README web version of /home/usg/OPS/MTS/readme_xml/readme_79076200
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We aim to spatially resolve the circumstellar material around the Herbig
Be star V921 Sco. By using AMBER's medium resolution mode, we want to measure the
visibility not only in the continuum, but also in the Brackett-Gamma emission line
at 2.166 micron.
Besides the standard calibrator HD141687 (K=4.4; at earlier right ascension than
the science target), we have prepared OBs for an alternative calibrator at later
right ascension (HD163197, K=3.9). The calibrator HD141687 (K=4.4, V=6.6, G5II/III,
UD-diameter=0.649+/-0.045 mas) is not in the CalVin list, but was selected using
Aspro.
For the V921Sco OBs, we specify three science templates (3 x AMBER_3Tstd_obs_1row)
each with the same spectral window (2.12-2.20 micron, containing the BrGamma line).
This way, we would like to obtain an increased number of recorded interferograms
in order to allow data selection and to increase the SNR in the derived visibilities
and phases.
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 15:40:20 2009
If you have comments, please contact usd-help@eso.org