README web version of /home/usg/OPS/MTS/readme_xml/readme_81038700
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a deep integration of a strongly lensed galaxy at z=3, with a
possible second strongly lensed galaxy within the same field of view at z=2.5. Observations
are very straight-forward, and do not require any special settings. The magnitude
of the offset star is K=15.1, that of the target is fainter than 20 mag. For the
standard star we'd prefer a B star, but would accept any other star if there should
be observational constraints.
The targets are very faint and should appear in the line image after about an hour
of on-source observing time (perhaps even more in case of the Triplet). The Sextet
has a nearby cluster member galaxy which should be partially within the field of
view. This galaxy should be detected signficantly faster, possibly within a single
integration.
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 15:40:24 2009
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