HUBBLE SPACE TELESCOPE DAILY REPORT #1812 PERIOD COVERED: 0000Z (UTC) 02/07/97 - 0000Z (UTC) 02/10/97 Daily Status Report as of 041/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed Two Sets of WF/PC-2 6419 (Testing Unified Models With a = Complete Sample of Seyfert Galaxies) The WF/PC-2 was used to make observations of the Seyfert galaxies = ESO-138-G1 and NGC-3516 to help build a complete survey of the Seyfert = class of galaxies. This will help test the current model for Seyfert = class galaxies. This model proposes that all Seyferts have Seyfert-1 = nucleus, which is surrounded by a torus of gas and dust. The observations = were completed as planned and no anomalies were noted. 1.2 Completed WF/PC-2 6119 (Snapshot Survey For Companions of = Planetary Nebula Nuclei) The WF/PC-2 was used to make images of the planetary nebui = NGC-5979 in order to search for companions to its nuclei. The = observations were executed as scheduled, and no anomalies were noted. 1.3 Completed FOC/96 5962 (Young Globular Clusters in Merging = Galaxies: Part III) The Faint Object Camera (f/96) was used to make observations of = two merging galaxies (aka, NGC-4038/4039) in order to study its compact = young blue globular clusters to determine their age, luminocity function, = and physical properties. The observations were executed as scheduled, and = no anomalies were noted. 1.4 Completed Four Sets of WF/PC-2 7553 (Pure Parallel Archive Survey = II) WF/PC-2 parallel observations were obtained in the ultraviolet in = search for interesting objects. This program is designed to find = extragalactic sources with near ultraviolet excesses (3000 A0) outside = the galactic plane and far ultraviolet sources (1600 A0) in the galactic = plane. The procedure was executed as scheduled, and no anomalies were = reported. 1.5 Completed WF/PC-2 6909 (WF/PC-2 Cycle 6 Calibration: Earth Flats The WF/PC-2 was used to make observations of the bright earth to = obtain streak flats which are used to construct high quality flat fields = for the WF/PC-2 filter set. The observations were executed as scheduled, = and no anomalies were noted. 1.6 Completed FOS/BL 6471 (A Bolometric Light Curve For Pulsating = Helium Star LSS3184) The Faint Object Spectrograph (Blue side) make spectrographic = observations of extreme helium, pulsating star LSS3184 in order to study = it bolometric. This star varies in a period of over 2.5 hours, which is = identical to the pulsating helium star V652. The observations were = executed as scheduled, and no anomalies were noted. 1.7 Completed Four Sets of WF/PC-2 6802 (Cosmology with The Medium = Deep Survey) The WF/PC-2 was used to make observations in parallel with the = prime science observations as part of the Medium Deep Survey. These = parallel MDS exposures have provided unique high resolution images which = clearly supplement the primary HST surveys. The observation were = executed as scheduled, and no anomalies were noted 1.8 Completed GHRS/2 6501 (Probing the Equatorial Ejecta of Eta = Carinae) The GHRS remains safed. The low voltage power supply was turned = off at 038/1605Z. No observations were taken. 1.9 Completed WF/PC-2 7203 (Cosmology with the Medium Deep Survey - = Short Orbit Cases) The WF/PC-2 was used to take short (about 20 minute) exposures, to = be taken in parallel with the prime science observations, using the I = filter. These exposures are part of the medium-deep survey, which = emphasizes exposures that will be useful in obtaining cosmological = parameters. The observations were completed as planned, and no problems = were reported. 1.10 Completed Three sets of WF/PC-2 6903 (WF/PC-2 Cycle 6 = Calibration: Decontamination) The WF/PC-2 was used to make several calibration bias = observations, internal flats, K-Spot images and dark calibration images = which are all part of a Cycle 6 decontamination procedure. No science was = interleaved with the dark exposures. The observations were completed as = scheduled, and no problems were reported. 