README web version of /home/usg/OPS/MTS/readme_xml/readme_76055801
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Infrared observations of SN 1987A.
The finding chart is a MASS K-band image. The SNR is located between the two stars
in the middle of the FOV as indicated in the finding chart. A high resolution HST
image is also attached in order to identify the objects in the FOV. We realize that
this will only help a little.
The positions are from HST which is accurate within 0.4", this should be marginally
better than the position given in proposal which was obtained from literature.
We have chosen the parallel mode of the chop/nod, so that the faint extended object
will be added twice the same place on the chip thereby reducing the S/N. Using the
parallel mode forces us to use the larger FOV so that the object is not lost in
the nodding.
All calibrations necessary are included in the calibration plan for VISIR.
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 15:40:10 2009
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