README web version of /home/usg/OPS/MTS/readme_xml/readme_78046400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
LGS-AO assisted SINFONI observations of two galaxy nuclei, NGC2784 and
NGC5846. The IFU should be centered on the target galaxy, as determined during acquisition.
The details of the targets and tip-tilt (TT) sources are as follows:
Target Object Kmag TT Rmag Separation
------- ----------- ------- ----------
NGC2784 12.6 16.0 30"
NGC5846 14.0 15.5 30"
For the second science exposure within an OB, a different return position after
the sky offset has been given for different OBs, to ensure some 'dithering' of the
exposures. The first exposure is always centered on the galaxy, the position being
set by the accuracy of the acquisition.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
If possible, please try to use hot (A/B) main-sequence stars for the telluric
standard that are not binary systems in the SIMBAD database, as this can really
help the data quality.
The calibration OB CAL-M0III-K-0.1_NoAO is a radial velocity template star, Vmag=11.3,
Kmag=6.2, spectral type M0III. The object name is given as its SIMBAD identifier.
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 15:40:16 2009
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