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Time Critical |
Last update of this page: Thu Jul 24 15:41:18 2008
Run State: TERMINATED/EP
USD review status:
O.K.!
| Pre-Imaging? | Special-Calibration? | Time-Critical? | ToO/GTO/Large program? | Carry-Over? | |
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Special Remarks:
Solar System Targets ! Actual coordinates and diff RA/DEC velocity have to be given to telescopes and delay line.
Abstract for MTS:
MIDI observations in prism/highsens mode of 4 asteroids, all with baseline UT2-3.
There are two observations of 951Gaspra and one on each of the other 3 targets (64Angelina, 234Barbara, and 21Lutetia). IT is preferred that the two observations
of 951Gaspra are executed in a row.
The observations are to be executed at certain date intervals for each target, which
are given in the ReadMe file and the OBs (time intervals).
The ephemeris list coordinates and differential velocity for every 15 minutes
for the required date intervals. Let me remind that the differential velocity from the target field in p2pp are not yet transmitted to telescopes and delay line, so the actual coordinates and diff velocities have to be manually inserted at the telescopes and delay lines.
README of this run:
Web version of approved README readme_76079800.html