README web version of /home/usg/OPS/MTS/readme_xml/readme_78031901
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Star formation at low metallicity: the morphology of young stellar objects
in the SMC
=====================================================================================
Simple imaging of compact red sources from the Spitzer survey (S3MC). The aim is
to improve upon the spatial resolution of Spitzer, and see whether the VISIR images
reveal structure on a scale of 0.3-2 arcsec, and to obtain a photometric measurement
in between the Spitzer 8 and 24 micron photometry.
The findercharts are Spitzer 8 micron images: target is always the bright source
in the centre of the finderchart (marked with a circle) and even brighter in the
PAH2 filter (11.25 micron; 50 mJy or more).
No special calibrations are required (we calibrate the photometry against the standard
calibration plan measurement).
Priorities are based upon target selection for other observing runs.
Guide stars are chosen following the guidelines of GuideCam.
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 15:40:15 2009
If you have comments, please contact usd-help@eso.org