HUBBLE SPACE TELESCOPE DAILY REPORT #2544 PERIOD COVERED: 0000Z (UTC) 01/20/00 - 0000Z (UTC) 01/21/00 Daily Status Report as of 021/0000Z 1.0 OBSERVATIONS SCHEDULED AND ACCOMPLISHED: 1.1 Completed Two Sets of STIS/CCD 8408 (STIS CCD Dark Monitor C8) The Space Telescope Imaging Spectrograph (CCD) was used to make a CCD bias calibration observation. This is to monitor the darks for the STIS CCD. The observations were executed as scheduled, and no anomalies were reported. 1.2 Completed STIS/CCD 8409 (CCD Bias Monitor C8) The Space Telescope Imaging Spectrograph (CCD) was used to monitor the bias in the 1x1, 1x2, 2x1, and 2x2 bin settings at gain=1, and 1x1 at gain = 4 in order to build up high-S/N superbiases and track the evolution of hot columns. The observations completed with no problems. 1.3 Completed FGS 8527 (Near Term Stability) FGS-2R was used to determine the near term stability of the instrument. The goals are twofold: {1} to establish the baseline Long Term Stability measurement for the new FGS and monitor changes in the relative plate scale and distortion since the SMOV MiniOFAD; and {2} to monitor changes in the transfer function over months. The proposal completed nominally. 1.4 Completed STIS/CCD/MA1/2 8505 (SM3a Contamination Plan) The Space Telescope Imaging Spectrograph (CCD, MA1 and MA2) was used to monitor STIS UV/optical sensitivity, using a spectrophotometric standard star. Changes due to contamination or other causes will be detected. The observations completed nominally. 1.5 Completed STIS/MA2 8509 (NUV MAMA Darks) The Space Telescope Imaging Spectrograph (MA2) was used to determine the health of the FUV MAMA detector by monitoring the background count rate. The observations completed with no reported problems. 1.6 Completed STIS/CCD 8202 (Bright Quasar Close Lensing Search) The Space Telescope Imaging Spectrograph (CCD) was used to make observations of HCLQ0353-2 as part of a second generation survey to search for bright lensing quasars. With the restored PSF, new images will be considerably more sensitive to the presence of both close separation and faint lens components, and because STIS reaches two magnitudes fainter the PC, the new snapshot images will have much greater dynamic range. The observations were executed as scheduled, and no anomalies were noted. 1.7 Completed WF/PC-2 8239 (Imaging the NLR in a Complete Sample of z<0.5 Radio-Quiet PG Quasars) The WF/PC-2 was used to observe quasar PG0052+251 and to determine its role in the evolution of galaxies, where a central engine leaves its visible imprints in the galaxy through strong ionization and heating of the ISM. The observations completed with no reported problems. 1.8 Completed STIS/CCD 8506 (STIS SM3a Corrector and Focus Check) The Space Telescope Imaging Spectrograph (CCD) was used to check the instrument's focus. The instrument's focus is checked in two ways: {1} taking a series of images with small dithering offsets {to effectively improve the spatial resolution, while rejecting cosmic rays and hot pixels}, and {2} stepping a star {in sub-pixel steps} across a narrow echelle slit {e.g., the 0.1x0.09 slit}, using the CCD. The observations completed with no reported problems. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions: 7 Successful: 7 Scheduled Re-acquisitions: 8 Successful: 8 2.2 FHST Updates: Scheduled: 18 Successful: 18 2.3 Operations Notes: Servicing Mission Observatory Verification (SMOV) activities continue. ROP SSR-1A was used to clear the SSR EDAC error counter on one occasion. The SSA transmitter was turned on and off three times per ROP IC-2. Per an operations request, an SSR-3 engineering performance characterization test was conducted at 020/1805Z. SSR-3 appeared to perform nominally, and will be turned off pending the completion of analyses. An SSR interrupt and events status log dump was performed at 020/1811Z. At 020/193711Z, a 486 ESB message 1101 hex was received, indicating a SERVO_RUNAWAY problem. This was probably a single event upset due to the vehicle passage through SSA level 1. HSTAR 7479 was written. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Continuation of SMOV and normal science observations and calibrations. /CAW