HUBBLE SPACE TELESCOPE DAILY REPORT #2528 PERIOD COVERED: 0000Z (UTC) 12/28/99 - 0000Z (UTC) 12/29/99 Daily Status Report as of 363/0000Z 1.0 OBSERVATIONS SCHEDULED AND ACCOMPLISHED: 1.1 Completed STIS/CCD 8502 (CCD Functional for SMOV3a) The Space Telescope Imaging Spectrograph (CCD) was used to measure the baseline performance and commandability of the CCD subsystem. The proposal completed normally 1.2 Completed Two Sets of FGS 8532 (White Dwarf and M-Stars in the Solar Neighborhood; Revealing Binarity) FGS-1 was used to conduct a high angular resolution survey with FGS1r to detect binarity among nearby M dwarfs and white dwarfs. The observations completed with no reported problems. 1.3 Completed S/C 8519 (Exercising the HST 486 Flight Software) The objective of this test is to exercise and verify the new 486 computer and pointing control system flight software with activities not utilized in other SMOV3A proposals. This includes moving target tracking while under FGS control, the gen-slew capability, guide star handoffs, handoffs from FGS control to gyro control while tracking, onboard parallax correction and verification that the 2047s tracking limit no longer applies. No problems were encountered. 1.4 Completed Two Sets of WF/PC-2 8491 (Transition to hold, Decon and Cool Down Procedure) This program covers the transition from Protect Safe Mode to Hold Mode, then performs a Protect Decontamination. This is followed by a series of UV monitors and focus checks at -43C, then a special decon to take the instrument to -88C. Proposal 8491/SU E5 may have potential impacts due to extended re-acquisition attempts. Proposal 8491/25 may have potential impacts due to loss of lock. These proposal impacts are under investigation 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions: 08 Successful: 07 Scheduled Re-acquisitions: 06 Successful: 05 2.2 FHST Updates: Scheduled: 20 Successful: 20 2.3 Operations Notes: Loss of lock see HSTAR 7446 (326/23:13) 3.0 SIGNIFICANT FORTHCOMING EVENTS: Continuation of SMOV and normal science observations and calibrations. /CAW