README web version of /home/usg/OPS/MTS/readme_xml/readme_79012100
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
In this run we intend to spatially resolve circumstellar matter around
stars which show circumstellar silicate emission (spectroscopically
detected). We further submit low-res spectroscopy OBs for one target
that has not yet been studied spectroscopically. While the four
different spectroscopic settings can be obtained at different times,
the corresponding STD for each setting must be acquired together with
the target.
Target brightness in general (from IRAS):
0.9 Jy < N < 7.2 Jy
1.7 Jy < Q < 5.5 Jy
Guiding:
Guide stars were selected with the guidecam tool. Only for CD-43 344
there is a potential problem: The selected (only one feasible) guide
star may marginally vignet a corner of the VISIR detector. Please
check whether the guide star list available at the telescope contains
any alternatives. No problems for all other targets.
Standard star (for spectroscopy):
HD 145897 is from the "selected list of 12 standard stars from Cohen"
which are frequently used for VISIR. We therefore consider it not
necessary to submit a finding chart for this well known target.
In case of any eventual problems, please contact the PI. Thank you.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Some info about target acquisition and finding charts:
The finding charts (FC) are a best effort, but for most targets
high-resolution IR imaging has not been obtained before. Note that
often more than one FC is attached (with different FOVs and different
wavelengths).
- HD 123356: We aim at imaging the component HD 123356 _B_, which is
already in the NIR the brighter star. In the MIR it will be the
dominant source of emission.
- HD 143006: This target is expected to be the only source in the
field (see TIMMI2 finding chart).
- V1045 Sco: Other FC than a 2MASS K-band could not be found. In the
MIR the target will be the brightest source in the field.
- HD 190073 and CD-43 344: Brightest source in the field.
- HD 145897 is from the "selected list of 12 standard stars from Cohen"
which are frequently used for VISIR. We therefore consider it not
necessary to submit a finding chart for this well known target.
Beside of finding charts, we further verified with the IRAS PSC that
our targets are always the brightest 12-micron source in a field
sufficiently larger (10') than the VISIR FOV.
In case of any eventual problems, please contact the PI. Thank you.
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 ?
If the provided finding chart is at a different wavelength than the observations,
did you clearly describe in the README file how to identify the target?
Did you specify a guide star brighter than V=12mag within a field of
r=5arcmin around the science target?
Last creation of page: Tue Oct 6 15:40:18 2009
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