HUBBLE SPACE TELESCOPE DAILY REPORT #1622 PERIOD COVERED: 0000Z (UTC) 04/26/96 - 0000Z (UTC) 04/29/96 Daily Status Report as of 120/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 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. 1.2 Completed Two Sets of WF/PC-2 6363 (The Environments and Host = Galaxies of BL-Lac Objects) The WF/PC-2 was used to make snapshot survey observations of = BL-Lac objects 1ES0525+71 and EXO-0706.1 in order to study their = environments and their host galaxies. The goal is to investigate = systematic trends in host galaxy type, unusual morphological features, = nearby companion galaxies, etc. The observations were executed as = scheduled, and no anomalies were noted. 1.3 Completed FGS 6326 (Monitor the Long Term Stability of FGS#3 - = Early 1996) FGS#3 was used to make astrometric observations of star OF956 and = other nearby standard stars which are located in the M-35 open star = cluster in order to test the long term stability of the FGS unit. The = observations were completed as planned, and no problems were reported. 1.4 Completed WF/PC-2 6303 (Observations of Galaxies Underlying = Quasars) The WF/PC-2 was used to make observations of low red shift quasar = LTT9491 in order to study its underlying galaxy. The purpose is to = detect structure down to the 0.1 arcsecond level. The observations were = completed as planned, and no problems were reported. 1.5 Completed Two Sets of WF/PC-2 5953 (Galactic Bulge Studies: A Deep = UV Survey) The WF/PC-2 was used to make ultraviolet observations of the UV = bright stars in areas BWUV-4 and BWUV-5 in order to perform a survey of = the galactic halo luminosities, effective temperatures, and star counts = per unit of luminosity. The observations were completed as planned, and = no problems were reported. 1.6 Completed FOS/BL 6202 (Cycle 5 FOS Spectral Flat field = Calibration) The Faint Object Spectrograph (Blue Side) was used to make = observations of the relatively featureless white dwarf star WD0501+527 in = order to make flat field calibration images. The observations were made = through the 1.0 aperture, with all usable detector/disperser = combinations. The observations were executed as schedule, and no anomalie= s were noted. 1.7 Completed Four 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. 1.8 Completed FGS 6241 (Companion to W922 (GL831)) The FGSs were used in both the POS and TRANS Mode to make = astrometric observations of star W922 (aka, Gleise 831) to measure its = parallax and looking for possible companions. Several other reference = stars were also observed. The observations were completed as planned, = and no problems were reported. 1.9 Completed WF/PC-2 6364 (Snapshot Survey of Proto-Planetary Nebulae = and AGB Stars) The WF/PC-2 was used to make some snapshot survey observations of = protoplanetary nebular system IRAS17441 to study its circumstellar = envelope. The purpose is to discern the evolutionary sequence that = produces axially-symmetric planetary nebulae. The observations were = executed as scheduled, and no anomalies were noted. 1.10 Completed Two Sets of WF/PC-2 6363 (The Environments and Host = Galaxies of BL-Lac Objects) The WF/PC-2 was used to make snapshot survey observations of = BL-Lac objects PKS1144-37 and PG1424+240 in order to study their = environment and their host galaxies. The goal is to investigate systemati= c trends in host galaxy type, unusual morphological features, nearby = companion galaxies, etc. The observations were executed as scheduled, = and no anomalies were noted. 1.11 Completed WF/PC-2 5972 (Determination of the Extragalactic = Distance Scale) The WF/PC-2 was used to make observations of the galaxy NGC-4321 = looking for standard candle Cepheid variable stars. The purpose of this = observations is to help estimate the Hubble constant with an accuracy of = 10%. The observations were executed as scheduled, and no anomalies were = noted. 1.12 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. 1.13 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. 1.14 Completed GHRS/2/1 6275 (Heavy Element Abundances and Isotope = Anomalies in HR7775 and Chi Lupi) The high Resolution Spectrograph (Sides One and Two) were used to = make observations of the Hg-Mn (mercury-manganese) class star HD193452 = (aka, HR7775) in order to study its chemical abundances and isotope = anomalies. This star is known to exhibit unusual heavy element = abundances. The observations were completed as scheduled, and no = problems were reported. 