README web version of /home/usg/OPS/MTS/readme_xml/readme_77050200
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Medium spectral resolution VLTI/AMBER interferometry of Eta Carinae's
optically thick stellar wind and test of the predicted binary nature at apastron.
Eta Carinae is the dominant star in the extended (approx. 15x10 arcsec), bright
Homunculus nebula. Earlier AMBER observations showed that the AO system is able
to properly operate in spite of the high surface brightness of the Homunculus nebula.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
We would prefer if the observations could be carried out as early in the
semester as possible (i.e. in April or May, if possible), because Eta Car's apastron
passage is in April 2006 (i.e. the separation of the companion and the wind-wind
bow shock is largest at this time), as described in the proposal.
Therefore, April or May would be preferable.
Special Execution Requirements
Special Calibration Information
For each science OB, we offer two calibrator OBs:
For SCI_EtaCar_1, the preferred calibrator OB is CAL_SAO237916_1.
For SCI_EtaCar_2, the prefereed calibrator OB is CAL_HD107446_1.
Alternativelty, for SCI_EtaCar_1, we offer the calibrator OB CAL_HD107446_2, and
for SCI_EtaCar_2, we offer CAL_SAO237916_2.
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 15:40:13 2009
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