README web version of /home/usg/OPS/MTS/readme_xml/readme_78079301
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Follow-up MIDI observations of the Infrared Companion (IRC) of GlassI.
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We would like to increase the uv-coverage we have by 2 additionnal baselines (run
A & B).
Run A uses U1-U2 baseline, and we ask to observe the object as early as possible
in order to get a PA~180 deg. (E of N).
This is the reason why we asked for a small LST-range (7h30-8h30) in order to make
sure to have HA of about -2h (or less).
Run B uses U2-U4 baseline, and there observations close to the meridian (HA~0h,
LST~11h) should be ok in order to get PA~90 deg.
Be aware that GlassI IRC has its primary at ~2.4 arcsec (see NACO 2.17 micron image
in finding chart), PA~285 deg. (E of N), but the IRC should be easily recognised
because much brighter than the primary at 10 micron (this is already the case in
the 2.17 micron
NACO image).
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 ?
Did you check that your chosen calibrator is bright enough for the instrument
mode used ?
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 15:40:17 2009
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