README web version of /home/usg/OPS/MTS/readme_xml/readme_84050000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
+ The program aims at observing 3 bright AGN in the Q-band window at 24.36um.
This window contains the [NeV] line which will be used for morphologic and kinematic
studies.
+ All targets are the brightest (and only) objects in the FOV
+ Please make sure that the correct central wavelength 24.36 is set in BOB since
this is non-standard.
+ For each scince target NGC7469, IC4329A, and MCG-3-34-64, we provide a calibrator
star OB which shall be executed before or after the respective sience OB
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
+ For the spectroscopic observations in the 24.36um window, please execute
the corresponding calibrator before or after the science target. Which calibrator
belongs to which target can be identified by the OB names
Science target OB name scheme: SCI_SPC_[Name of target]
Calibrator OB name scheme: CAL_SPC_[Name of target]_[Name of calibrator]
Science calibrator pairs are:
NGC7469 -- HD186791
IC4329A -- HD123139
MCG-3-34-64 -- HD146051
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 15:40:31 2009
If you have comments, please contact usd-help@eso.org