HUBBLE SPACE TELESCOPE

       DAILY REPORT #3064

PERIOD COVERED:  0000Z (UTC) 02/25/02 - 0000Z (UTC) 02/26/02

Daily Status Report as of 057/0000Z

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 Three Sets of WF/PC-2 8937 (Cycle 9 Supplemental Darks pt2/3)

        The WF/PC-2 was used obtain three dark frames every day to provide 
data for monitoring and characterizing the evolution of hot pixels.  No 
problems were encountered.

    1.3 Completed Three 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.

    1.4 Completed Five Sets of WF/PC-2 9318 (POMS Test Proposal: WFII 
Parallel Archive Proposal Continuation)

        The WF/PC-2 was used to perform the generic target version of the 
WFPC2 Archival Pure Parallel program.  The program was used to take 
parallel images of random areas of the sky, following the recommendations 
of the Parallels Working Group.  There were no reported problems.

    1.5 Completed Two Sets of STIS/CCD 9317 (Pure Parallel Imaging Program: 
Cycle 10)

        The Space Telescope Imaging Spectrograph (CCD) was used to perform 
the default archival pure parallel program for STIS during cycle 10.  There 
were no reported problems.

    1.6 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.

    1.7 Completed STIS/MA2 8590 (UV Imaging and Spectroscopy of Luminous 
Blue Compact Galaxies from z=0 to z=1)

        The Space Telescope Imaging Spectrograph (MA2) was used to observe 
two well-defined samples of low-mass starburst galaxies, one in the local 
universe {z<0.1} and another at intermediate redshifts {0.2 < z < 
0.7}.  Both samples show optical sizes, morphologies, emission line widths, 
and luminosities comparable to those of LBGs at z=3, and are therefore 
probably the best local analogs and testbeds for further study of 
LBGs.  Our main goals are to: {1} explore the morphologies, surface 
brightness distributions, and half-light radii of nearby starforming 
galaxies in the FUV, near Ly-alpha; {2} search for systematic differences 
among UV, optical, and near-IR morphologies and structural parameters; {3} 
investigate the intrinsic emission and absorption spectra near Ly-alpha of 
starbursting dwarf galaxies, with special attention to Ly- alpha profiles 
and interstellar and stellar photospheric absorption from Si II, O I, C II, 
Si IV, and C IV; {4} measure their FUV-optical colors and dust extinction 
properties; and {5} test the hypothesis that low-mass starbursts are the 
local counterparts of LBGs.  The observation completed normally.

    1.8 Completed STIS/MA2 9573 (NUV-MAMA Daily Dark Monitor)

        The Space Telescope Imaging Spectrograph (MA2) was used to perform 
daily monitoring of the NUV MAMA detector dark noise in order to monitor 
the effects of thermal changes on the NUV dark rate.  No problems occurred.

    1.9 Completed STIS/CCD/MA1 9054 (Star Formation Triggers and Chemical 
Reprocessing in I Zw 18)

        The Space Telescope Imaging Spectrograph (CCD and MA1) was used to 
observe I Zw 18, a blue compact galaxy {BCD} with the smallest known 
abundance of heavy elements yet observed.  No anomalies were reported.

    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 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.

    1.12 Completed WF/PC-2 9180 (Gamma-ray Burst Progenitors: Probing Their 
Environment)

        The WF/PC-2 was used to perform a target of opportunity observation 
of gamma ray burster (GRB), GRB-020124.   GRB astronomy is a field maturing 
at a phenomenal rate.  Three important new observational and theoretical 
discoveries, formulated over the last twelve months, allow the proposer to 
address new, and in many cases, more sophisticated questions than could 
have been posed previously.  These developments: the discovery of X-ray 
lines in GRB 991216; the observation that N_H as deduced from X-ray 
afterglow are one to two orders of magnitude larger than the dust 
extinction inferred from optical afterglow; and the growing realization 
that the afterglow emission may exhibit features of dust echoes, appear to 
offer unexpected and new diagnostics that will directly inform us about the 
progenitor, the circum-progenitor material and the immediate interstellar 
environs.  There were no reported problems.

2.0 FLIGHT OPERATIONS SUMMARY:

    2.1 Guide Star Acquisitions:
       Scheduled Acquisitions:  5
    Successful:  5

  Scheduled Re-acquisitions:  9
    Successful:  9

    2.2 FHST Updates:
    Scheduled: 12
    Successful:  9

        As detailed in HSTAR 8509, the tracker 2 and 3 full maneuver 
updates at 057/011102Z and at 057/011347Z failed on tracker 3.  The 
following acquisition at 057/011705Z, however, was successful.  Then, the 
tracker 2 and 3 roll delay update at 057/023508Z also failed due to tracker 3.

    2.3 Operations Notes:

        Using ROP DR-18-A, the CCS limit for SESBSLD was modified twice.

        The flight operations team transferred to the GSFC STOCC at 
056/1530Z in preparation for Servicing Mission 3B.

        The ephemeris table was loaded at 057/0023Z per ROP DF-07A.

        SSR-1 EDAC errors were cleared at 057/0258Z as directed by ROP SR-1A.

3.0 SIGNIFICANT FORTHCOMING EVENTS:

         Servicing Mission 3B, currently scheduled for February 28.

        Continuation of normal science observations and calibrations.

/CAW