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Time Critical |
Last update of this page: Tue Jul 29 15:41:14 2008
Run State: COMPLETED
USD review status:
O.K.!
| Pre-Imaging? | Special-Calibration? | Time-Critical? | ToO/GTO/Large program? | Carry-Over? | |
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Special Remarks:
RR Aql observations preferred in July to meet concurrent VLBA observations.
Abstract for MTS:
AMBER observations in MR mode with 1 wavelength setting of the Mira star RR Aql and the supergiant AH Sco. There is one observation per target. The RR Aql observation shall be carried out in approximately in July to match re-scheduled concurrent MERLIN and VLBA observations, and is followed by a second epoch of this target in run B. The AH Sco observation is not time critical, and can be executed any time during the period. The visibility on the long baseline will be low, but experience from P76 has shown that fringes of similar correlated magnitude and visibility value can be tracked, plus this baseline is bootstrapped by the two shorter baselines, i.e. fringes shall be searched on UT1-2 and UT2-3.
README of this run:
Web version of approved README readme_77063000.html