HUBBLE SPACE TELESCOPE

       DAILY REPORT #2977

PERIOD COVERED:  0000Z (UTC) 10/15/01 - 0000Z (UTC) 10/16/01

Daily Status Report as of 289/0000Z

1.0 OBSERVATIONS SCHEDULED AND ACCOMPLISHED:

    1.1 Completed Two Sets of STIS/CCD 8901 (Dark Monitor-Part 1)

        The Space Telescope Imaging Spectrograph (CCD) was used to monitor 
the darks.  There was no anomalous activity.

    1.2 Completed FGS/1 8898 (Calibrating FGS1r's Interferometric Response 
as a Function of Spectral Color)

        Fine Guidance Sensor #1 was used to obtain reference point source 
Transfer Functions {S-Curves} through the F583W filter and the F5ND 
attenuator at the center position of the FGS1r FOV for a variety of stellar 
spectral colors.  The data will be added to the library of point source 
interferograms that was assembled from the Cycles 8 and 9 calibration 
program.  These Transfer Functions are needed to support the analysis of GO 
science data for the study of close and wide binary star systems and for 
determining the angular diameter of extended sources.  The proposal 
completed with no reported problems.

    1.3 Completed Eight Sets of WF/PC-2 9244 (POMS Test Proposal: WFII 
Parallel Archive Proposal Continuation)

        The WF/PC-2 was used to perform a generic target version of the 
Archival Pure Parallel program.  The program will be used to take parallel 
images of random areas of the sky, following the recommendations of the 
Parallels Working Group.  The observations completed with no anomalous 
activity.

    1.4 Completed Two Sets of STIS/CCD 9285 (POMS Test Proposal: STIS 
Non-scripted Parallel Proposal Continuation III)

        The Space Telescope Imaging Spectrograph (CCD) was used to make low 
galactic latitude, non-scripted parallel observations as part of a POMS 
test proposal.  The observations were completed as planned, and no 
anomalies were reported.

    1.5 Completed Four Sets of WF/PC-2 8936 (Cycle 10 Supplemental Darks Pt1/3)

        The WF/PC-2 was used to perform a dark calibration program that 
obtains three dark frames every day to provide data for monitoring and 
characterizing the evolution of hot pixels.  The proposal completed with no 
reported problems.

    1.6 Completed WF/PC-2 9124 (Mid-UV SNAPSHOT Survey of Nearby 
Irregulars: Galaxy Structure and Evolution Benchmark)

        The WF/PC-2 was used to investigate the relation between star 
formation and the global physical characteristics of galaxies to interpret 
the morphologies of distant galaxies in terms of their evolutionary 
status.  Distant galaxies are primarily observed in their rest frame 
mid-ultraviolet.  They resemble nearby late-type galaxies, but are they 
really physically similar classes of objects?  It is proposed to address 
this question through a SNAPSHOT survey in the 2 mid-UV filter F300W of 98 
nearby late-type, irregular and peculiar galaxies.  No problems were reported.

    1.7 Completed STIS/MA1/MA2 9120 (Planetary Nebulae In The LMC: A Study 
On Stellar Evolution And Populations)

        The Space Telescope Imaging Spectrograph (MA1 and MA2) was used to 
investigate the final phase of the evolution of low- and intermediate-mass 
stars, the Planetary Nebula {PN} ejection that is thought to provide the 
main source of carbon and nitrogen enrichment in galaxies.  The 
observations completed nominally with no reported problems.

    1.8 Completed WF/PC-2 8059 (POMS Test Proposal: Targeted Parallel 
Archive Proposal)

        The WF/PC-2 was used to observe the parallel opportunities 
available in the neighborhood of bright galaxies are treated in a slightly 
different way from the normal pure parallels.  Local Group galaxies offer 
the opportunity for a closer look at young stellar 
populations.  Narrow-band images in F656N can be used both to identify 
young stars via their emission lines, and to map the gas distribution in 
star-forming regions.  The observations completed nominally.

    1.9 Completed STIS/MA2 8920 (Cycle 10 MAMA Dark Measurements)

        The Space Telescope Imaging Spectrograph (MA2) was used to perform 
the routine monitoring of the MAMA detector dark noise, and is the primary 
means of checking on health of the MAMA detectors systems through frequent 
monitoring of the background count rate.  The proposal completed with no 
reported anomalous activity.

    1.10 Completed WF/PC-2 8939 (Cycle 10 Internal Monitor)

        The WF/PC-2 was used to calibrate the internal monitor, to be run 
weekly to monitor the health of the cameras.  No problems were encountered.

    1.11 Completed STIS/CCD 8617 (Ultraviolet Spectroscopy of Hot 
Horizontal-Branch Stars in the Globular Cluster M13)

        The Space telescope Imaging Spectrograph (CCD) was used to observe 
blue horizontal-branch {BHB} stars in the metal-poor globular clusters M13, 
M15, NGC 288 and NGC 6752 that have recently been found to exhibit 
remarkable metallicity enhancements and helium depletions relative to the 
canonical cluster composition.  These abundance anomalies are most likely 
due to diffusion processes -- radiative levitation of the metals, and 
gravitational settling of helium --- in the stable radiative atmospheres of 
these hot stars.  With available ground-based facilities, we have observed 
stars in M13 as hot as 19000 K, but beyond this point we are constrained by 
low V- and B-band flux and an insufficient number of visible-wavelength 
spectral lines.  There were no reported problems.

