HUBBLE SPACE TELESCOPE DAILY REPORT #1409 PERIOD COVERED: 0000Z (UTC) 06/09/95 - 0000Z (UTC) 06/12/95 Daily Status Report as of 163/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed FOS/RD 5684 (Geometry and Generalizability of the Reflected Light Model for Seyfert Galaxies) The Faint Object Spectrograph (Red Side) was used to make polarization observations near the nucleus of Seyfert galaxy MARK463E to test the theory that the Seyfert galaxies actually have Seyfert Type I cores, obscured by surrounding matter. The observations were completed as scheduled, and no problems were reported. 1.2 Completed FOS/BL 5095 (Spectra at Lambda <3000 Angstroms for QSOs with Z~2 (FOS 3): Cycle 4) The Faint Object Spectrograph (Blue Side) was used to make ultraviolet spectral observations of the absorption lines and high-ionization emission lines in QSO PKS0109+17. The observations were executed as scheduled, and no problems were noted. 1.3 Completed WF/PC-2 5981 (Calibration of Nearby Type IA Supernova as Standard Candles: NGC-4639) The WF/PC-2 was used to make observations of Cepheid variable stars in Galaxy NGC-4639 (which has produced a Type IA Supernova) to calibrate the nova's absolute brightness so that it can be used as a standard candle for distance measurements.The observations were executed as scheduled, and no anomalies were noted. 1.4 Completed WF/PC-2 5985 (WF/PC-2 B-Band + Lyman Alpha Imaging of a Cluster of Young Galaxies at Z = 2.0) The WF/PC-2 was used to make B-Band and Lyman Alpha observations (i.e., two color images) of the young dwarf spheroidal galaxy 53W002 located in Draco and which has a redshift of around 2.0. The observations were executed as planned, and no problems were reported 1.5 Completed WF/PC-2 5560 (WF/PC-2 Cycle 4 Calibration: Internal Monitor. 1) The WF/PC-2 was used to make several internal bias, K-Spot, and flat calibration observations to monitor the CCD camera electronics, the optical alignment, and to check for contamination. The observations were completed as planned, and no anomalies were noted. 1.6 Completed WF/PC-2 6234 (Stellar Populations in the Dwarf Spheroidal Galaxy Draco) The WF/PC-2 was used to make two color observations of a dwarf spheroidal galaxy located in Draco to study its stellar population and its star formation history. The observations were executed as scheduled, and no anomalies were noted. 1.7 Completed WF/PC-2 5476 (Continuum Snapshots of 3CR Radio Galaxies) The WF/PC-2 was used to make snapshot images of radio galaxy 3C460.0 as part of a continuum survey and to study the galaxy's morphology. The observations were executed as scheduled, and no anomalies were noted. 1.8 Completed WF/PC-2 5397 (Determination of the Extragalactic Distance Scale: Cycle 4 High) The WF/PC-2 was used to make images of galaxy NGC-4414 to be used in measuring the periods of Cepheid variable stars within this galaxy. The observations were completed as planned, and no anomalies were noted. 1.9 Completed FOS/RD 5535 (Cycle 4 Internal Wavelength Calibration) The Faint Object Spectrograph (Red Side) was used to make internal calibration observations to monitor the stability of the wavelength scale for different gratings. A wavelength calibration observation was also taken. The observations were completed as planned, and no problems were reported. 1.10 Completed WF/PC-2 5239 (Miscellaneous (WC18) Supplemental: Post-ERO Observations of Eta Car) The WF/PC-2 was used to make observations of Eta Carinae searching or interesting features and to provide second epoch information on the nebula for comparison with earlier observations. The observations were executed as scheduled, and no anomalies were noted. 1.11 Completed Two Sets of WF/PC-2 5479 (Subarcsecond Structure in Nearby AGNs) The WF/PC-2 was used to make snapshot observations of the nearby active galactic nuclei of NGC-788, IC184, PG0003+199 and IR0147-076 to study the interactions between the central engine, the stars, and the interstellar matter in these AGNs. The observations were executed as scheduled, and no anomalies were noted. 1.12 Completed GHRS/2 5424 (High Resolution Observations of the Jovian UV Aurora: Cycle 4 Medium) The High Resolution Spectrograph was used to make high resolution ultraviolet spectrographic observations of the aurora on the planet Jupiter short of 2000 A0. The goal is to determine the kinetic temperatures of the auroral region and the range of altitudes over which precipitating auroral particles deposit their energy and H2 Lyman and Werner Band emissions. The observations were executed as scheduled, and no anomalies were noted. 1.13 Completed WF/PC-2 5706 (Morphology of Distant Galaxies - Cycle 4 Carryover) The WF/PC-2 was used to make observations of a field of view designated as Field-0017. This is part of a study of the morphology of distant galaxies. The observations were completed as planned, and no problems were reported. 1.14 Completed WF/PC-2 5701 (Galaxy Populations in Intermediate Redshift Clusters: Cycle 4) The WF/PC-2 was used to observe fields in the Abell galactic cluster AC103 to study the morphology of the galaxies in the cluster so that they can be classified and used to learn more about the Butcher-Oemler effect. The observations were completed as planned, and no problems were reported. 1.15 Completed FOS/BL 6146 (FOS Location of Spectra and Aperture - Part 2) The Faint Object Spectrograph (Blue Side) was used to conduct a test to determine the repeatability of positioning the filter-grating wheel. All observations were internal. A wave length and a dark calibration image were also taken. All observations were executed as scheduled, and no anomalies were noted. 1.16 Completed FOS/BL 5658 (White Dwarf Calibration) The Faint Object Spectrograph (Blue Side) was used to make absolute sensitivity calibrations of the detectors using standard white dwarf star GD153. The observations were executed as planned, and no anomalies were noted. 1.17 Completed WF/PC-2 5629 (WF/PC-2 Cycle 4 Photometric Calibration Monitor 1C: 4-Chip STD in F170W) The WF/PC-2 was used to make photometric calibration observations of the ultraviolet standard star GRW+70D582. The observations were executed as scheduled, and no anomalies were noted. 1.18 Completed GHRS/1 5542 (GHRS Side One Wavelength (1st Order Gratings): Cycle 4) The High Resolution Spectrograph (Side One) used the spectral calibration lamp (Side Two) to calibrate the Side One characteristics. Notice that the Side Two lamp was used to calibrate Side One. The observations were executed as scheduled, and no anomalies were noted. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 14 Successful : 14 Scheduled Reacquisitions : 34 Successful : 34 2.2 FHST Updates: Scheduled : 48 Successful : 48 2.3 Significant HSTARs: None 2.4 Operations Notes: There were no reported operational problems. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH -END-