README web version of /home/usg/OPS/MTS/readme_xml/readme_77013700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The aim of this program is to obatin photometric imaging of 22 AGN, using
the high angular resolution capability of VISIR.
The provided finding charts are 2MASS atlas images at 2.2 microns with our science
targets marked by coloured circles. Our targets are all AGN and thus the brightest
sources in the FOV of VISIR when centered on the given coordinates. Furthermore
they can be identified by being situated in the geometrical center of their respective
host galaxy.
Please note that the coordinates given for NGC 1097 slightly differ from those given
in NED or SIMBAD. This is because the latter are actually inaccurate as a visual
inspection of both the 2MASS and SDSS atlases revealed. With the coordinates given
in the OB, acquisition of NGC 1097 should be possible without any problems.
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 15:40:12 2009
If you have comments, please contact usd-help@eso.org