First Night Sky Commissioning Run A Success!
LWS had its first night sky testing on the Keck I telescope 31
Oct 1998, Halloween, and 01 Nov 1998. Many of the scheduled
engineering tasks were completed and much progress was made
towards commissioning the instrument. Accomplishments include:
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Optical Alignment of Dewar
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Pointing Model Calibration
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Establish Chopping Operations
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Establish Chop-Nod Operations
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Test Guiding Performance during Chop-Nod Operations
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Test LWS/Guide Camera differential Flexure
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Background Measurements as a Function of Filter
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Instrument Sensitivity
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Acquisition of Primary Mirror Focus Mode Images for Possible MAlign with
LWS
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Detector Temperature Control
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Dewar Hold Time
The run was deemed successful as many goals were
achieved. Of course not all was perfect and few problems
arose. In particular, a baffle in the LHe fill neck designed
to damp out He oscillations became frozen in place on
the second day of the run. The LHe was venting ok and
thus not a safety risk to the instrument or personnel . The
frozen baffle did prevent getting more LHe into the
dewar. Using what LHe remained in the dewar we proceeded with
observing and were able to work for several hours into the
second night. The dewar held for > 30 hours exceeding the 24
hour specification. There were some other problems
encountered include glitches the chop-nod operations.
The next run is scheduled for 02Dec1998 and 03Dec1998.
The frozen baffle problem and chop-nod irregularities will be
among the priority tasks to work on for the next run.
Images and Data From First Commissioning Run
11.7 µm LWS image mosaic of Saturn
This false color image has been enhanced.
Primary Mirror Focus Mode Image Mosaic.
Chop-Nod Guiding Performance.
The Plot shows the X (top) and Y (bottom) centroids on LWS
while tracking a bright source, Beta Peg, for about 1 hour
during transit. Images were written to disk at a rate of 1 Hz
during the acquisition of 4 seperate fits files. The plot
shows a minimum scatter of about 0.1 arcsec with occasional
increases in guide errors possibly due to chop-nod
operations. There is also some longer term errors perhaps
caused by differential flexure between LWS and the guider.
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Last modified: Tue Feb 2 14:45:18 HST