HUBBLE SPACE TELESCOPE DAILY REPORT #1671 PERIOD COVERED: 0000Z (UTC) 07/09/96 - 0000Z (UTC) 07/10/96 Daily Status Report as of 192/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed WF/PC-2 6359 (Core Properties of the Bulges of Spiral = Galaxies) The WF/PC-2 was used to make snapshot survey observations of = spiral galaxy ESO498G5 in order to study its central bulge. The aim is to = investigate the core properties, correlation's with global galactic = properties, and the frequency of occurrence of multiple and/or = miscentered nuclei. The observations were completed as scheduled, and no = anomalies were noted. 1.2 Completed FOC/96 6580 (Hot Stars and Young Super Star Clusters in = the Wolf-Rayet Starbursting Galaxy) The Faint Object Camera (F/96) was used to make intensive study = of the hot stars and the super star bursting knots (aka, super star = clusters) which are located in the starbursting regions of the Wolf-Rayet = galaxy He2-10. A Wolf-Rayet galaxy is a starburst galaxy which is just = past the onset of the star formation burst, in which a large number of = the most massive stars have evolved to the Wolf-Rayet stage. The = observations were executed as scheduled, and no anomalies were noted. 1.3 Completed Three sets of WF/PC-2 5971 (HST Medium Deep Survey) The WF/PC-2 was used to make a long exposure medium deep sky = survey observations at latitudes larger than 10 degrees taken in parallel = with the prime science observations. The observations were executed as = scheduled, and no anomalies were noted. 1.4 completed GHRS/2 6620 (Density Diagnostics for the Dynamic = Atmospheres of LPV Stars) The High Resolution Spectrograph (Side Two) was used to make = observations of LPV (Long Period Variable) Mira class star HD117287 in = order to study its density dynamics and other atmospheric properties. = These data will be compared with similar GHRS spectra obtained for = semi-regular variable stars. The observations were completed as planned, = and no problems were reported. 1.5 Completed Two sets of WF/PC-2 6253 (Pure Parallel Archive Program) The WF/PC-2 was used to execute a pure parallel program taking = ultraviolet observations running concurrently with prime science = observations. The intent is to search for extra-galactic sources with = flux excesses at 3000 A0 and galactic sources with excesses at 1600 A0. = The observations were completed as planned, and no problems were = reported. 1.6 Completed WF/PC-2 6365 (A Snapshot survey For Companions and = Clusters around Wolf-Rayet Stars) The WF/PC-2 was used to make snapshot observations of Wolf-Rayet = star WR27 in order to look for companion stars and clusters. Photometry = was performed on the Wolf-Rayet star and associated stars. The = observations were completed as planned, and no anomalies were reported. 1.7 Completed COSTAR/U 6895 (FOC Cycle 6 PSF Monitoring) The Faint Object Camera/Costar were used to make observations of = object 01-001 (aka, white dwarf star BPM16274) in order to check out the = Point Spread Function (PSF) and focus of the system. The observations = were executed as scheduled, and no problems were reported. 1.8 Completed WF/PC-2 6188 (WF/PC-2 Cycle 5 Calibration: Dark) The WF/PC-2 was used to make internal dark calibration images. The = observations were completed as scheduled, and no problems were reported. 1.9 Completed WF/PC-2 6346 (Snapshot Survey of the Ultraluminous IRAS = Galaxy Sample-Part 1 High) The WF/PC-2 was used to make snapshot survey observations of the = ultraluminous IRAS galaxy IR20087-03. These data will be searched for = multiple cores, which imply a merger has occurred, and for starburst = regions. The observations were executed as scheduled, and no anomalies = were noted. 1.10 Completed WF/PC-2 6250 (WF/PC-2 Cycle 5 Calibration: Internal = Monitor) The WF/PC-2 was used to make a series on internal calibration = observations. Internal flats, biases, and K-Spot calibration images were = taken. These observations are designed to monitor the health of the = cameras. The observations were executed as scheduled, and no anomalies = were noted. 1.11 Completed GHRS/2 6748 (Abundances of Very Heavy Elements in the = Early Galaxy III) The High Resolution Spectrograph (Side Two) was used to make = observations of the very old, metal poor, halo star HD115444. From these = spectra, the abundances of irridium, lead, platinum, and osmium will be = determined. These elements are synthesized in stellar interiors by either = rapid or slow neutron capture processes. The observations were completed = as planned, and no problems were reported. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 7 Successful : 7 Scheduled Reacquisitions : 9 Successful : 9 2.2 FHST Updates: Scheduled : 9 Successful : 9 2.3 Operations Notes: No anomalies to report, normal operations 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH