68B0366A.html |
RA Range: 0, 5 (SMC, LMC)
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 2.0 4THK 5.0 1.0 30
| Pre-imaging run? |
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Chilean run? |
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Special calibrations? |
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| Time critical? |
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ToO? |
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Carry-over run? |
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Medium-resolution spectroscopy scans across several clusters in the
Magellanic Clouds. Two OBs for each cluster: one with the scans in the H
band, one in the K band. Note that each OB in turn contains several
central wavelength settings (4 in the H band, 3 in the K band).
Constraints relaxed to maximum, transparency relaxed from 3THN in
phase 1 to 4THK in phase 2.
Telescope will spend less than 1 min per position (waiver submitted
and approved). Since the offsets are only 1 sec, it should be no problem for
active optics. Even so, given the relaxed constraints image deterioration
during the exposures can be tolerated.
User-provided priority list in the README file repeated here. Within
each cluster, give priority to H band observations. Although some time
can be saved by observing each object in both setups one after another,
please beware of the calibration needs (7 wavelength setups to calibrate
in that case)
Priority Cluster
==================
1 NGC2002
2 NGC0330
Standard calibration plan is sufficient for this program. No time
constraints.
README of this run: