README web version of /home/usg/OPS/MTS/readme_xml/readme_75085003
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This run consists in observing two bright Vega-like stars (alfpsa=hd216956
and zetlep=hd38678) with the VLTI/MIDI instrument in the PRISM mode and with the
UT3-UT4 baseline. High precision measurements are expected. Therefore, sequential
observations of calibrators and scientific target are preferred.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Currently, one calibrated visibility point should be obtained per hour
on a regular basis. The calibrator star acquisition is at least as important as
the scientific target for this program. Therefore, it is preferable -if operations
proceed well- to use two different calibrators instead of one.
For alpha PsA (=alfpsa), the following sequential observing sequence should be preferred
during the allocated 2 hours :
(CalA - Sci-1) - (CalB - Sci-2), where calA=hd218594 & CalB=hd213009
For zeta Lep (=zetlep), the following sequential observing sequence should be preferred
during the allocated 3 hours :
(CalA - Sci-1) - (CalB - Sci-2) - (CalA - Sci-3), where calA=hd36673 & calB=hd36079
if it not feasible, the following is preferred:
1-(CalA - Sci-1) - (CalB - Sci-2)
2-(CalA - Sci-3)
Please try to ensure (at least partly) the sequential execution of the OBs related
to the same target.
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 'User 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 15:40:08 2009
If you have comments, please contact usd-help@eso.org