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INTRODUCTION
THE OT
Startup Screens
Science Prog Window
Template library
MSBs
Program elements
Use of Inheritance
Constraints
A complete program
The position editor
How to document a program
Observer notes
Typical program setup
Time estimates
Storing programs
Worked example
ADVANCED USAGE NOTES
AND and OR
Drag and Drop
Cloning an MSB
Firewalled ?
Spectroscopy standards
Guide stars and acquisition
RELEASE SPECIFIC NOTES
Site Quality Editor
THE SITE QUALITY EDITOR

The site quality component has a number of sub-frames, for each of the conditions on which the OMP database can filter observations. In these subframes, "Allocated" means "I don't want to specify a limit any more strict than that already imposed by the UKIRT TAG" (if the TAG has done so - this will be outlined in your TAG feedback). Otherwise, enter numerical values for:
  • seeing range (in arcseconds),
  • J-band sky brightness (mag/square arcsecond - note that the number in the "min" box should be larger than the number in the "max" box)
  • tau (for reference, a dry spectroscopic night is currently defined as tau<=0.09 and dry photometric conditions mean tau<=0.15),
and click appropriate buttons in the "moon" and "cloud" boxes. Note that clicking "Thin Cirrus" doesn't mean you require thin cirrus - your observation might get done even in photometric conditions. At present we are not able to explicitly cater for programs which actually need thin cloud cover !






Contact: Andy Adamson. Updated: Mon Jul 16 16:32:42 HST 2007

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