HUBBLE SPACE TELESCOPE DAILY REPORT #1987 PERIOD COVERED: 0000Z (UTC) 10/20/97 - 0000Z (UTC) 10/21/97 Daily Status Report as of 294/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed Two Sets of WF/PC-2 7621 (WF/PC-2 Cycle 7 Supplemental Darks PT1/3) The WF/PC-2 was used to make supplemental dark calibration images. This set of calibrations is intended to obtain three dark frames every day to provide data for monitoring and characterizing the evolution of hot pixels. The observations were executed as scheduled, and no anomalies were noted. 1.2 Completed STIS/CCD 7802 (Daily Darks to Update Acquisition Bad Pixel Table) The Space Telescope Imaging Spectrograph (CCD) was used to make calibration observations to obtain daily darks to update the acquisition bad pixel table. These daily darks are intended to identify hot pixels for update to the acquisition on-board FSW hot pixel table. Daily hot pixel lists can also be used for science data analysis. The observations were executed as scheduled, and no anomalies were noted. 1.3 Completed Two Sets of NIC/2 7420 (A Near-Infrared Search for Very Low Mass Companions to Stars Within 10 Parsecs of the Sun) The Near Infrared Camera (Camera Two) was used to make searching observations for very low mass companions to variable stars HD10476 and HD20794. These stars are known to be within 10 parsecs of the Sun. The observations were executed as scheduled, and no anomalies were noted. 1.4 Completed STIS/CCD 7711 (STIS CCD G750L fringing flats.) The Space Telescope Imaging Spectrograph (CCD) was used to investigate and monitor the STIS CCD flat-field fringing in the G750L grating at it's nominal wavelength setting {7751A}. WAVECALs were also taken at the same gain and wavelength setting (typical S/N = 100 for each integration, and GAIN=4 on each). The observations were executed as scheduled, and no anomalies were noted. 1.5 Completed Five Sets of WF/PC-2 7620 (WF/PC-2 Cycle 7 Standard Darks) The WF/PC-2 was used to make a series of Cycle 7 standard dark calibration images. This dark calibration program obtains dark frames every week in order to provide data for the ongoing calibration of the CCD dark current rate, and to monitor and characterize the evolution of hot pixels. The observations were executed as scheduled, and no anomalies were noted. 1.6 Completed Two Sets of STIS/CCD/MA1 7432 (Morphological and Spectral Evolution of Galaxies) The Space Telescope Imaging Spectrograph (CCD and MA1) were used to make observations to study the morphological and spectral evolution of the galaxies 3C346 and 3C381. A library of ultraviolet images of normal galaxies at low redshifts is essential to our understanding of the properties and evolution of the high redshift universe. The observations were completed as planned, and no problems were reported. 1.7 Completed Two Sets of NIC/1/2/3 7729 (NICMOS Short One Orbit Parallel) The Near Infrared Camera (Cameras One, Two, and Three) was used to obtain "JHK" imaging of sky regions while another instrument was prime. These observations were part of the short NICMOS one-orbit parallel program. The observations were executed as scheduled, and no anomalies were noted. 1.8 Completed Nine Sets of NIC/1/2/3 7789 (MULTIACCUM Dark Characterization of Pedestal) The Near Infrared Camera (Cameras One, Two, and Three) was used to take a series of dark images to characterize the pedestal problem fix which was installed in NICMOS flight software version 4.08. The observations were completed as planned with no reported anomalies. 1.9 Completed Four Sets of STIS/MA2 7604 (Cycle 7 MAMA Dark Measurements) The Space Telescope Imaging Spectrograph (MA2) was used to make MAMA dark measurements. These darks will be used in later image reductions and also trended over the instrument's life time as an indicator of the detector's degradation or damage. The observations were completed as scheduled, and no problems were reported. 1.10 Completed NIC/1/2/3 7726 (NICMOS One Orbit Parallel) The Near Infrared Camera (Cameras One, Two and Three) was used to make a one orbit parallel calibration observations. The observations were executed as scheduled, and no anomalies were noted. 1.11 Completed Three Sets of NIC/1/2 7443 (Mineralogic Mapping of Asteroid 4 Vesta) The Near Infrared Camera (Cameras One and Two) was used to make mineralogic mapping of asteroid 4 Vesta. The 1997 opposition of asteroid 4 Vesta offers an important opportunity to map its diverse mineralogy with uniquely high contrast and to investigate more thoroughly the newly discovered major topographic feature at the south pole. The observations were completed as planned, and no anomalies were reported. 1.12 Completed Two Sets of WF/PC-2/NIC/3 7382 (The Star-Formation History of the Large Magellanic Cloud) The WF/PC-2 and the Near Infrared Camera (Camera Three) were used to make observations of the disk of the Large Magellanic Cloud (LMC). These data will enable us to quantitativly study the intermediate to low-mass stellar populations and the star-formation history of the LMC. The observations were executed as scheduled, and no anomalies were noted. 1.13 Completed Two Sets of STIS/CCD 7782 (STIS Non-Scripted Parallel Archive Proposal - Half Orbit) The Space Telescope Imaging Spectrograph (CCD) was used for a non-scripted parallel archive proposal (one-half orbit). The observations were executed as scheduled, and no anomalies were noted. 1.14 Completed Two Sets of STIS/CCD 7783 (STIS Parallel Science) The Space Telescope Imaging Spectrograph (CCD) was used to make observations taken in parallel with the prime science. The observations were completed, and no problems were reported. 1.15 Completed WF/PC-2 6559 (An Imaging Study of Asteroids) The WF/PC-2 was used to make multi-color observations of the main belt asteroid 11-Parthen. This asteroid reached perigee during Cycle 6. The images will be searched for companions. The observations were executed as scheduled, and no anomalies were noted. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 7 Successful : 7 One acquisition defaulted to fine lock on FGS-3 only at 294/0020335 when the scan steps limit was exceeded. The following five reacquisitons also resulted in single FGS guidance. HSTAR 6307 was written. The effect on science proposals will be included in tomorrow's report. Scheduled Reacquisitions : 6 Successful : 6 2.2 FHST Updates: Scheduled : 14 Successful : 14 2.3 Operations Notes: Contrary to yesterday's report, the STIS MAMA2 reset that occurred, and was corrected, during the weekend had no effect on the STIS science proposal 7783. Each of the iterations of this proposal used the CCDs rather than the MAMA2. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Continuation of normal science observations and calibrations. /DMH