HUBBLE SPACE TELESCOPE DAILY REPORT #1661 PERIOD COVERED: 0000Z (UTC) 06/21/96 - 0000Z (UTC) 06/24/96 Daily Status Report as of 176/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed Two Sets of FOS/RD 6236 (FOS Cycle 5: Location of = Spectra and Wavelength Calibration: Red Side Detector) The Faint Object Spectrograph (Red Side) was used to make = calibration observations in order to determine the location of the = spectra and to perform a wavelength calibration. All observations were = internal. A Taled calibration was also completed. The observations were = completed as planned, and no anomalies were reported. 1.2 Completed WF/PC-2 6629 (Observations of a New Sample of = Gravitational Lens Candidates ) The WF/PC-2 was used to make observations of the gravitational = lens candidate QSO-113000. This object was identified in the first and = second phases of the Cosmic Lens All-Sky Survey done with the Very Large = Array radio telescope. The observations were executed as scheduled, and = no anomalies were noted. 1.3 Completed WF/PC-2 6431 (Determination of the Extragalactric = Distance Scale) The WF/PC-2 was used to make observations of the galaxy NGC-4535 = to be used in measuring the periods of Cepheid variable stars within this = galaxy. This will allow for a more accurate estimate of the distances to = these galaxies through the period-luminosity relation for the Cepheid = stars. The observations were executed as scheduled, and no anomalies = were noted. 1.4 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. 1.5 Completed WF/PC-2 6002 (Spectroscopy of the Rapidly Rotating = Nuclear Disk in the Virgo S0 NGC-4526) The WF/PC-2 was used to make spectrographic observations of the = rapidly rotating nuclear disk in S0 class galaxy NGC-4526 which is = located in the Virgo Cluster. The nucleus of this galaxy was imaged in = cycle 4, and new images with different filters were used to make color = corrections and allow the subtraction of the stellar continuum. The = observations were completed as planned, and no problems were reported. 1.6 Completed WF/PC-2 5997 (The Cores of Elliptical Galaxies in the = Coma Cluster) The WF/PC-2 was used to make observations of the large elliptical = galaxies GAL-125054 and IC832 which are located in the Coma Cluster. The = purpose is to study the luminosity profiles in their central nuclear = regions. The observations were completed as scheduled, and no anomalies = were noted. 1.7 Completed GHRS/1 6758 (Far UV airglow and Albedo Observations of = Europa and Ganymede) The High Resolution Spectrograph (Side One) was used to make far = ultraviolet spectrographic observations of the airglow and albedo of = Jupiter's moon Ganymede. Observations were made of both the leading and = trailing hemispheres. The long term stability of the oxygen airglow = emission and the magnitude of the hemisphere asymmetry will be = determined. The observations were completed as planned, and no problems = were reported. 1.8 Completed Two Sets of WF/PC-2 6183 (WF/PC-2 Cycle 5 Calibration: = Decon) The WF/PC-2 was used to make some internal flat, K-Spot, and dark = calibration images. The purpose is to define decontamination procedures = to be run during Cycle 5. The calibration observations were completed as = scheduled, and no anomalies were reported. 1.9 Completed WF/PC-2 5984 (Absorption - Selected Galaxies) The WF/PC-2 was used to study the morphology of galaxy PKS1354+19, = at redshifts from 0.4 to 1.0, that is absorbing light from background = quasars. The absorbing galaxies were discovered from ground-based = surveys. The observation was completed with no reported anomalies. 1.10 Completed FOS/BL 6474 (UV Spectroscopy of a Peculiar Highly = Magnetic White Dwarf) The Faint Object Spectrograph (Blue Side) was used to make = ultraviolet spectrographic observations of the peculiar, highly magnetic, = white dwarf star HE1211-170. This star shows spectral variations which = are believed to be due to a magnetic field which is relatively uniform in = one hemisphere and much more heterogeneous in the other. The = observations were executed as scheduled, and no anomalies were noted. 1.11 Completed Two 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. 1.12 Completed FOS/RD 6577 (An Expanded Survey for Study of the = Lyman-Alpha Line and QSO Mg II Absorption) The Faint Object Spectrograph (Red Side) was used to make = observations of the QSO PKS1127-14 in order to make a survey of the = Lyman-Alpha line and the 68 Mg II absorption line system. The = observations were completed as scheduled, and no problems were reported. 1.13 Completed WF/PC-2 6557 (Redshift Absorption Selected Galaxies) The WF/PC-2 was used to make observations of the galaxy Q1241 = where a halo appears to be absorbing light from the background = quasi-stellar object (QSO) Q1241. The observations were completed as = planned, and no problems were reported. 