HUBBLE SPACE TELESCOPE DAILY REPORT #893 PERIOD COVERED: 0800 EST Daily Status Report as of 144/1200Z. 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed WFC 4105 (HST Medium - Deep Survey: cycle 1 High Latitude) The Wide Field Camera was used to make one high latitude medium - deep sky survey image taken in parallel with the prime science observations. The observation was received and displayed in the OSS. There was a recentering event which occurred during the exposure, however, the observations was reported to look okay. 1.2 Completed Two Sets of PC 4714 (WF/PC Cycle 2 Calibration: PC Internal Delta Flats) The Planetary Camera was used to make two internal delta flat observations which will be used for the restoration of Earth flat images, which were altered due to changes in quantum efficiency which occurred during WFPC decontamination operations. Both observations were received and displayed. They were reported to look okay. 1.3 Completed FGS 2941 (High Speed Astrometry - A Search for Planetary Companions to Low Mass) The Fine Guidance Sensors were used to make astrometric observations of Barnard's star to determine the presence of a Jupiter size planet in orbit around the target star. The astrometric observations were monitored in the OSS while they had telemetry. No problems were seen. 1.4 Completed FGS 3688 (Diagnostic of Early Stellar Evolution: Search for Pre-Main Sequential Stars) Fine Guidance Sensor #3 was used to make astrometric observations of pre-main sequence star 100628 to see if that star may have a planetary companion. The astrometric observation occurred completely during LOS and could not be monitored. When the telemetry reappeared it was noted that the stop flag was set and the search radius limit had been exceeded for FGS #3. 1.5 Completed FGS 3886 (Orbital Parameter of Known Binary, Sequel) Fine Guidance Sensor transfer scans were used to observe a close binary star UPGREEN69 near the time of its periastron. The astrometric observations were monitored in the OSS, and no problems were seen in the telemetry. 1.6 Completed FOC/96 4804 (UV Imaging of Nearby Galaxies with FOC/96) The Fine Object Camera (f/96) was used to make one ultraviolet observation of nearby galaxy ESO-0430-3. The exposure lasted ten minutes, and used filter F220W. The observation was received via the science tape recorder playback and displayed in the OSS. The image appeared to be normal. 1.7 Uplinked Updated Ephemeris Tables, Per MOSES 2871 1.8 Completed FOS/RD 3858 (The Inner Regions of Quasars: Cycle 2 Continuation) The Faint Object Spectrograph was used to make snapshot images and spectral observations of the active galactic nuclear region around the center of quasar B21555+33. The OSS reported that the observations appeared to have been completely successful. 1.9 Completed Two Sets of WFC 4381 (HST Medium - Deep Survey - Cycle 3) The wide Field Camera was used to make two sets of high latitude medium - deep sky survey (Cycle 2) observations which were taken in parallel with the prime science observations. The observations were executed as scheduled, and no problems were reported. 1.10 Completed Two Sets of FOS/BL 4054 (Probing the Nuclear Regions of Seyfert Galaxy NGC-5548) The Faint Object Spectrograph was used to make two set of ultraviolet spectral observations of the central core region of Seyfert galaxy NGC-5548, to look for time dependent variations in its continuum, and emission line of Helium II and Carbon IV. The observations were monitored in the OSS, and the data quality was assessed. No problems were reported. 1.11 Completed PC 3603 (Snapshot of Protoplanetary Nebulae) The Planetary Camera was used to make snapshot images of the protoplanetary nebula PK058-10D1 which is thought to be in the process of formation. The intent is to study its current morphology. The observations were executed as scheduled, and monitored in the OSS. No problems were reported, except that the core of the target image was saturated. 