README web version of /home/usg/OPS/MTS/readme_xml/readme_77060502
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Supporting spectroscopic monitoring for the interferometric AMBER/VLTI
study of the
circumstellar disk of the Be star delta Sco. Using the self-consistent disk model,
we would like to determine its main geometrical and physical parameters.
The Feros spectroscopic observations to be taken before during and after the AMBER
run
on July 14/15 and 15/16 will provide information about the disk evolution and more
constrains for the modeling.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
The observations are time critical. Of the 9 identical OB, 4 must be executed
during
the interferometric observations, 3 before and 1 after them. In order to achieve
the
maximum coordination with the interferometric observations and needed info on the
evolution of
the circumstellar disk on the appropriate time scale, the following schedule should
be
followed
OB 1: June 13-18
OB 2: June 28 - July 2
OB 3: July 6-8
OB 4: July 14, beginning of the night
OB 5: July 14, end of the night
OB 6: July 15, beginning of the night
OB 7: July 15, end of the night
OB 8: July 21-23
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 set 'New Preset' flag in all acquisition templates to 'True'?
If you use any lamp, did you check that it should never be left on at
the end of any OB?
Last creation of page: Tue Oct 6 15:40:13 2009
If you have comments, please contact usd-help@eso.org