HUBBLE SPACE TELESCOPE DAILY REPORT #1601 PERIOD COVERED: 0000Z (UTC) 03/28/96 - 0000Z (UTC) 03/29/96 Daily Status Report as of 089/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed FOS/RD 6167 (FOS Cycle 5: Dark Monitoring) The Faint Object Spectrograph (Red Side) was used to make several = dark calibration images. All exposures were internals. All spectra was = done in the image mode. The observations were completed as planned, and n= o problems were reported. 1.2 Completed FOS/RD 6165 (FOS Cycle 5: Discriminator Test) This is a calibration proposal, which is being used to verify the = optimal discriminator settings for the FOS. The observations were = executed as scheduled, and no anomalies were noted. 1.3 Completed Two Sets of WF/PC-2 6363 (The Environments and Host = Galaxies of BL-Lac Objects) The WF/PC-2 was used to make snapshot survey observations of = BL-Lac objects PKS0426-38 and MS1312.1-4 in order to study their = environment and their host galaxies. The goal is to investigate = systematic trends in host galaxy type, unusual morphological features, = nearby companion galaxies, etc. The observations were executed as = scheduled, and no anomalies were noted. 1.4 Completed WF/PC-2 5983 (Curcumstellar Disks in Young Nebulous = Clusters) The WF/PC-2 was used to make observations of the young nearby = nebulous cluster NGC-2264 looking for possible curcumstellar disks (Solar = nebula analogs), like the type seen in the Orion Nebula. The = observations were completed as planned, and no problems were reported. 1.5 Completed WF/PC-2 6346 (Snapshot Survey of the Ultraluminous IRAS = Galaxy Sample-Part 1 High) The WF/PC-2 was used to make snapshot survey observations of the = ultraluminous IRAS galaxy QDOTULIR18. These data will be searched for = multiple cores, which imply a merger has occurred, and for starburst = regions. The FGS acquisition for this proposal defaulted to guidance on = FGS #3 only at 088/073646Z. HSTAR 5551 documented the event. Otherwise, = the observations were executed as scheduled, and no anomalies were noted. 1.6 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. 1.7 Completed WF/PC-2 5997 (The Cores of Elliptical Galaxies in the = Coma Cluster) The WF/PC-2 was used to make observations of the large elliptical = galaxy NGC-4906 which is located in the Coma Cluster. The purpose is to = study the luminosity profiles in the central nuclear region. The = observations were completed as scheduled, and no anomalies were noted. 1.8 Completed FOS/RD 6089 (Eclipse Mapping and Tomography of the UV = Emitting Region of DQ Her) The Faint Object Spectrograph (Red Side) was used to make Rapid Mod= e ultraviolet observations of the eclipsing binary star 14Aur-C in order = to do eclipse mapping and tomographic studies. Observations were made of = both the ultraviolet continuum and emission lines. The observations were = executed as scheduled, and no anomalies were noted. 1.9 Completed WF/PC-2 6102 (Chemical Evolution and History of Star = Formation in the Large Magallanic Cloud) The WF/PC-2 was used to make observations of the "Bar" region in = the Large Magellanic cloud to study the chemical evolution and the = history of star formation in that region. The goal is to observe = individual field stars near the main sequence turnoff in order to study = the large scale process that control star formation and nucleosynthesis = in galaxies. The observations were executed as planned, and no anomalies = were reported. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 7 Successful : 7 Scheduled Reacquisitions : 10 Successful : 10 2.2 FHST Updates: Scheduled : 9 Successful : 9 2.3 Operations Notes: There were no operational problems. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH