README web version of /home/usg/OPS/MTS/readme_xml/readme_77036201
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Since the original target (GQ Lup) was observed with Spitzer IRS in the
meanwhile, a target
exchange request was sent to USD (support request number 15676). It was approved
to observe
IRAS 10510-5820 instead (presumably a class I source, the next best TTS was observed
with
Spitzer as well...). The N band spectrum is needed to establish its SED and to study
the silicate feature. Gamma Cru shall be observed after the target to get a reference
spectrum.
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 ?
Last creation of page: Tue Oct 6 15:40:12 2009
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