README web version of /home/usg/OPS/MTS/readme_xml/readme_77035001
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The aim of this proposal is to look at the triggered formation of massive
young stellar objects, observed on the borders of Galactic HII regions.
This run contains two parts:
1) Imaging in the PAH2_2 and Q2 bands at several positions towards three different
Galactic HII regions (RCW 79, RCW 82, RCW 120).
At some positions (corresponding to the peak of the 1.2-mm continuum emission, observed
with SIMBA at SEST) no source is visible at 8 microns (at the GLIMPSE detection
limit). The idea there is to look for embedded YSOs that could be seen with VISIR.
On all FCs, the VISIR field centre is indicated by the pink cross
Calibration is needed in the PAH2_2 and Q2 filters
2) Spectroscopy in the 7 - 13 micron range for one red source observed on the borders
of RCW82.
Calibration is needed in the corresponding spectral range
The flux of the source is 0.8 Jy at 8 microns
The guide stars have been choosen using the GuideCam tool with the selection criteria
of both V<=12 mag and r=5arcmin
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 ?
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 15:40:12 2009
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