1.11 Completed WF/PC-2 6619 (High Resolution Images of QSO Lyman Alpha = Absorbing Galaxies) The WF/PC-2 was used to make several images of galaxy field (Field = 1427) in order to obtain high resolution observations of the Lyman Alpha = absorbing galaxies within this field-of-view. The purpose is to directly = identify the objects responsible for low and intermediate redshift QSO = Lyman-Alpha systems. The observations were executed as scheduled, and no = anomalies were noted. 1.12 Completed Two Sets of GHRS/1 6760 (The Second Measurement of D/H = in Mars' upper Atmosphere) The GHRS remains safed. The low voltage power supply was turned = off at 038/1605Z. No observations were taken. 1.13 Completed GHRS/1/2 6410 (Low Red Shift Lyman Alpha Clouds: ) The GHRS remains safed. The low voltage power supply was turned = off at 038/1605Z. No observations were taken. Even though the low voltage was powered and no observations were taken, = there was a re-acquisition failed at 039/0738Z which defaulted to RGAs. = See HSTAR 5892. 1.14 Completed 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 object Q0351-390. This is to determine if this high = redshifted object has a far ultraviolet flux. The observations were = executed as scheduled, and no anomalies were noted. 1.15 Completed FOS/BL 6682 (Geometry and Generalizability of the = Reflected Light Model for Seyfert Galaxies) The Faint Object Spectrograph (Blue side) was used to make = spectropolarimetry observations of the Seyfert (class 2) galaxy NGC-5135 = in order to study its geometry and the generalizablity of its reflected = light model. The goal is to determine if the polarization components of = all Seyfert class two galaxies have Seyfert class one characteristics. = The observations were completed as scheduled, and no problems were = reported. 1.16 Completed WF/PC-2 6053 (Extreme UV Stars in Omega Cent) The Faint Object Spectrograph (Blue Side) was used to make = spectrographic observations of extremely ultraviolet bright stars in = NGC-5139 (aka, Omega Cent). These stars were also viewed by the UIT on = ASTRO-1. The observations were executed as scheduled, and no anomalies = were noted. 1.17 Completed Two Sets of GHRS/1/2 6928 (GHRS Far UV Throughput = without Costar Mirrors-Cycle 6 Close-out) The GHRS remains safed. The low voltage power supply was turned = off at 038/1605Z. No observations were taken. 1.18 Completed WF/PC-2 6348 (Blue Continuum Snapshots of 3CR Radio = Galaxies) The WF/PC-2 was used to make some snapshot images of the blue = continuum in radio galaxy 3C469.1. Combined with existing data, these = exposures will provide high spatial resolution information on the color = distribution within galaxies, redding due to dust, spacial indices of the = optical synchrotron jets, and colors of the active nuclei and tidal jets. = The observations were executed as scheduled, and no anomalies were noted. 1.19 Completed WF/PC-2 6942 (WF/PC-2 Camera Electronics) The WF/PC-2 was used to make an observations of giant, elliptical, = galaxy NGC-4472 in order to study the linearity of the camera's = electronics. The observations were completed as planned and no anomalies = were reported. 1.20 Completed WF/PC-2 6902 (WF/PC-2 Cycle 6 Photometric Calibration = Monitor UV/OPT STD) The WF/PC-2 was used to make both ultraviolet and optical = photometric observations of the standard star GRW+70D582 as part of a = Cycle 6 calibration procedure. This observations was done immediately = before and after decontamination procedures. The observations were = completed as planned, and no problems were reported. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions :21 Successful :20 039/0738, HSTAR #5892 was written Scheduled Reacquisitions : 26 Successful : 26 2.2 FHST Updates: Scheduled : 32 Successful : 32 2.3 Operations Notes: The GHRS remains safed. The low voltage power supply was turned = off at 038/1605Z. 3.0 SIGNIFICANT FORTHCOMING EVENTS: SM2 is scheduled to begin tomorrow, Tuesday Feb. 11, with the = launch of the Shuttle at approximately 042/0856Z. /DMH