    1.12 Completed Five Sets of WF/PC-2 8935 (Cycle 10 Standard Darks)

        The WF/PC-2 was used to obtain dark frames every week in order to 
provide data for the ongoing calibration of the CCD dark current rate, and 
to monitor and characterize the evolution of hot pixels.  Over an extended 
period these data will also provide a monitor of radiation damage to the 
CCDs.  The proposal completed with no reported problems.

    1.13 Completed STIS/CCD 8903 (Bias Monitor - Part 1)

        The Space Telescope Imaging Spectrograph (CCD) was used to monitor 
the bias in the 1x1, 1x2, 2x1, and 2x2 bin settings at gain=1, and 1x1 at 
gain = 4 to build up high-S/N superbiases and track the evolution of hot 
columns.  There were no problems.

    1.14 Completed WF/PC-2 9045 (The Relationship Between Radio Luminosity 
and Radio-Loud AGN Host Galaxy Properties)

        The WF/PC-2 was used to determine the relationship between the 
properties of the host galaxies of radio-loud AGN and their radio 
luminosities.  Previous studies in this area with the HST have concentrated 
on the 3C sample which shows a tight correlation between luminosity and 
redshift, such that evolutionary effects cannot be distinguished from those 
depending upon radio luminosity.  Our sample of 46 radio galaxies at z ~ 
0.5 comes from four complete, low-frequency-selected samples of radio 
sources with differing flux limits.  Thus the total sample spans an 
unprecedented three orders of magnitude in radio luminosity at a fixed 
redshift interval.  The proposal completed with no reported problems.

    1.15 Completed STIS/CCD 8669 (Merger-Driven Evolution Of Galactic 
Nuclei: Observations Of The Toomre Sequence)

        The Space Telescope Imaging Spectrograph (CCD) was used to observe 
galaxy mergers that are believed responsible for triggering starburst and 
AGN activity in galaxies, and even perhaps transforming spiral galaxies 
into ellipticals.  The proposal completed nominally.

    1.16 Completed Three Sets of WF/PC-2 8941 (Cycle 10 UV Earthflats)

        The WF/PC-2 was used to monitor flat field stability by obtaining 
sequences of earth streak flats to improve the quality of pipeline flat 
fields for the WFPC2 UV filter set.  The proposal had no problems.

    1.17 Completed Two Sets of STIS/CCD 9088 (Next Generation Spectral 
Library of Stars)

        The Space Telescope Imaging Spectrograph (CCD) was used to produce 
a "Next Generation'' Spectral Library of 600 stars for use in modeling the 
integrated light of galaxies and clusters by using the low dispersion UV 
and optical gratings of STIS.  The library will be roughly equally divided 
among four metallicities, very low {Fe/H < -1.5}, low {-1.5 < Fe/H < -0.5}, 
near-solar {-0.5 < Fe/H < 0.1}, and super-solar {Fe/H > 0.1}, well-sampling 
the entire HR-diagram in each bin.  Such a library will surpass all extant 
compilations and have lasting archival value, well into the Next Generation 
Space Telescope era.  No problems occurred.

    1.18 Completed STIS/CCD 9187 (A Lyman Limit Snapshot Survey: The Search 
for Candidate D/H Absorbers)

        The Space Telescope Imaging Spectrograph (CCD) was used to measure 
D/H in gas clouds seen against background QSOs.  This provides a unique and 
fundamental cosmological probe of the baryonic density parameter.  To date, 
most of the QSO absorption line D/H constraints have been derived at high 
redshift.  In this proposal the proposers investigate a lower redshift 
range, because there are two potentially crucial advantages to be gained by 
carrying out D/H measurements at intermediate redshift.  First, the 
background of HI forest lines is lower and contamination of the DI feature 
is significantly reduced.  Second, a far larger sample of very bright QSOs 
exists.  There were no reported problems.

2.0 FLIGHT OPERATIONS SUMMARY:

    2.1 Guide Star Acquisitions:
       Scheduled Acquisitions:  7
Successful:  7

  Scheduled Re-acquisitions:  8
Successful:  8

    2.2 FHST Updates:
Scheduled: 13
Successful: 12

        Per HSTAR 8368, the roll delay update scheduled for 288/124809Z 
failed due to the error box results for tracker #3.  The subsequent two 
full maneuver updates and acquisition were successful.

    2.3 Operations Notes:

        Using ROP SR-1A, the SSR EDAC error counter was cleared three times.

       The engineering status buffer limits were adjusted twice per ROP DF-18A.

        The HST ephemeris table was uplinked at 289/0301Z as directed by 
ROP DF-07A.

        SSA transmitter #2 was turned on and off from 289/0710Z to 
289/0746Z per ROP IC-2.

3.0 SIGNIFICANT FORTHCOMING EVENTS:

        Continuation of normal science observations and calibrations.

/CAW