HUBBLE SPACE TELESCOPE DAILY REPORT #2448 PERIOD COVERED: 0000Z (UTC) 08/31/99 - 0000Z (UTC) 09/01/99 Daily Status Report as of 244/0000Z 1.0 OBSERVATIONS SCHEDULED AND ACCOMPLISHED: 1.1 Completed WF/PC-2 8443 (WF/PC-2 Cycle-8 Supplemental Darks pt1/3) The WF/PC-2 was used to obtain three dark frames every day to provide data for monitoring and characterizing the evolution of hot pixels. The observations were completed as planned, and no problems were reported. 1.2 Completed Three Sets of WF/PC-2 8090 (POMS Test Proposal: WF-II Parallel Archive Proposal Continuation) The WF/PC-2 was used in the parallel mode to make some low galactic latitude archive observations. The program will be used to take parallel images of random areas of the sky. The observations were executed as scheduled, and no anomalies were noted. 1.3 Completed STIS/CCD 8271 (A Snapshot Survey of LMC Planetary Nebulae: A Study of Nebular and Late Stellar Evolution) The Space Telescope Imaging Spectrograph (CCD) was used to make medium-resolution slitless spectroscopy snapshot images of the planetary nebula LMC-SMP-65 located in the Large Magellanic Cloud to study the parallel evolution of the nebulae and their central stars. The observations were completed as planned, and no problems were reported. 1.4 Completed WF/PC-2 8243 (SINS: The Supernova Intensive Study - Cycle 8) The WF/PC-2 was used to make observations of supernova LMC-SN1987. Supernovae reveal the last stages of stellar evolution, create the chemical history of the Universe, energize the interstellar gas, and occupy the center of attention for the extragalactic distance scale and cosmology. A wavelength calibration image was also taken. The observations were completed as planned, and no problems were reported. 1.5 Completed Two Sets of STIS/CCD 8202 (Bright Quasar Close Lensing Search) The Space Telescope Imaging Spectrograph (CCD) was used to make observations of HCLQ2252-5 and HCLQ1350-2 as part of a second generation survey to search for bright lensing quasars. With the restored PSF, new images will be considerably more sensitive to the presence of both close separation and faint lens components, and because STIS reaches two magnitudes fainter the PC, the new snapshot images will have much greater dynamic range. The observations were executed as scheduled, and no anomalies were noted. 1.6 Completed STIS/CCD 8408 (STIS CCD Dark Monitor C8) The Space Telescope Imaging Spectrograph (CCD) was used to make a CCD bias calibration observation. This is to monitor the darks for the STIS CCD. The observations were executed as scheduled, and no anomalies were reported. 1.7 Completed WF/PC-2 6631 (Imaging a Cluster of Galaxies at Redshift 2.38) The WF/PC-2 was used to make observations of the galactic cluster Gal-Clus-2073 which is located at a distance of z = 2.38. This is a sub-set of about four galaxies within the cluster that forms a very compact {< 100 kpc} galaxy group and may be merging to form a giant elliptical galaxy. The observations were executed as scheduled, and no anomalies were noted. 1.8 Completed STIS/CCD 8409 (STIS CCD Bias Monitor C8) The Space Telescope Imaging Spectrograph (CCD) was used to make a CCD bias calibration observation. This is to monitor the bias in the 1x1, 1x2, 2x1, and 2x2 bin settings at gain=1, and 1x1 at gain = 4, to build up high-S/N superbiases and to track the evolution of hot columns. The observations were executed as scheduled, and no anomalies were reported. 1.9 Completed Two Sets of STIS/CCD 8406 (POMS Test Proposal: STIS Non-Scripted Parallel Proposal Continuation V) The Space Telescope Imaging Spectrograph (CCD) was used to make high galactic latitude observations taken in parallel with the prime science observations as part of a POMS proposal. This is a STIS non-scripted parallel Condition V proposal. The observations were completed as scheduled, and no anomalies were reported. 1.10 Completed WF/PC-2 7469 (Internal Velocity Distribution in Globular Clusters) The WF/PC-2 was used to make observations of the globular cluster NGC-7078 in order to study the internal velocity distribution in its cores and as a function of distance from the cluster center, and thus also infer its mass distribution. The observations were executed as scheduled, and no anomalies were noted. 1.11 Completed WF/PC-2 8457 (UV Earthflats) The WF/PC-2 was used to make a ultraviolet Earth flat calibration image. This is to improve the quality of pipeline the ultraviolet flatfields. The observations were completed as scheduled, and no problems were reported. 1.12 Completed FGS 8335 (Calibrating Stellar Models with the Pleiades: Resolving the Distance Discrepancy) The Fine Guidance Sensors were used to make astrometric observations of the star H320 that is located in the Pleiades cluster. This is the first phase of a multi-year effort to measure true masses for low-mass dwarfs in the Pleiades and to determine an accurate distance to this fundamental cluster. The observations were completed as scheduled, and no anomalies were noted. 1.13 Completed STIS/CCD/MA1 7758 (Physics of Diffuse Clouds in the Local Bubble , Part I : The CMa Tunnel) The Space Telescope Imaging Spectrograph (CCD and MA1) was used to make observations of star HD44743 to study the physical conditions in diffuse clouds in the Local Bubble environment and their interfaces with the hot gas filling the bubble. The local interstellar medium presents a favorable situation to check the general ISM theories. A wavelength calibration image was also taken. The observations were completed as planned, and no anomalies were reported. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions: 6 Successful: 6 Scheduled Re-acquisitions: 11 Successful: 11 2.2 FHST Updates: Scheduled: 15 Successful: 15 2.3 Operations Notes: The SSR EDAC error counter was cleared five times per ROP SR-1. The ephemeris tables were loaded, dumped and compared as directed by ROP DF-7 at 243/1422Z. A TTR was written for a 15-minute, 34-second loss of unrecoverable 32k engineering data, from 244/065100Z until 244/070634Z, when the event was not scheduled at the NCC. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Continuation of normal science observations and calibrations. /DMH