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| subject: | 3\13 Pt-3 HST Daily Rpt No 3319 |
This Echo is READ ONLY ! NO Un-Authorized Messages Please!
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3\13 HST Daily Rpt No 3319
Part 3 of 3
FGS 9603
Monitoring FGS1r's Interferometric Response as a Function of Spectral
Color
This proposal obtains reference point source Transfer Functions
{S-Curves} for FGS1r through the F583W filter and the F5ND attenuator
at the center position of the FGS1r FOV for a variety of stars with
different 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 programs. 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
size and shape of extended sources. This proposal observes stars that
have been observed in previous cycles to check for long term temporal
stability of the FGS1r S-curves. This proposal monitors the cycle 10
calibration the FGS1r Lateral Color response {using stars Latcol-A and
Latcol-B}, as well as calibrates the "Pos/Trans" bias of a star's
position as determined from Transfer mode and Position mode
observations, and finally the shift of a star's centroid when observed
with F5ND relative to that when observed with F583W {the cross filter
shift} is calibrated for the fainter stars in this proposal {stars
brighter than V=8 can not be observed with F583W.}
STIS 9605
CCD Dark Monitor-Part 1
Monitor the darks for the STIS CCD
STIS 9607
CCD Bias Monitor - Part 1
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.
ACS 9673
CCD Daily Monitor
This program consists of basic tests to monitor, the read noise, the
development of hot pixels and test for any source of noise in ACS CCD
detectors. This programme will be executed once a day for the entire
lifetime of ACS
WFPC2 9676
POMS Test Proposal: WFII parallel archive proposal
This is the generic target version of the WFPC2 Archival Pure Parallel
program. The program will be used to take parallel images of random
areas of the sky, following the recommendations of the 2002 Parallels
Working Group.
NICMOS 9702
NICMOS Parallel Thermal Background
NICMOS Camera 2 pure parallel exposures in the F222M and F237M filters
to establish the stability of the HST+NCS+Instrument thermal emission.
This data will be compared against the already available Camera 3
measurements in F222M which show an increased thermal background.
STIS 9706
STIS Pure Parallel Imaging Program: Cycle 10
This is the default archival pure parallel program for STIS during
cycle 10.
FLIGHT OPERATIONS SUMMARY:
Significant Spacecraft Anomalies: (The following are preliminary
reports of potential non-nominal performance that will be
investigated.)
HSTAR 8958: GSacq(3,1,3) results to Finelock Backup (1,0,1). The
GSACQ(3,1,3) scheduled at 072/16:29:36 - 16:36:52
resulted to finelock backup(1,0,1) using FGS#1 due to
scan step limit exceeded on FGS#3. Possible observations
affected: WFPC 218,219 ACS 144. The guide star
acquisition for this observation was non-nominal, further
analysis will determine if a repeat observation is
required. Under investigation.
COMPLETED OPS REQs:
None
OPS NOTES EXECUTED:
1085-0 SSR ENGINEERING DUMP {at} 072/1908z
SCHEDULED SUCCESSFUL FAILURE TIMES
FGS GSacq 08 08
FGS REacq 07 07
FHST Update 14 14
LOSS of LOCK
SIGNIFICANT EVENTS:
Aft Flight Deck Command Dry Run (March 12, 2003) Objectives: To dry
run AFD commands for SM4 to ensure that the CCS verifiers responded
with correct values. This first test is also verifying the SM4 AFD
test procedures and the SOCs scenario files. The test was a partial
success. Testing was delayed by the inability to access the DM14
calibration report from CCSPDT or the legacy DM14 bluebooks from the
web. Everett Pope responded quickly to reload the PDT application on
select SMOR machines before testing resumed. Several mnemonic
conflicts were resolved by the SOC filtering said mnemonics out of
there database during testing. All considered this was a good first
dry run with actions resulting for both teams. SOC and HITT will meet
on Friday to discuss all issues.
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