Swift XRT imaging observation of HETE J1900.1-2455

Details Swift XRT imaging observation of HETE J1900.1-2455 Swift XRT imaging observation of HETE J1900.1-2455

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..541....1k&link_type=abstract

The Astronomer's Telegram, #541

Astronomy and Astrophysics

Astronomy

2

X-Ray, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

We have obtained a Swift TOO observation of the millisecond X-ray pulsar HETE J1900.1-2455 on 2005 June 29 UT 21:36:06 for about 900s. The X-ray Telescope (XRT) observation was done in Photon Counting (imaging) mode. The source is clearly detected with significant pile-up. The bright point source is located at R.A.=19:00:08.4, Decl.=-24:55:16. We estimated an uncertainty of 5 arcsec. The millisecond X-ray pulsar is the only X-ray source in the field of view of the XRT.

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