README web version of /home/usg/OPS/MTS/readme_xml/readme_78078001
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The observations proposed aim at finding the most embedded population
of stars in regions of recent or on-going high-mass star formation. In the case
of regions sampled by IRAC/GLIMPSE observations (10-70deg on both sides of the Galactic
Centre), the core of emission saturates even 2 second exposures. In this cases,
the VISIR data only samples the brightest area.
We have selected a blind preset Acquisition that shifts the first position to the
South-East corner of the field.
The GenericChopNod template has been used to raster the areas we want to observe,
with a reference position (A) and subsequent nodding offsets that map the region.
Our finding charts show the region to map (continuous red square) and the different
nodding pointings (Bi) required to map with the 32 arcsecs camera field with a throw
of 16 arcsec (yellow points). We have indicated reference chopping position and
first nodding offset pattern (discontinuous squares). An offset of thow/2. has been
added to the pointings. The order of the OB pointings is from east to west and
from south to north.
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 15:40:17 2009
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