README web version of /home/usg/OPS/MTS/readme_xml/readme_77006103
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
MIDI observations of OH/IR stars have 2 complications:
1) no visual counterparts => coude guiding on off-axis source and blind acquisition
(finding charts are provided in optical, also showing the guide star, and in K).
The guide stars may be too faint; Please switch to Guide star: NONE mode for both
science target and associated calibrator if the guide stars I found are too faint
2) deep silicate absorption in all objects but WX Psc => only significant flux
at 8 and 13 micron, but not in between.
strategy: some rough earth-rotation-synthesis. LST constraints are entered such
that different projected baselines are obtained, but the observer may deviate from
these intervals, as long as the different projected lengths are guaranteed (different
angles will be obtained with a perpendicular UT baseline)
Thanks, I know these are not trivial observations!
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Is this a Pre-imaging run ?
Pre-imaging Requirements
Source(s) of Pre-imaging
Pre-imaging sources not listed above
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
If this is a pre-imaging run, did you select PRE-IMAGING for the Observing
Category for each Observing Template ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
Did you indicate for each science star OB the corresponding calibrator
star OB (and vice versa) in the 'Instrument Comments' field ?
If you use calibrator stars which are not in the CalVin database, did
you specify their characteristics in the README file and in the OBs ?
Last creation of page: Tue Oct 6 15:40:12 2009
If you have comments, please contact usd-help@eso.org