68B0366A.html


Last update of this page: Thu Apr 24 17:45:05 2003
Last update of the USG file: Jul 17 09:42:42 2002

Major Instrument Modes: ISAAC SW MR spectroscopy

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? No! Chilean run? No! Special calibrations? No!
Time critical? No! ToO? No! Carry-over run? No!


Special Remarks:


 
 
  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. 


 


Information about the progress of this run:

Run status page 68.B-0366A

README of this run:

68.B-0366A.README