README web version of /home/usg/OPS/MTS/readme_xml/readme_75048000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We propose to use TIMMI2 for mapping the dust and gas distribution around
HM Sge in various N band filters, in order to better constrain some characteristic
physical processes of Mira symbiotic systems. In particular, we want to:
- Image a map around the central region, which will be complementary with high-resolution
measurments of the inner structures made with MIDI at the same wavelengths
- compare the size and flux density of the (silicate) dust and of the IR continuum
regions, by measuring them with different spectral filters, respectively centered
before (N8.9), around (N9.8) and after (N12.9) the silicate peak emission wavelength.
The source is fairly bright in the mid-IR (120 Jy) so they should be easily visibile
in the RTD. We've put large chop and nod throws (50 arcsec) so that negative images
fall out of the array, in order to minimize cross-talk and smear-and-stripe patterns.
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 ?
Last creation of page: Tue Oct 6 15:40:07 2009
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