README web version of /home/usg/OPS/MTS/readme_xml/readme_77052101
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
MIDI observations of three Young Stellar Objects.
We want to obtain three visibility points per target. With these observations we
want to measure the 10 micron silicate bump arising from the surface of the
rotating disks around the three sources. Comparing these observations with
the UVES spectra (run A) will allow us to study the thermal coupling state
of the gas and the dust in the proto-planetary disks.
Since some targets might be too faint for fringe detection in the requested mode,
a more sensitive mode is authorized if no fringe can be dedected.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Due to the time variability of the sources emission the MIDI observations
need to be carried out quasi-simultaneously to the UVES observations (run A).
These MIDI OBs need to be carried out within 3 or 4 weeks from the UVES OBs whose
name is labelled with "B1". Namely:
This run should be excecuted within 3 or 4 weeks from the following UVES OBs (run
A):
HD101412_UVES_B1_0, HD101412_UVES_B1_90,
HD135344_UVES_B1_0, HD135344_UVES_B1_90,
HD179218_UVES_B1_0, HD179210_UVES_B1_90.
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 15:40:13 2009
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