HUBBLE SPACE TELESCOPE DAILY REPORT #1533 PERIOD COVERED: 0000Z (UTC) 12/08/95 - 0000Z (UTC) 12/11/95 Daily Status Report as of 345/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed WF/PC-2 6277 (Stellar Populations in the Magellanic = Clouds) The WF/PC-2 was used to make observations of the Magellanic Cloud = globular cluster NGC-1818 to study its stellar populations. This will = study the mass function within the globular cluster. The observations = were completed as planned, and no anomalies were noted. 1.2 Completed FGS 6040 (Ultra-High Angular Resolution of O3 Stars in = the Carina Nebula) The FGSs were used in the TRANS Mode to make ultra-high resolution = astrometric observations of the O3 class star LMC-053705 which is located = in the Large Magellanic Cloud. This is to determine if this object is a = single star or a multiple star system. The observations were completed as = scheduled, and no anomalies were reported. 1.3 Completed 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. 1.4 Completed GHRS/1 6070 (Interstellar Tin: Probing Galactic S-Process = Element Enrichment) The High Resolution Spectrograph (Side One) was used to make = Echelle A observations of star HD24398 in order to probe for interstellar = tin and to study the galactic S-process neutron capture of element = enrichment. The observations were completed as planned, and no problems = were reported. 1.5 Completed Two Sets of WF/PC-2 5972 (Determination of the = Extragalactic Distance Scale) The WF/PC-2 was used to make observations of the galaxies NGC-3198 = and NGC-2541 looking for standard candle Cepheid variable stars. The = purpose of these observations is to help estimate the Hubble constant with = an accuracy of 10%. The observations were executed as scheduled, and no = anomalies were noted. 1.6 Completed FOS/BL 6166 (FOS Cycle 5: Location of Spectra and = Wavelength Calibration) The Faint Object Spectrograph (Blue Side) was used to make = wavelength calibration images to measure the stability of the FOS blue = side wavelength scale and spectral locations. A Taled calibration = observations was also taken. The observations were completed as planned, = and no anomalies were reported. 1.7 Completed WF/PC-2 5904 (Primordial Mass Segregation and Main = Sequence Age Spreads in Young LMC Stars) The WF/PC-2 was used to make observations of young cluster NGC-2157 = which is located in the Large Magellanic Cloud in order to study the = primordial mass segregation and the main sequence age spread of its young = stars. The observations were executed as scheduled, and no anomalies were = noted. 1.8 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. 1.9 Completed GHRS/1 5945 (Diffuse Helium Absorption as a Probe of = Quasar History) The High Resolution Spectrograph (Side One) was used to make = observations of diffuse helium absorption lines in the spectra of quasar = Q0302-0019 to confirm the detection of intergalactic helium by the FOC. = The observations were completed as planned and no anomalies were reported. 1.10 Completed WF/PC-2 6187 (WF/PC-2 Cycle 5 Calibration: Earth Flat) The WF/PC-2 was used to make Earth streak flat calibration images. = These streak flats will be used to produce flat fields, to map the OTA = illumination pattern and, in combination with other data, to produce new = superflats. The observations were completed as planned, and no problems = were reported. 1.11 Completed WF/PC-2 5476 (Continuum Snapshots of 3CR Radio = Galaxies) The WF/PC-2 was used to make snapshot images of radio galaxy 3C99.0 = as part of a continuum survey and to study the galaxy's morphology. The = observations were executed as scheduled, and no anomalies were noted. 1.12 Completed FOS/RD 6059 (Imaging Low-Mass Companions of Nearby = Stars) The Faint Object Spectrograph (Red Side) was used to make = observations of low-mass nearby star GL1245AC to search for possible faint = companions. The bright star was placed behind an occulting bar. The = observations were executed as scheduled, and no anomalies were noted. 1.13 Completed WF/PC-2 5999 (The Nuclear Structure of S0 Galaxies: A PC = Imaging Survey) The WF/PC-2 was used to make observations of S0 class galaxies = NGC-1375, ESO118-034 and NGC-6703 in order to study their nuclear = structure. This is a part of a large survey of S0, E/S0, and S0/a class = galaxies. The targets will cover a wide range in luminosity and = environment. The observations were completed as planned, and no anomalies = were noted. 1.14 Completed FOS/BL 5851 (Post Asymptotic Giant Branch Evolution in = the Magellanic Clouds) The Faint Object Spectrograph (Blue Side) was used to make = ultraviolet observations of the planetary nebula LMC-SMP101 which is = located in the Large Magellanic Cloud. Extensive ground-based and HST = observations and imaging work has already been done on this object. The = observations were completed as planned, and no problems were reported. 1.15 Completed WF/PC-2 5916 (The Oldest Globular Clusters in the Large = Magellanic Cloud) The WF/PC-2 was used to make observations of the metal-poor = globular cluster NGC-1898 which is known to be the one of the two oldest = globular clusters located in the Large Magellanic Cloud. The observations = were completed as planned, and no anomalies were reported. 1.16 Completed GHRS/2 5887 (The Depletion Behavior of Chromium Relative = to Zinc ) The High Resolution Spectrograph (Side Two) was used to make = observations of star SK-68D73 which is located in the Large Magellanic = Cloud. The intent is to measure the relative abundances of Cr II relative = to Zn II in the interstellar medium. Because zinc does not deplete onto = dust grains while chromium does, their abundance ratio measures dust = distribution. A wavelength calibration image was also taken. Near the = beginning of this proposal, at 344/042837Z there was a brief loss of fine = lock during which the take data flag went down. HSTAR 5399 was written to = document this event. Otherwise, the observations were completed as = planned, and there were no reported anomalies 1.17 Completed FGS 6271 (L726-8/UV Ceti) The FGSs were used to make astrometric observations of the binary = star L726/UV Ceti to search for a short period low-mass companion around = either component of this binary object. The observations were executed as = scheduled, and no anomalies were reported. 1.18 Completed WF/P-2 6254 (GTO Pure Parallel Program - Cycle 5) The WF/PC-2 was use to make random long exposures of high galactic = fields taken in parallel with the prime science observations to obtain a = random sample of galaxies. The observations were executed as scheduled, = and no anomalies were noted. 1.19 Completed FOS/RD 6110 (Abundances of Evolved Massive Stars in the = LMC) The Faint Object Spectrograph (Red Side) was used to make = spectrographic observations of the ejecta from the evolved luminous = massive star R143, which is located in the Large Magellanic Cloud. This = star is at a point in its evolution between an O class star and a = Wolf-Rayet class star, and the spectra will be used to determine the = elemental abundances and electron temperatures and densities. The = observations were executed as scheduled, and no anomalies were noted. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 20 Successful : 20 The was a brief loss of fine lock at 344/042837Z. HSTAR 5399 was written. Scheduled Reacquisitions : 15 Successful : 15 2.2 FHST Updates: Scheduled : 38 Successful : 38 2.3 Operations Notes: HST operations continue to be performed uneventfully from the SEER = as the MOR/SMOR is undergoing refurbishment. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH