HUBBLE SPACE TELESCOPE DAILY REPORT #2026 PERIOD COVERED: 0000Z (UTC) 12/17/97 - 0000Z (UTC) 12/18/97 Daily Status Report as of 352/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 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 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. 1.2 Completed Two Sets of WF/PC-2 7612 (Infrared Imaging of 3CR Radio Galaxies) The WF/PC-2 was used to make infrared observations of the radio galaxy 3C342 to look for an infrared image counterpart to the radio image. A dark calibration image was also taken. The observations were executed as scheduled, and no anomalies were noted. 1.3 Completed STIS/CCD 7462 (Velocity Structure in High Redshift Galaxies) The Space Telescope Imaging Spectrograph (CCD) was used to make observations of the high redshift galaxy E-0050-275 in order to study its velocity structure and to make imaging spectrographic observations of its recently-discovered optical Einstein ring. A wavelength calibration observations was also taken. The observations were executed as scheduled, and no anomalies were noted. 1.4 Completed WF/PC-2 6609 (The WF/PC-2 B-Band Parallel Survey: A Systematic and Synoptic Study ) The WF/PC-2 was used to make B-Band survey observations in parallel with the prime science observations. A total of 216 exposures will be taken over a period of time to make a statistical study of the formation and evolution of the galaxies. The observations were executed as scheduled, and no anomalies were noted. 1.5 Completed FGS 6875 (Parallax of Delta Cephei) The Fine Guidance Sensors were used to make astrometric observations of the Cephied class variable star Delta Cephei. Delta Cephei is a classical Cepheid variable, whose trignometric parallax is presently known to around 30%. HST observation shave the potential to reduce this uncertainty to 15%. The observations were completed as planned, and no anomalies were reported. 1.6 Completed Three Sets of WF/PC-2 7786 (Pure Parallel Archive Survey - Continuation) The WF/PC-2 was used to make observations as part of an archival survey program in which the images were taken in parallel with the prime science observations. These WF/PC-2 parallel observations were obtained in the ultraviolet in a search for interesting objects. The observations were completed as planned, and no problems were reported. 1.7 Completed STIS/CCD 7781 (STIS Non-Scripted Parallel Archive Proposal - Full Orbit) The Space Telescope Imaging Spectrograph (CCD) was used for a non-scripted parallel archive proposal (one full orbit). The observations were executed as scheduled, and no anomalies were noted. 1.8 Completed NIC/1 7344 (Witnessing the Birth of Radio Galaxies: WF/PC-2 & NICMOS Observations of CSOs) The Near Infrared Camera (Camera One) was used to make observational images of the cores of bright, nearby galaxy (Compact Symmetric Objects) CSO 4C31.4 in order to try to witness the birth of a radio galaxy. Only HST can image these galaxies at the same size scale of the CSO itself, also allowing us to search for nuclear structures aligned with the radio source in this formative stage. The observations were completed as planned, and no anomalies were reported. 1.9 Completed 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. 1.10 Completed 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. 1.11 Completed WF/PC-2/STIS/CCD/NIC/1/2 7307 (The Formation and Evolution of Rich Star Clusters in the LMC) The WF/PC-2, the Space Telescope Imaging Spectrograph (CCD), and the Near Infrared Camera (Cameras One and Two) were used to make observations of the rich star cluster NGC-1831 which is located within the Large Magellanic Cloud in order to study its formation and evolution. These observations will help us understand the origin and evolution of rich star clusters in our own Galaxy. The observations were complete as scheduled, and no anomalies were reported. 1.12 Completed NIC/1/2/3 7608 (NICMOS Focus Monitoring) The Near Infrared Camera (Cameras One, Two, and Three) was used to determine and monitor the optimal focus and tilt settings for all three NICMOS cameras. This proposal is built to run NIC1/2/3 sweeps on a 2-week basis. The observations completed without incident with no reported anomalies. 1.13 Completed NIC/2 7331 (Near-IR Properties of the Bulges of Spiral Galaxies) The Near Infrared Camera (Camera Two) was used to make infrared observations of the bulge in spiral galaxy NGC-7421. Near-IR data at HST resolution are essential for correcting for the effect of dust and will enable us to derive robust nuclear properties for the sample. The observations were executed as scheduled, and no anomalies were noted. 1.14 Completed NIC/2/3 7453 (The SBF Hubble Diagram) The Near Infrared Camera (Cameras Two and Three) was used to make deep NICMOS observations of galactic cluster Abell-2199 to determine its distance using the surface brightness fluctuation {SBF} method. HST is essential for its high spatial resolution which makes it possible to detect and remove globular clusters and background galaxies that contaminate the SBF measurement. The observations were executed as scheduled, and no anomalies were noted. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 10 Successful : 10 Scheduled Reacquisitions : 6 Successful : 6 2.2 FHST Updates: Scheduled : 23 Successful : 23 2.3 Operations Notes: There were no reported operational problems. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Continuation of normal science observations and calibrations. /DMH