HUBBLE SPACE TELESCOPE DAILY REPORT #2301 PERIOD COVERED: 0000Z (UTC) 02/03/99 - 0000Z (UTC) 02/04/99 Daily Status Report as of 035/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed Two Sets of STIS/CCD 7948 (CCD Dark and Bias Monitor -- Cont. to Dec. 98) The Space Telescope Imaging Spectrograph (CCD) was used to measure CCD dark current and bias rates for the two supported amplifier settings {GAIN=1 and GAIN=4} in order to gather data for making superdarks and superbiases. The data will be used to track the growth of hot pixels on the CCD in general and within the various target acquisition apertures specifically. The observations were executed as scheduled, and no anomalies were noted. 1.2 Completed Two Sets of WF/PC-2 7713 (WF/P-2 Cycle 7 Supplemental Darks pt3/3) The WF/PC-2 was used to make supplemental dark calibration images. This dark calibration program obtains three dark frames every day to provide data for monitoring and characterizing the evolution of hot pixels. The observations were completed as planned, and no anomalies were noted. 1.3 Completed WF/PC-2 6352 (Dwarf Elliptical Galaxy Snapshots) The WF/PC-2 was used to survey galaxy VCC1495, from a sample of 30 dwarf elliptical galaxies. The observations were completed as planned, and no anomalies were reported. 1.4 Completed Four Sets of STIS/CCD 8091 (POMS Test Proposal: STIS Non-Scripted Parallel Proposal Continuation) The Space Telescope Imaging Spectrograph (CCD) was used to make high galactic latitude, non-scripted, parallel observations. The observations were completed as planned, and no anomalies were noted. 1.5 Completed Three Sets of STIS/CCD 8084 (POMS Test Proposal: STIS Non-Scripted Parallel Proposal Continuation) The Space Telescope Imaging Spectrograph (CCD) was used to make non-scripted parallel high galactic latitude observations as part of POMS test proposal. The observations were executed as scheduled, and no anomalies were noted. 1.6 Completed WF/PC-2 6344 (Low - Mass Binaries in the Hyades - Completing the Survey) The WF/PC-2 was used to make observations of the low mass binary star RHY326 (M-Class Dwarf Stars) which is located in the Hyades Cluster. The observations were executed as scheduled, and no anomalies were noted. 1.7 Completed WF/PC-2 8289 (Development and Evolution of YSO Outflows and Jets) The WF/PC-2 was used to study the jets and YSO outflow from variable star XZ-Tau in order to study its development and evolution. The observations were executed as scheduled, and no anomalies were noted. 1.8 Completed STIS/CCD/MA1 7440 (Eclipse Mapping of the Touchstone Binary System YY Gem) The Space Telescope Imaging Spectrograph (CCD and MA1) was used to make eclipse mapping observations of the touchstone eclipsing binary star system YY-Gem. Solar images clearly demonstrate that its atmosphere consists not of homogeneous, temperature-stratified layers, but rather of discrete structures on spatial scales ranging from <100 km to a large fraction of the solar radius, non-uniformly distributed across the solar disk. A wavelength calibration image was also taken. The observations were completed as planned, and no anomalies were reported. 1.9 Completed Two Sets of WF/PC-2 8090 (POMS Test Proposal: WF-II Parallel Archive Proposal Continuation) The WF/PC-2 was used in the parallel mode to make some low galactic latitude archive observations. The program will be used to take parallel images of random areas of the sky. The acquisition failure described in 2.1 and HSTAR 6968 occurred during the first iteration of this proposal. The take data flag remained down, affecting two observations. Otherwise, the observations were executed as scheduled, and no further anomalies were noted. 1.10 Completed STIS/CCD/MA1/MA2 7389 (Chromospheres and Transition Layers in Hyades and Pleiades F stars) The Space Telescope Imaging Spectrograph (CCD, MA1 and MA2) was used to make observations of the F class star HD28033 which is located in the Hyades star cluster. This proposal seeks to obtain additional empirical constraints on the heating mechanisms for stellar chromospheres, transition layers and coronae. The acquisition failure described in 2.1 and HSTAR 6968 occurred at the beginning of this proposal but, since the re-acquisition was successful, only a part of the proposal was affected (five observations). Otherwise, the observations were completed as planned, and no further problems were reported. 1.11 Completed WF/PC-2 6347 (A Search for Jets in Planetary Nebulae) The WF/PC-2 was used to make observations of the planetary nebulae (class PNe) M1-92 in order to search for the presence of possible narrow jets. The current model for PNe formation indicates that jets are an unexpected phenomena, yet there is a growing body of circumstantial evidence that suggests narrow jets are common feature in PNe. The observations were completed as scheduled, and no anomalies were noted. 1.12 Completed WF/PC-2 7468 (Young Globular Clusters in Merger Remnants -- Part 4) The WF/PC-2 was used to make observations of merging galaxy NGC-5018 to study its globular clusters. Mergers seem to have played a major role in determining the shapes and dynamics of E and S0 galaxies. The observations were executed as scheduled, and no anomalies were noted. 2.0 FLIGHT OPERATIONS SUMMARY 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 6 Successful : 5 The acquisition scheduled for 034/150932Z failed when the search radius limit was exceeded on FGS-1. HSTAR 6968 was written. Previous FHST updates had shown small errors. An ARU/PRT was performed at 034/1626Z, followed by a real-time map at 034/1631Z, and the following re-acquisition was successful. The proposals described in 1.9 and 1.10 were affected. Scheduled Reacquisitions : 9 Successful : 9 2.2 FHST Updates: Scheduled : 15 Successful : 15 2.3 Operations Notes: Using ROP SR-1, the SSR EDAC error counter was cleared three times. Two TTRs were written for data inversions and for a data hit with seven accompanying missing minor frames. There has been no significant change in the Gyro-3 bias trend. Because the gyro does not appear to be stabilizing to a value consistent with the remaining gyros (this was expected since that was the case with Gyro-6 when it experienced a similar anomaly), Gyro-3 will not be placed into the control loop until it obtains a nominal bias rate of approximately 0.003 arcseconds/second per day. PCS engineers will continue to monitor the bias trend and all other key performance measures. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Continuation of normal science observations and calibrations. /DMH