HUBBLE SPACE TELESCOPE DAILY REPORT #1192 PERIOD COVERED: 0000Z Daily Status Report as of 213/1200Z. 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed Three Sets of WF/PC-2 5479 (Subarcsecond Structure in Nearby AGNs) The WF/PC-2 was used to make snapshot observations of the nearby active galactic nuclei of MARK1400, MARK1308, and MARK577. The observations were executed as scheduled, and no anomalies were noted. 1.2 Completed FGS 5336 (Linking the HIPPARCOS to the Extragalactic Reference Frame: NEWHIP-B) The Fine Guidance Sensor #3 was used to make two sets of astrometric observations of object NEWEGOB-38, 1820_REF,1821-REF, and 1822-REF. The observations were executed as scheduled. No anomalies were reported. 1.3 Completed WF/PC-2 5370 (HST Medium-Deep Survey: Cycle 4 High, High Galactic Latitude) The WF/PC-2 was used in parallel with the prime science observations to make high galactic latitude observations as part of a medium-deep sky survey. This observations was taken under single star guidance. There may have been some motion around a point centered on the guide star in FGS#2. Also, the HST underwent two guide star recenterings for a total of seven seconds. 1.4 Completed WF/PC-2 5464 (A Study of the AGB in Local Bulge Populations) The WF/PC-2 was used to make observations of the stellar bulge in galaxy NGC-224-G1 to make a survey of its stellar population. The observations were completed as expected, and no problems were reported. 1.5 Completed Two Sets of WF/PC-2 5655 (WF/PC-2 Cycle 4 Calibration: Internal Monitor. 2: Flats Part 2) The WF/PC-2 was used to make visual flats calibration images. The observations were completed as planned, and no problems were reported. 1.6 Completed WF/PC-2 5450 (Host Galaxies and Cluster Environments of Quasars) The WF/PC-2 was used to make observations of Quasar Q1218+1734 to study the properties of its host galaxy and surrounding environment. The observations were executed as scheduled, and no anomalies were noted. 1.7 Complete WF/PC-2 5642 (Observations of the Impact of Comet Shoemaker-Levy (1993E) and Jupiter) The WF/PC-2 made observations to support the Jupiter/ Shoemaker-Levy event. During one of the observations there was a tape recorder track change while the observations was being written to tape. As a result one picture was lost. No other anomalies were reported on the other observations. 1.8 Completed WF/PC-2 5560 (WF/PC-2 Cycle 4 Calibration: Internal Monitor. 1) The WF/PC-2 was used to make several internal bias, K-Spot, and flat calibration observations to monitor the CCD camera electronics, the optical alignment, and to check for contamination. The observations bwere completed as planned, and no anomalies were noted. 1.9 Completed FOS/RD 5385 (Detecting the Hydroxyl Radical in the Jovian Magnetosphere) The Faint Object Spectrograph (Red Side) was used to obtain image mode data of Jupiter's magnetosphere near its moon Europa. The observations were executed as scheduled, and no anomalies were noted. 1.10 Complete WF/PC-2 (WF/PC-2 Cycle 4 Calibration: Internal Flats) The WF/PC-2 was used to make flat field exposures using the VIS lamp and the internal source. The observations were executed as scheduled, and no anomalies were noted. 1.11 Completed Two Sets of WF/PC-2 5446 (The Nuclei of Nearby S0 and Spiral Galaxies: A PC Snapshot Imaging) The WF/PC-2 was used to make observations of of the core region of galaxy IC3021 to provide statistics on the presence of nuclear cusps, stellar condensations, and inner stellar disks and dust lanes. The observations were executed as scheduled, and no anomalies were noted. 1.12 Completed WF/PC-2 5237 (Stellar Populations in Local Group Galaxies (WC13): Cycle 4) The WF/PC-2 was used to make observations of galaxy M-33-Field-N (which is in the local group). The observations were completed as planned, and no problems were reported. 1.13 Completed FOS/RD 5451 (The Absorption Cross-sections of Nearby Galaxies) The Faint Object Spectrograph (Red Side) was used to observe light from quasi-stellar object 0026+129, which acts as a probe as it passes through the outer reaches of a nearby galaxy. The observations were executed as scheduled, and no anomalies were noted. 