HUBBLE SPACE TELESCOPE DAILY REPORT #1506 PERIOD COVERED: 0000Z (UTC) 10/27/95 - 0000Z (UTC) 10/30/95 Daily Status Report as of 303/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed FOS/RD 6080 (Rotation and Kinematics of Blue Stragglers = in 47 Tuc) The Faint Object Spectrograph (Red Side) was used to make = spectrographic observations for blue straggler stars located in 47 Tuc = (aka, NGC-104) in order to study the rotation and radial velocity of these = stars. The observations were completed as scheduled, and no anomalies = were noted. 1.2 Completed WF/PC-2 6189 (WF/PC-2 Cycle 5 Calibration: Internal = Monitor - Vis Flats) The WF/PC-2 was used to make internal visual flat calibration = images. Both photometric and narrow-band filters were used. The = observations were executed as planned, and no problems were reported. 1.3 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 SMC-SMP02 which is = located in the Small 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. 1.4 Completed Two Sets of WF/PC-2 6119 (Snapshot Survey for Companions = of Planetary Nebula Nuclei) The WF/PC-2 was used to make snapshot survey observations of = planetary nebulae NGC-6572 and NGC-2346 to study their nuclei and to look = for possible companions. During the second iteration of this proposal, = an FGS acquisition, described in 2.1, failed. Otherwise, the observations = were executed as scheduled, and no anomalies were noted. 1.5 Completed WF/PC-2 6250 (WF/PC-2 Cycle 5 Calibration: Internal = Monitor) The WF/PC-2 was used to make a series of internal calibration = observations. Internal flats, biases, and K-Spot calibration images were = taken. These observations are designed to monitor the health of the = cameras. During this proposal, there were two FHST update failures, = described in 2.2. There was no report of possible effects on science. 1.6 Completed FGS 6268 (The Parallax of NGC-6853) The FGSs were used to make astrometric observations in order = measure the parallax to NGC-6853, one of the nearest planetary neabulae. = Observations were also taken of several reference stars. During this = observation, the guide star acquisition failed. This event is described = in 2.1. Otherwise, the observations were executed as planned, and no = problems were reported. 1.4 Completed Two Sets of 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. 1.8 Completed FGS 6325 (Monitor the Long-Term Stability for FGS #3 = Still) FGS#3 was used to make observations of standard star OF957, and = several reference stars which are located in the star cluster M-35 in = order to monitor the long-term internal stability of the FGS unit. The = observations were completed as planned, and no anomalies were noted. 1.9 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 concurrent 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. 1.10 Completed WF/PC-2 6187 (WF/PC-2 Cycle 5 Calibration: Earth Flats) 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 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. The observations were = completed as planned, and no anomalies were reported. 1.12 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. 1.13 Completed WF/PC-2 5996 (The Morphology of Field Galaxies at High = Redshifts) The WF/PC-2 was used to make observations of several field galaxies = (Field 2217) in order to study their morphologies. The observations were = completed as planned, and no anomalies were reported. 1.14 Completed WF/PC-2 5914 (The Formation History of Globular Clusters = in M-33) The WF/PC-2 was used to make V and I observations of globular = cluster NGC-598-U13 which is located in the M-33 galaxy in order to study = its formation history. Color-magnitude diagrams made from these images = will be examined for evidence of a parameter, other than metallicity, that = influences the evolutionary development of stars. The observations were = executed as scheduled, and no anomalies were noted. 1.15 Completed WF/PC-2 5968 (Extragalactic Background Light) The WF/PC-2 was used to make direct observations of the magnitude = and color of the diffuse extragalactic background light. Knowledge of the = value of the integrated optical flux of this background is of fundamental = importance to cosmology. A dark and bias observations were also taken. = The observations were completed as planned, and no anomalies were = reported. 1.16 Completed WF/PC-2 6184 (WF/PC-2 Cycle 5 Photometric Calibration = Monitor UV/OPT STD) The WF/PC-2 was used to make ultraviolet and optical observations = of standard star GRW+70D582 in order to monitor the photometric = calibrations of the camera and to check for decontamination. The = observations were executed as scheduled, and no anomalies were noted. 1.17 Completed FOS/RD 6050 (Spectrographic and Photometric Study of the = very Low Mass Triple System) The Faint Object Spectrograph (ResSide) was used to make = spectrographic observations of the very low mass triple star system = LHS1070-A which has a high proper motion, high internal motions, and has = annual parallax of 0.13". The observations were completed as planned, and = no problems were reported. 1.18 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 1.19 Completed WF/PC-2 5913 (Low-Mass Binaries and Luminosity Fuction) The WF/PC-2 was used to make observations of the low-mass binary = system MT003 (Late Type Class M dwarf stars). The intent is to determine = why the local stellar luminosity function is flat below Mv=3D12, while = that found from more distant stars falls by an order of magnitude by = Mv=3D14. The observations were executed as scheduled, and no anomalies = were noted. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 15 Successful : 13 The FHST update failures, mentioned in 2.2, caused the acquisitions at 301/012603Z and 301/021002Z to fail. A subsequent ARU/PRT corrected the attitude error. HSTAR 5344 was written. Scheduled Reacquisitions : 27 Successful : 27 2.2 FHST Updates: Scheduled : 35 Successful : 33 There were failures at 301/002331Z and 301/002616Z because of an attitude error. HSTAR 5344 described these events. 2.3 Operations Notes: HSTAR 5343 was written to document an FGS-1B star selector comp error exceeding the +10 volt limit for approximately one second. This event occurred at 300/221325Z. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH -END-