Swift/XRT non-detection of HETE J1900.1-2455

Details Swift/XRT non-detection of HETE J1900.1-2455 Swift/XRT non-detection of HETE J1900.1-2455

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1098....1d&link_type=abstract

The Astronomer's Telegram, #1098

Astronomy and Astrophysics

Astronomy

5

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

Scientific paper

During a ~0.8 ksec pointed Swift/XRT observation performed on June 6, 2007 (18:26-21:38 UT), we did not detect the accreting millisecond pulsar HETE J1900.1-2455. We can set a 2-10 keV upper limit on the source flux of ~(5-15)E-14 erg/cm2/s (depending on the assumed spectral model). This is more than a factor of 10 weaker than the X-ray flux observed with Swift/XRT last week, on May 31 (ATEL #1091).

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