README web version of /home/usg/OPS/MTS/readme_xml/readme_75007400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The intention is to map H_2 emission around the nucleus
of the cooling flow galaxy at the center of Abell 2597. We are interested in
both kinematics and line ratios. There are 4 separate pointings and 4 OBs
per pointing, 1 extra for P3. Finding chart for P2 is mislabelled P1 but is OK
OBs are dithered by 0.25" in RA to account for possible bad pixels.
Each OB consists of 2AB cycles between source and sky with
no jitter because the entire field is full of emission.
Acquisition is on a nearby reference "star" which is actually a small high
surface brightness galaxy. Previous ISAAC experience shows that it is easy
to center on this galaxy.
The sky pointings are about 40" away from the source pointings. There should
be no cluster emission this far away. There is only one finding chart per
OB, showing the 8x8" sinfoni field of view. I don't think a smaller-scale
chart will do much good in acquisition; this must be done by accurate
offsets from the reference "star".
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 ?
Did you indicate the magnitude of the brightest object in the field in
each SINFONI OB?
If you are using the AO: Did you indicate for every OB the magnitude
of the guide star, and its distance to the target (if any)?
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?
Did you make really sure that none of your OBs ever saturates the detector?
If you are using the AO: did you enter the correct Strehl Ratio (on-axis,
K-band) AND the seeing value in the constraint set?
Last creation of page: Tue Oct 6 15:40:06 2009
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