1.15 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 = observation was also taken. The observations were completed as planned, = and no anomalies were reported. 1.16 Completed FGS 6264 (Parallax of RR-Lyrae) The FGSs were used to make astrometric observations of the = variable star RR-Lyrae in order to measure its parallax. RR-Lyrae is the = proto-type for a class of variable stars whose pulsation periods = correlate with their absolute magnitudes. The observations were = completed as planned, and no problems were reported. 1.17 Completed WF/PC-2 6360 (A Snapshot Survey of "Radio Load" IRAS = Galaxies) The WF/PC-2 was used to make snapshot survey observations of the = radio load IRAS galaxy GAL-0749+2. The WF/PC-2 was used to discern high = surface brightness structures in its post-starburst active nuclear = regions. The observations were completed as scheduled, and no anomalies = were reported 1.18 Completed WF/PC-2 6646 (WF/PC-2 Imaging Dwarf Spirals) The WF/PC-2 was used to make ultraviolet and blue observations of = the dwarf spiral galaxy D564-15. It is known to have low surface = brightness with very blue mean color but no evidence of recent or past = star formation. As reported in 2.1, the FGS acquisition for this = proposal failed. No other problems were reported. 1.19 Completed FGS 6049 (Monitoring the Size and Shape of Mira Type = Stars) The FGSs were used to make astrometric observations of the Mira = class star HD847748 in order to study its size and shape during different = phases of its pulsation cycle. The observations were completed as = planned, and no anomalies were reported. 1.20 Completed FOC/BL 6053 (Extreme UV Stars in Omega Cent) The Faint Object Spectrograph (Blue Side) was used to make = observations of extremely ultraviolet bright stars in NGC-5139 (aka, = Omega Cent). These stars were also viewed by the UIT on ASTRO-1. The = observations were executed as scheduled, and no anomalies were noted. 1.21 Completed WF/PC-2 6286 (Nuclei of Nearly Normal Galaxies (WC12): = Cycle 5) The WF/PC-2 was used to make observations of nuclei of the nearly = normal galaxy NGC-4649 to measure the space density profile of luminous = material and the nuclear color gradients in this object. The images will = be searched for bright stars, inner globular clusters, and absorbing = interstellar dust. The observations were executed as scheduled, and no = anomalies were noted. 1.22 Completed WF/PC-2 5920 (Extragalactic Globular Cluster System) The WF/PC-2 was used to make observations to compile a catalogue = of the extragalactic globular clusters in galaxy NGC-5846. A luminosity = function will be derived which should be complete down to the 27th = magnitude in V. The observations was completed as planned, and no = problems were reported. 1.23 Completed WF/PC-2 6117 (Fliers in Planetary Nebulae) The WF/PC-2 was used to make observations of planetary nebula = NGC-7009 in order to look for fliers. A flier is plasma knot embedded = within highly ionized elliptical and bipolar planetary nebulae. As = mentioned in 5.1, the FGS acquisition failed to fine lock backup on FGS = #3 only. No other anomalies were noted. 1.24 Completed FOS/BL 6476 (A Study of Circumstellar Material Formed = in a Hydrogen-Deficient Environment) The Faint Object Spectrograph (Blue Side) was used to make low = resolution ultraviolet spectral observations of the hot variable CrB-type = star V348-SGR in order to study the curcumstellar material formed in its = Hydrogern-deficient environment. The objective is to study the newly = formed dust associated with the brightness changes: fullerenes are one = possible component of the dust. The observations were completed as = planned, and no problems were reported. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 23 Successful : 21 The acquisition at 119/035008Z failed when the search radius limit = was exceeded. HSTAR 5585 was written. At 119/190852Z, as documented in HSTAR 5586, the acquisition = failed to fine lock backup on FGS #3 only. Scheduled Reacquisitions : 24 Successful : 24 2.2 FHST Updates: Scheduled : 45 Successful : 45 2.3 Operations Notes: No significant problems were reported at HST operations = experienced a relatively quiet week-end. 3.0 SIGNIFICANT FORTHCOMING EVENTS: GSFC Internal Simulation #4 (EVA #2) will be conducted on = Thursday. /DMH