README web version of /home/usg/OPS/MTS/readme_xml/readme_83053601
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Low resolution N-band spectroscopy in the 4 wavelength settings 8.5, 9.8,
11.4, 12.4 of the galactic nucleus of NGC 4579 to investigate its complex nature.
Concerning the finding charts: The source is very faint ant will only be visible
on long time exposures. It will appear pointlike and should be the brightest source
in the field of view.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
The telescope guide star is provided in the OB. It fulfills the constraints
given in the guidecam manual of VISIR and is chosen from the UCAC2-catalog. As far
as possible, the telescope operator should use it. For some objects there are 1
or 2 alternative provided guide stars given in the user comments of the according
OB. So please write down in the README notes which guide star was used so that all
subsequent OBs use the same guide star. The telescope operator should check that
the guide star is not changed automatically by the TCS after, for example, an uncompleted
offset. This is necessary to be able to combine data from different OBs.
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 15:40:30 2009
If you have comments, please contact usd-help@eso.org