1.14 Completed WF/PC-2 5494 (Stellar Winds of Massive Stars in Nearby Galaxies) The WF/PC-2 was used to make far ultraviolet spectral observations of one bright star in galaxy M-33 to learn more about the stellar wind, mass loss rate, and abundances of the target star. The observations were executed as scheduled, and no anomalies were noted. 1.15 Completed WF/PC-2 5479 (Subarcsecond Structures of Nearby AGNs) The WF/PC-2 was used to make snapshot observations of the active galactic nuclei of galaxy MARK-1308 to study the interactions between the central engine, the stars, and the interstellar matter in the AGN. The observations were executed as scheduled, and no anomalies were noted. 1.16 Completed WF/PC-2 5427 (Calibration of Nearby Galaxy Type IA Supernovae as Standard Candles) The WF/PC-2 was used to make observations of nearby galaxy NGC-4536-FI as part of an effort to find Cepheids in this galaxy which has produced a Type I supernovae. The observations were executed as scheduled, and no anomalies were noted. 1.17 Completed FOS/BL 5530 (FOS Location of Spectra and Aperture) The Faint Object Spectrograph (Blue Side) was used to make Y-base maps of the FOS detectors using internal lamps. The purpose is to determine the location of the spectra on the diodes. The observations were monitored, and no anomalies were reported. 1.18 WF/PC-2 5429 (Imaging Polarimetry of Extended UV Emission in Radio Galaxies: Cycle 4) The WF/PC-2 was used to make extended ultraviolet observations of the high redshift radio galaxy 3C368 with the polarizer. The observations were executed as scheduled, and no anomalies were noted. 1.19 Completed WF/PC-2 5570 (WF/PC-2 Cycle 4 Calibration: Earth Flats, Large Set) The WF/PC-2 was used to make a set of Earth flat calibration images using different filters in order to construct high quality flat fields of the OTA illumination pattern. The observations were completed as planned, and no anomalies were noted. 1.20 Completed FOS/RD 5455 (The Level of Ionization and Chemical Composition of QSO BAL Region Gas) The Faint Object Spectrograph (Red Side) was used to make ultraviolet observations of quasi-stellar object (QSO) Q0226-1024 which is known to have broad absorption lines (BALs). The observations were executed as scheduled, and no anomalies were noted. 1.21 Completed WF/PC-2 5205 (Disk Around Main Sequence Stars) The WF/PC-2 was used to make observations of star Vega (aka, HD172167), which was found to have an infrared excess by IRAS, to try and detect a circumstellar disk. The observations were completed as planned, and no problems were reported. 1.22 Completed Two Sets of GHRS/2 5671 (GHRS Dark Noise Monitor: Cycle 4) The High Resolution spectrograph (Side Two) was used to make dark Calibrations images. These were strictly internal tests for routine monitoring of detector dark noise. The observations were executed as scheduled, and no anomalies were noted. 1.23 Completed WF/PC-2 5395 (High Spatial Resolution Imaging of the Pre-Main Sequence Binary Stars) The WF/PC-2 was used to make ultraviolet observations of pre-main sequence binary star V410TAU. The observations were executed as scheduled, and no anomalies were noted. 1.24 Completed WF/PC-2 5476 (Continuum Snapshots of 3CR Radio Galaxies) The WF/PC-2 was used to make snapshot images of radio galaxy 3C44.0 as part of a continuum survey and to study the galaxy's morphology. The observations were completed as planned, and no problems were reported. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 21 Successful : 21 Scheduled Reacquisitions : 23 Successful : 23 2.2 FHST Updates: Scheduled :41 Successful :41 2.3 Significant HSTARs: None 2.4 Operations Notes: No anomalies were reported on the spacecraft sub-systems during the weekend. 3.0 ANOMALY STATUS: 3.1 Significant New Anomalies: None 3.2 Significant Unresolved Anomalies: None 4.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH -END-