HUBBLE SPACE TELESCOPE DAILY REPORT #1651 PERIOD COVERED: 0000Z (UTC) 06/07/96 - 0000Z (UTC) 06/10/96 Daily Status Report as of 162/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 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. 1.2 Completed WF/PC-2 6431 (Determination of the Extragalactric = Distance Scale) The WF/PC-2 was used to make observations of the galaxy NGC-4548 = 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 star= s. The observations were executed as scheduled, and no anomalies were = noted. 1.3 Completed Two Sets of 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. 1.4 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. 1.5 Completed FOS/RD 6449 (Spectroscopy of Two Further UV Bright High = Red Shifted Quasars) The Faint Object Spectrograph (Red Side) was used to make = ultraviolet spectrographic observations of the newly discovered, = ultraviolet bright, high red shifted quasar HE-2347-43 to look for = absorption from systems along the line of sight to the QSO. The = observations were executed as scheduled, and no anomalies were noted. 1.6 Completed WF/PC-2 5971 (HST Medium Deep Survey) The WF/PC-2 was used to make a 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. 1.7 Completed FOS/RD 6536 (IZW-18: Building Model) The Faint Object Spectrograph (Red Side) was used to make = observations of galaxy I-ZW-18-SEHI. This galaxy contains the H II = region with the lowest known metallicity. Thus it is important to our = understanding of the chemical evolution of galaxies, the primordial He = abundance, and low metallicity stellar populations. The observations = were completed as planned, and no problems were reported. 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 WF/PC-2 6439 (Using Cepheid Based Distance to Test Large = Peculiar Motions) The WF/PC-2 was used to make observations of the spiral galaxy = NGC-4603 which is located in the Centaurus galaxy cluster to look for = Cepheid variable stars to be used to measure the distance to the object, = which in turn will be used to study its large peculiar motions. If this = galaxy is a cluster member, as appears from secondary distance = indicators, then its peculiar velocity is inconsistent with that = predicted from the density field as reconstructed from the observational = distribution of galaxies in the cluster. The observations were executed = as scheduled, and no anomalies were reported. 1.10 Completed FOS/RD/BL 6017 (Soft X-Ray Transients, Outburst in = Black Hole Accretion Disks) The Faint Object Spectrograph (Both the Blue and Red Sides) were = used to make target of opportunity observations of the cataclysmic = contact-binary star J1655-40 which is known to show soft X-ray = transients. These outburst are believed to be caused by the accretion = disk surrounding a black hole. The observations were completed as = scheduled, and no problems were reported. 1.11 Completed FGS 6047 (Calibrating the Mass Luminosity Relation at = the End of the Main Sequence) The FGSs were used to make astrometric observations of star = GL866-FIXE as part of a study to determine its mass luminosity relationshi= p. The purpose is to measure the precise parallax and relative orbit of = its faint companion. The observations were completed as planned, and no = problems were reported. 1.12 Completed GHRS/1 5950 (Spectroscopy of the Three UV Brightest = Known High-Redshift Quasars) The High Resolution Spectrograph (Side One) was used to make = ultraviolet observations of quasar HS-1103+64 which is known to be one of = the brightest high redshift quasars. The objectives are to measure the = C, N, O, and Ne abundances in the halos of early galaxies, to measure the = intensity of the ionizing UV background, to measure He I, and to study = the Lyman-Alpha forest. The observations were completed as scheduled, = and no anomalies were reported. 1.13 Completed WF/PC-2 6964 (Photometry of Candidate Dwarf Spheroidal = Galaxies in the M81 Group) The WF/PC-2 was used to make photometric and two color images of = the candidate dwarf, spheroidal galaxy (dSph) GAL-100441 which is located = in the M-81 galaxy cluster group. From these data, a color-magnitude = diagram will be constructed, which will allow the determination of = various physical properties for the candidate dSphs. Near the end of = this 10-hour proposal, a loss of lock occurred at 161/210542Z. The = observations completed as scheduled, and no further problems were = reported. 1.14 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 QDOTULIR20 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. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 14 Successful : 14 A loss of lock occurred at 161/210542Z. Scheduled Reacquisitions : 26 Successful : 26 2.2 FHST Updates: Scheduled : 31 Successful : 3 2.3 Operations Notes: There were no significant problems encounterd this weekend. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH