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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)....


Degenaar, N.;  Wijnands, R.;  Campana, S.;  Galloway, D.;  Lewin, W.;  Homan, J.;  Chakrabarty, D.;  Jonker, P.;  Cackett, E.;  Miller, J.

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