README web version of /home/usg/OPS/MTS/readme_xml/readme_76033800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
These are AMBER and MIDI observations of the stellar diameter and the
circumstellar environment of the Mira stars S Ori and GX Mon.
Run A consists of AMBER observations. Run A is related with runs B-D,
which are MIDI+UT observations. The remaining OBs of runs A-D shall, if possible,
be
executed within about 1-2 months, and preferably close to mid-February in order
to
meet rescheduled coordinated VBLA observations.
Runs E/F with MIDI+AT observations are fully independent in terms of scheduling.
Any baseline configuration for AMBER is equally useful.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Run A is related with runs B-D, which are MIDI+UT observations. The remaining
OBs of
runs A-D shall, if possible, be executed within about one month, and preferably
in mid-March
in order to meet re-scheduled coordinated VLBA observations (obtained on March 12).
Any baseline configuration is eqaully useful !
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 15:40:09 2009
If you have comments, please contact usd-help@eso.org