To:sot_shift from: Dan Schwartz date: 26 Aug 99, 10:00pm EDT Subject: SOT shift report, Shift M36 -------- See http://asc.harvard.edu/acis/SOT_reports/sot-shift.html, or /proj/ascwww/AXAF/extra/science/htdocs/acis/SOT_reports/Aug_26_1999_M36.txt. Shift M36 Start at 238:18:00 GMT = 02:00pm 26 Aug EDT End 10:00pm 26 Aug SOT Lead DAS Spac/Aspect RAC,MF FOT/Sci liason ERM HRC ACIS LT,RB (Times will be given in GMT on day 238/239. In general times are rough, not precise.) PLAN Run under stored command segment P8. Finish OBSID 0065 observing NGC 2516. Shut down ACIS to enter radiation belts. EVENTS Start of shift, OBSID 0065, 5 stars, 3 fid lights. 18:44 ACIS stop science run 20:13 ACIS video boards power down. 20:40 EPHIN rates start to increase. Actual belt entry. 21:40 Start CAP 338, to playback contents of ACA memory, to aid debug of failure to acquire stars. 00:00 LOS. NOTES/ISSUES/PROBLEMS Because the OR for OBSID 0065 only requested 11,000 sec on NGC2516, and because there was nothing else for the scheduler to do, we SAT IDLE, WITH ACIS TURNED OFF, for 5500 seconds while pointing at NGC2516 !! 4800 seconds of idle time are planned while pointing at the CRAB Pulsar at 238:18:40:35, for OBSID 0168. CAN THESE BE AVOIDED IN THE FUTURE?? FOT/MP is working on it! CSC has developed a fix to the OFLS system, to correct the positions searched for fid lights when the SIM is translated. This will be brought up here for testing tonight or tomorrow, and is planned to be installed prior to generating the P9 loads. It is REQUIRED for P9 loads. P8b has been replanned to restore most of the time needed for OBSID 1237, the HETG focus on Capella. This uses the CRAB pulsar idle time mentioned above to good advantage. The reworked schedule and command loads for the second half of Part 8 are now complete and products are available. This schedule takes up at 240:07:50, and continues through 242:06:20. The review meeting for these products is currently scheduled for Friday, Aug 27th, at noon. ACIS, RB, has reviewed and approved the DOT md240:0718.dot (if it doesn't change). The CAP 338 investigation was extremely fruitful. A 10.2 magnitude star failed to be acquired via OBC commands. However, in monitor mode it showed 2100 counts -- at strong signal that should be easily tracked. When the ACA was commanded directly from the ground, the star was acquired and tracked! This indicates that faint star acquisition failure is an OBC software and/or K-constant problem. T. Aldcroft finds that the OBC code does indeed impose a threshold, and identifies the relevant K-constant!! ------------------------------------------------------- Dan Schwartz, MS #3 das@head-cfa.harvard.edu phone: (617)495-7232 FAX: (617)495-7356 cell phone: (617)512-5627 pager: 800-759-8352 PIN 1636502 or e-mail 1636502@skytel.com -------------------------------------------------------