README web version of /home/usg/OPS/MTS/readme_xml/readme_77071900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This programme aims at performing spectrophotometry of small regions suspected
of containing massive YSOs: to detect the embedded YSOs and characterise the immediate
physical conditions.
The finder charts for each target have indicated the (approximate) field centre,
at the first chop position. The finder chart images are 8 micron IRAC/Spitzer images.
It is not known how the images will look like in the VISIR narrow band filters at
much higher spatial resolution.
The telescope angle (tel.rot.offangle) is generally different from the chop angle
(tel.chop.posangle). This is intentional to overcome the complexity of the local
environment and make sure the desired region is properly imaged.
Each target is observed in 4 OBs; the 4 OBs for each target are linked using the
priority settings. It is preferable to complete the 4 OB set for fewer targets than
observe all targets incompletely.
Guide stars have been included in the OBs to make sure that all observations of
the same target are done with the same guide star. The guide stars are the brightest
star (generally brighter than 13 mag), closest to field center (within a few arcmins)
not affected by vignetting.
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 15:40:14 2009
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