1.12 Completed PC/WFC 4109 (WF/PC Cycle 2 Calibration: Rapid Internal Monitor) Internal flat observations were made using both the Planetary Camera and the wide Field Camera to revile possible changes in contamination and the possible return of quantum efficiency hysteresis. The OSS monitored to observations and assessed the data quality. The observations were reported to look okay. 1.13 Completed GHRS/2 3463 (Highly Ionized Nitrogen in galactic Halo) The High Resolution Spectrograph was used to make ultraviolet spectral observations of the active galactic nuclear regions in Markarian galaxy MARK509 to look for absorption line of Nitrogen IV. The return to brightest option was specified. The target search flux was 3321. The confirmation showed the target well centered. A recentering event was reported to have occurred during one of the spectral observations. The OSS reported that the science observations looked good. 1.14 Completed HSP/POL 4888(Remnant Stars in Supernova Remnants AUG - Cycle 3 High) The High Speed Photometer was used to make observations of the supernova remnant SS443 which is known to have emission lines which vary in velocity by relativistic amounts in a 162 day period. The principal investigator was present to monitor the observations. Most of the observations were monitored in real-time. There were no problems. 1.15 Completed FOC/96 3591 (Massive Stars in Star Bursting Galaxies - FOC Images (Part 1)) The Faint Object Camera was used to make observations of the star bursting regions of galaxy NGC-4670. The OSS conducted routine monitoring and assessed the data quality. No problems were seen. 1.16 Completed FOC/96 4800 (The Stellar Content of Wolf-Rayet Galaxies (FOC Images)) The Faint Object Camera (f/96) was used to make ultraviolet images of Wolf - Rayet galaxy NGC-3049. This star bursting galaxy exhibits broad Helium II emission lines from stellar sources. The main goal is to determine why this galaxy produces such a large number of Wolf - Rayet stars. The observations were executed as scheduled and no problems were reported. 1.17 Completed WFC 4713 (WF/PC Cycle 2 Calibration: WFC Internal Delta Flats) The Wide Field Camera was used to make a series of internal delta flat observations to look for new forms of contamination. The observations were executed as planned, and no problems were seen. 1.18 Completed FOS/BL 4793 (The Extended Featureless Continuum Source in Cygnus A - Cycle 2 Spertr.) The Faint Object Spectrograph was used to make spectral observations of the Cygnus A. It is known to have an extended, unpolarized continuum emission from the nucleus. The strength of the Carbon IV lines were to have been measured. The binary search for the offset star was received and displayed. It failed, producing a status buffer error message indicating "target not found". The maximum counts were much below the faint limit. Although it was fainter than expected the offset star appeared to be well centered., A pointing correction was not attempted. There was a guide star recentering event during the observations. Subsequent spectral observations showed counts of around five counts and twelve. These observations were also reported to have had recentering events occur during the observations. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 18 Successful : 18 Scheduled Reacquisitions : 22 Successful : 22 Losses of Lock : 0 2.2 FHST Updates: Scheduled : 36 Successful : 36 2.3 Significant HSTARs: None 2.4 Operations Note: FGS "Breathing" Test -------------------- A test using all three FGSs is currently under way (Monday, May 24). This test will take repeated astrometry observations using a small set of stars to investigate scale changes ("breathing") in the spacecraft structure. 3.0 ACTIVITIES SCHEDULED FOR NEXT REPORTING PERIOD: 3.1 Complete GHRS/2 4792 (Hydrogen Lyman Alpha Day Glow Emission Line Profiles from Outer Planets) 3.2 Complete WFC 4929 (WF/PC Cycle 2: Improved Dark Calibration) 3.3 Complete FGS 2941 (High Speed Astrometry - A Search for Planetary Companions to Low Mass) 3.4 Complete PC 3603 (Snapshots of Protoplanetary Nebulae) 3.5 Complete FOC/96 5009 (ST Focus Investigation) 3.6 Complete FGS 5011 (Astrometry for ST Focus Investigation) 3.7 Complete FOS/BL 4054 (Probing the Nuclear Regions of Seyfert Galaxy NGC-5548) 3.8 Complete WFC 4381 (HST Medium - Deep Survey - Cycle 3) 4.0 ANOMALY STATUS: 4.1 Significant New Anomalies: None 4.2 Significant Unresolved Anomalies: None 5.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH -END-