README web version of /home/usg/OPS/MTS/readme_xml/readme_76080701
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
These are feasibility observations of globules in Helix nebula
using VISIR.
This region has a high background originated from Helix nebula
itself, although this background would not saturate the detector.
Targets are two globules, namely globule1 and globule3.
Finding charts are shared for these two globules, and north is top
and east is left.
Neither of globules nor nearby stars will not be detected
with acquisitions. Therefore, these are blind observations.
Calibration is standard: as far as there is a calibration
with the same pixel scale and the same filter, there is no specific request.
(note; PI's e-mail address is m.matsuura@manchester.ac.uk, now (July 2005).
After October 2005, this e-mail might not be valid. Please use
alternative e-mail address: mikako@ir.isas.jaxa.jp,
until I get a new e-mail address at new institute.)
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 15:40:11 2009
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