HUBBLE SPACE TELESCOPE DAILY REPORT #1529 PERIOD COVERED: 0000Z (UTC) 12/04/95 - 0000Z (UTC) 12/05/95 Daily Status Report as of 339/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed Four Sets of WF/PC-2 6188 (WF/PC-2 Cycle 5 Calibration: = Dark) The WF/PC-2 was used to make internal dark calibration images. The = observations were completed as scheduled, and no problems were reported. 1.2 Completed WF/PC-2 5972 (Determination of the Extragalactic Distance = Scale) The WF/PC-2 was used to make observations of the galaxy NGC-3351 = 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. 1.3 Completed FOS/BL 5843 (First Ultraviolet Spectrographic Survey of = 2060 Charon) The Faint Object Spectrograph (f/48) was used to make ultraviolet = spectrographic observations of the deep solar-system object 2060-Chiron = while it is near perihelion. This will provide information on the = properties of the surface of Chiron and the gas surrounding it. At = 338/032856Z and at 338/084050Z, there were two losses of lock, resulting = in the take data flag going down. Otherwise, the observations were = executed as scheduled, and no anomalies were noted. 1.4 Completed WF/PC-2 6313 (The Hubble Deep Field (HDF) Experiments) The WF/PC-2 was used to make selected ultraviolet, visible and = near-inferred in the continuous view zone (i.e., CVZ) using the Hubble = Deep Field HDF-123649 to study the morphology and spectral information on = extremely faint field galaxies. This is a feasibility test in preparation = for further studies. The observations were completed as scheduled, and no = anomalies were reported. 1.5 Completed GHRS/2 5857 (Is Mixing or Mass Loss the Cause of Decline = in 12C/13C?) The High Resolution Spectrograph (Side Two) was used to make = spectrographic observations of the halo star HD3546 to study the ratio of = its 12C/13C carbon and the abundance of its boron. The results will = influence models of evolution off of the main sequence. The observations = were completed as planned, and no problems were reported. 1.6 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 SGP017 (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. 1.7 Completed Two Sets of FOC/48 6255 (Long Slit Spectroscopy of the = Center of M-31) The Faint Object Camera (f/48) was used to make long-slit = spectrographic observations of the central region and double nucleus of = galaxy NGC-224 (aka, the Andromeda Galaxy). The aim is to get a = high-resolution rotation curve and also to get velocity dispersion as a = function of position. A dark calibration image was also taken. The = observations were completed as planned, and no problems were reported. 1.8 Completed Two Sets of WF/PC-2 6114 (White Dwarf Distance and = Precision Age for the Globular Cluster 47 Tuc) The WF/PC-2 was used to make observations of white dwarf star = WD1647+591 which is located in the globular cluster 47 Tuc in order to = study the cluster's age and distance. This set of observations will be = used to determine the distance to 47 Tuc, hopefully to an accuracy of = better than 10%. The observations were executed as scheduled, and no = anomalies were noted. 1.9 Completed WF/PC-2 5849 (Host Galaxies of Luminous Nearby Quasars) The WF/PC-2 was used to make deep exposure observations of host = galaxy PG1444+407 which is known to have a luminous nearby quasar. The = observations were executed as scheduled, and no anomalies were noted. 1.10 Completed 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 nebula NGC-3132 to study its nuclei and to look for possible = companions. The observations were executed as scheduled, and no anomalies = were noted. 1.11 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 galaxy = NGC-2768 in order to study its 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. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 8 Successful : 8 Scheduled Reacquisitions : 9 Successful : 9 2.2 FHST Updates: Scheduled : 13 Successful : 13 2.3 Operations Notes: There were no operational problems reported. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH