Problems with PCU 0

May 12, 2000

Starting at about 1:06 UT May 12, 2000, the pressure in the propane volume of PCU 0 suddenly began decreasing. The propane pressure is expected to reach zero within a day. The PCU 0 high voltage is currently off. At this moment, we expect the xenon volume will be maintained, and we will test this early next week after the pressures have become stable.

We expect that PCU 0 will remain functional, have an increased background rate, and a somewhat different gain. We will provide additional information next week.

- Keith Jahoda for the PCA team

More Information about PCU 0

May 16, 2000

The propane layer of PCU 0 has effectively been emptied. The xenon layer pressure has come to equilibrium at a value about 0.5% lower. Pressure plots of loss can be found at http://asd.gsfc.nasa.gov/users/keith/pcu1/ . The xenon voltage in PCU 0 was turned on again briefly on May 15. The xenon total rates were similar to what they were when the propane layer was intact, as expected. The rate of events with one and only one xenon anode triggered were 20-25 % higher than the corresponding rate in PCU 2. The majority of this increase is expected to be due to electrons entering the top layer of the xenon volume, which used to be vetoed because they triggered both the propane layer and the top xenon layer. Further analysis of these data will be presented soon. Operations plans are being developed.

- Jean Swank, Project Scientist

PCU_0 Xenon HV turned on again

May 19, 2000

On May 17 (Day 138) at 15:00 UT, the xenon volume of PCU 0 was turned on again. We plan to continue using PCU 0 for upcoming RXTE observations, with occasional exceptions for operational reasons. The PCA Team is working to generate an appropriate background model and an updated response matrix for PCU 0.

PIs are advised to review their chosen EDS data modes for upcoming observations. The majority of cases will require no action: the Standard Modes, GoodXenon Modes, and many of the other modes used for faint sources contain detector ID and thus already allow separate analysis of the different detectors. Some Event, Binned and Single Bit modes used for bright sources do not contain detector ID, but for most timing purposes the PCU0 changes may not be significant. If you wish to request a change to your observing modes, please give the SOF as much lead time as possible.

- Jean Swank, Project Scientist