HUBBLE SPACE TELESCOPE DAILY REPORT #2309 PERIOD COVERED: 0000Z (UTC) 02/15/99 - 0000Z (UTC) 02/16/99 Daily Status Report as of 047/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed WF/PC-2 6353 (A Snapshot Emission Line Imaging Survey of Very Low Excitation Planetary Nebulas) The WF/PC-2 was used to make snapshot observations as part to an emission line survey of the very low excitation planetary nebula PK082+11D1 (Class PNe). This target was selected based on the O III/H alpha line flux ratio. The observations were executed as scheduled, and no anomalies were noted. 1.2 Completed STIS/CCD 7948 (CCD Dark and Bias Monitor -- Cont. to Dec. 98) The Space Telescope Imaging Spectrograph (CCD) was used to measure CCD dark current and bias rates for the two supported amplifier settings {GAIN=1 and GAIN=4} in order to gather data for making superdarks and superbiases. The data will be used to track the growth of hot pixels on the CCD in general and within the various target acquisition apertures specifically. The observations were executed as scheduled, and no anomalies were noted. 1.3 Completed STIS/CCD/MA2 7348 (Boron in the Extreme Pop II Star HD 140283) The Space Telescope Imaging Spectrograph (CCD and MA2) was used to make observations of the extreme POP II dwarf class star HD140283. Using the HST and ground-based observations it has been determined that there is an abundances of boron and beryllium in this star. A wavelength calibration image was also taken. The observations were executed as scheduled, and no anomalies were noted. 1.4 Completed WF/PC-2 7713 (WF/P-2 Cycle 7 Supplemental Darks pt3/3) The WF/PC-2 was used to make supplemental dark calibration images. This dark calibration program obtains three dark frames every day to provide data for monitoring and characterizing the evolution of hot pixels. The observations were completed as planned, and no anomalies were noted. 1.5 Completed WF/PC-2 8090 (POMS Test Proposal: WF-II Parallel Archive Proposal Continuation) The WF/PC-2 was used in the parallel mode to make some low galactic latitude archive observations. The program will be used to take parallel images of random areas of the sky. The observations were executed as scheduled, and no anomalies were noted. 1.6 Completed WF/PC-2 6357 (The Nuclear Morphology of Elliptical Galaxies) The WF/PC-2 was used to make images of the early type, large, elliptical galaxy UGC-5467 (taken from a list of 150 galaxies) in order to study its nuclear morphology. This survey will complement Illingworth's snapshot study of later Hubble types. The observations were completed as scheduled, and no anomalies were reported. 1.7 Completed STIS/CCD 8081 (STIS CCD Hot Pixel Annealing [2- II) The Space Telescope Imaging Spectrograph (CCD) was used to make a dark and a bias calibration observation. The effectiveness of the CCD hot pixel annealing process is assessed by measuring the dark current behavior before and after annealing and by searching for any window contamination effects. The observations were executed as scheduled, and no anomalies were noted. 1.8 Completed WF/PC-2 7475 (The Chemical Content of the Universe at Z< 1.6) The WF/PC-2 was used to make observations of the background quasar Field-Q045. Damped Lyman-Alpha absorption systems provide a means of directly probing the chemical content of the deep universe. A wavelength calibration image was also taken. The observations were completed as planned, and no problems were reported. 1.9 Completed FOC/96 6350 (FOC Spectroscopy of BALQSOs) The Faint Object Camera (f/96) was to be used to make ultraviolet spectrographic images of BALQSO 0113-4040 which is known to show broad emission lines from abundant ions. This observation was lost due to the guide star acquisition failure detailed in 2.1 and HSTAR 6999 when the take data flag remained down. 1.10 Completed WF/PC-2 6435 (A WF/PC-2 Search for Surviving Binary Companions in SN Ia Remnants) The WF/PC-2 was used to make observations of the class Ia super nova remnant Tycho-SNR in order to search for surviving binary companions. The type Ia supernovae {SNe Ia} are widely believed to be explosions of white dwarfs undergoing binary mass accretion. The observations were completed as planned, and no anomalies were reported. 2.0 FLIGHT OPERATIONS SUMMARY 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 4 Successful : 3 Per HSTAR 6999, the acquisition scheduled for 046/12/1231Z failed when the scan step limit was exceeded on FGS-3. The proposal described in 1.9 was affected by this failure. Scheduled Reacquisitions : 10 Successful : 10 2.2 FHST Updates: Scheduled : 18 Successful : 18 2.3 Operations Notes: Using ROP SR-1, the SSR EDAC error counter was cleared twice. A TTR was written when UPDs were no issued due to a software anomaly at the NCC. The gyro-3 drift rate bias trend data shows a step shift in the bias trend since 2/12/99. The rate of change over the last two days is 74.83 arcseconds/hour per day, well above the desired limit of 10.8 arcseconds/hour per day. During the night, battery 5 temperature flagged out of limits at 047/054634. HSTAR 7000 was written. Later, at 047/084805Z, both the battery 2 and the battery 4 voltages temporarily flagged out of limits, due to the solar eclipse encountered this morning. HSTAR 7001 was written. This problem was corrected by disabling and then re-enabling the rate of charge test, as directed by an operations request. 3.0 SIGNIFICANT FORTHCOMING EVENTS: The start of sustained CCS "A" string operations will begin this morning at approximately 047/1448Z. Continuation of normal science observations and calibrations. /DMH