README web version of /home/usg/OPS/MTS/readme_xml/readme_77051400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This programme looks at the large scale (i.e. extended over several arcsec)
kinematics in a few AGN for which we also have adaptive optics data. The features
of interest are the H2 1-0S(1) line at 2.12microns and the CO bandheads longward
of 2.3microns - with which we can trace the velocity and dispersion of both the
gas and stars.
Because the extended emission is faint, we need to integrate for relatively long
times (although the AGN itself is rather bright).
And because we are interested in stellar kinematics, it is necessary to observe
some velocity standards (i.e. the HD* targets, which also need their own telluric
standards).
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Because there are 4 OBs for each galaxy (covering 2 wavelength settings
at 2 position angles), it would be preferable to complete all OBs for each galaxy
before moving on to the next.
It is also important that at least 1 of the HD* velocity standard sars is observed.
However, the integration time on these is not important, and I would be happy for
the Service Observer to adjust it if necessary (e.g. saturation, etc).
The user priorities have been set to reflect these wishes.
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 you submitted OBs for standard stars, did you use the provided StandardStar
templates ?
If you are using a specific offset pattern or position angle, did you
check carefully the definition in the manual ?
If you are doing spectroscopy, did you draw the slit on the Finding Charts
?
Did you enter the magnitude of the brightest star in the field-of-view
in the 'Instrument Comments' field of each OB ?
If you use the MoveToPixel acquisition, have you given clear instructions
on the FC and in the OB comment section as to how the field should be centered ?
Last creation of page: Tue Oct 6 15:40:13 2009
If you have comments, please contact usd-help@eso.org