1.14 Completed Two sets of WF/PC-2 5844 (HST Investigation of a = Bright, New Comet) The WF/PC-2 was used to make observations of the bright new comet = Hale-Bopp (aka, Comet C/1995 O1). The images will yield information of = the nuclear size and coma near the nucleus. The observations were = completed as planned, and no anomalies were noted. 1.15 Completed GHRS/2 5869 (Chromospheric Activity in Quiet stars: = Halo Subdwarfs) The High Resolution Spectrograph (Side Two) was used to make = spectrographic observations of the quiet star HD219617 to study its = chromospheric activity. This is a search for Mg II emission in low = metallicity solar temperature field stars in the galactic halo. The = observations were completed as planned, and no problems were reported. 1.16 Completed FOS/BL 6721 (Ultra-Rapid Continuum Variability as a = Probe of AGN Physics) The Faint Object Spectrograph (Blue Side) was used to make observat= ions of the ultra-rapidly variability in the continuum of the active = galactic nuclei of Seyfert galaxy NGC-7469. These data will be used to = study the temporal variations which have been observed in the past, and = to determine its wavelength dependence and the time delay between the = variations in the ultraviolet and optical parts of the spectrum. The = observations were completed as scheduled, and no problems were noted. 1.17 Completed FOC/96 6349 (Snapshot search for High Redshift QSOs = with Far-UV Flux) The Faint Object Camera (f/96) was used to make snapshot images of = the quasi-stellar object Q2203-357. This is to determine if this high = redshifted object has a far ultraviolet flux. The observations were = executed as scheduled, and no anomalies were noted. 1.18 Completed FOS/BL 6489 (The Identification and Cooling of the = White Dwarf in WZ SGE Like Systems) The Faint Object Spectrograph (Blue Side) was used to make = spectrographic observations of the white dwarf nova in the AL Com system. = AL Com, like WZ Sge, has outburst in the last month. These outbursts = are usually separated by decades, but Al Com went though an outburst in = the spring of 1995. The observations were completed as planned, and no = anomalies were reported. 1.19 Completed WF/PC-2 5971 (HST Medium Deep Survey) The WF/PC-2 was used to make long-exposure, medium-deep sky survey = observations at latitudes larger than 10 degrees taken in parallel with = the prime science observations. The observations were executed as = scheduled, and no anomalies were noted. 1.20 Completed WF/PC-2/GHRS/1 5828 (HST Far-UV Imaging and Spectra of = Jupiter Coordinated With the Galileo Probe) The WF/PC-2 and the High Resolution Spectrograph (Side One) were = both used to make images and ultraviolet spectrographic observations of = the planet Jupiter in order to study the auroral zones located near the = planet's magnetic poles. These observations were taken at the same time = that the Galileo spacecraft makes spectral observations. As reported in = Section 2.1, after the initial acquisition and reacquisition, several = periods of guide star loss of lock occurred. No further problems were = reported. 1.21 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 HE3-1475 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. 1.22 Completed WF/PC-2 6348 (Blue Continuum Snapshots of 3CR Radio = Galaxies) The WF/PC-2 was used to make some snapshot images of the blue = continuum in radio galaxy 3C415.2. Combined with existing data, these = exposures will provide high spatial resolution information on the color = distribution within galaxies, redding due to dust, spacial indices of the = optical synchrotron jets, and colors of the active nuclei and tidal jets. = The observations were executed as scheduled, and no anomalies were = noted. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 23 Successful : 23 Scheduled Reacquisitions : 22 Successful : 22 As documented in HSTAR 5640, several periods of guide star loss of = lock occurred after the successful acquisition and reacquisition at = 175/1305Z and 175/1312Z. 2.2 FHST Updates: Scheduled : 50 Successful : 49 The update scheduled at 176/0230Z failed. 2.3 Operations Notes: HSTAR 5638, written by Data Capture Facility personnel reported = data drop-outs during several WF/PC-2 observations made on day 170. = Subsequent HSTAR 5639, written by the STScI, pointed out similarities = between this occurrence and events which happened just before ESTR #2 was = turned off. Further analysis is being performed. Otherwise, there were no significant operational problems = occurring this weekend. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH