HUBBLE SPACE TELESCOPE DAILY REPORT #1630 PERIOD COVERED: 0000Z (UTC) 05/08/96 - 0000Z (UTC) 05/09/96 Daily Status Report as of 130/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed WF/PC-2 5964 (Detecting Emission Lines at Half the = Hubble Time) The WF/PC-2 was used as part of a parallel program to make = observations which are used to search for emission lines in distant = clusters of galaxies. The objective is to study star formation at Z=3D = 0.75. The observations were completed as planned and no problems were = reported. 1.2 Completed GHRS/2 6169 (HRS Eschelle Wavelength Monitor) The High Resolution Spectrograph (Side 2) was used to calibrate = carrousel function, Y-deflection, resolving power, sensititity, and = scattered light for both eschelle-A and eschelle-B. All exposures are = internals. The observations were completed as planned, and no problems = were reported. 1.3 Completed Two Sets of 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 objects Q2226+023 and Q1338+381. This is to determine = if these high redshifted object have a far ultraviolet flux. The observat= ions were executed as scheduled, and no anomalies were noted. 1.4 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. 1.5 Completed FOS/BL 5928 (Hidden QSOs in "Warm" Infrared Ultraluminaou= s Galactic Nuclei) The Faint Object Spectrograph (Blue Side) was used to make = spectropolarimetric observations of active galactic nuclei IR1334+24 to = look for "warm" infrared ultra luminous galactic nuclei. = Spectropolarmetry of this object was done from the ground at optical = wavelengths, and the ultraviolet observations with HST are needed to = distinguish between the different mechanisms producing the polarization. = The observations were completed as planned, and no problems 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 WF/PC-2 6684 (WF/PC-2 Imaging of 2 JY Radio Galaxies) The WF/PC-2 was used to make observations of the radio galaxy = 6C1129+39 from the 6C catalog. These data will be used to look for a = correlation of optical structures with known radio luminosity. If such a = correlation exists, then it will allow the importance of the radio beam = power to the optical structure to be quantified. The observations were = executed as scheduled, and no anomalies were noted. 1.8 Completed WF/PC-2 6524 (WF/PC-2 Mapping of Dust Obscuration and = Stellar Populations in Starburst Galaxies) The WF/PC-2 was used to make narrow and broad band observations of the = nearby galaxy NGC-5253 in order to map dust obscuration and stellar = populations in its star bursting regions. Its starburst regions are = resolved with the HST, so the spatial distribution of the massive (i.e., = bright) stars and the ionized gas map can be constructed. The = observations were completed as planned, and no problems were reported. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 3 Successful : 3 Scheduled Reacquisitions : 12 Successful : 12 2.2 FHST Updates: Scheduled : 7 Successful : 6 The update at 130/0130Z failed due to FHST2. 2.3 Operations Notes: There were no significant reported problems. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH