityMerida, Yucatan
Period7/3/077/11/07

Fingerprint

large scale integration
x rays
orbitals

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics

Cite this

Holder, J., Falcone, A. D., & Morris, D. (2007). X-ray observations of LSI+61303 with swift. 571-574. Paper presented at 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico.
Holder, J. ; Falcone, Abraham David ; Morris, D. / X-ray observations of LSI+61303 with swift. Paper presented at 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico.4 p.
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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.",
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Holder, J, Falcone, AD & Morris, D 2007, 'X-ray observations of LSI+61303 with swift' Paper presented at 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico, 7/3/07 - 7/11/07, pp. 571-574.

X-ray observations of LSI+61303 with swift. / Holder, J.; Falcone, Abraham David; Morris, D.

2007. 571-574 Paper presented at 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico.

Research output: Contribution to conferencePaper

TY - CONF

T1 - X-ray observations of LSI+61303 with swift

AU - Holder, J.

AU - Falcone, Abraham David

AU - Morris, D.

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N2 - 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.

AB - 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.

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Holder J, Falcone AD, Morris D. X-ray observations of LSI+61303 with swift. 2007. Paper presented at 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico.