README web version of /home/usg/OPS/MTS/readme_xml/readme_79057600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This project aims to map out the gas and stellar kinematics in the central
region of a few nearby spiral galaxies (mostly Seyfert). The galaxies are known
to have nuclear disks. Based on 2 other objects where we have seen these, they are
expected to be around 0.5-1arcsec (50-100pc) diameter. We will use the kinematics
and distributions of the gas and stars measured to determine the properties of these
disks (i.e. size, mass, age of star formation, etc) and their likely influence on
fuelling the central supermassive black holes.
The K-band view of each target is dominated by the nucleus - which on seeing-limited
scales is single. Please centre the nucleus in the field of view each time.
For each target there are 3 OBs, each with 40mins on source. While the emission
lines are likely to be quickly visible, long integrations are needed to reach sufficient
signal-to-noise to measure the kinematics of the stellar absorption features.
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 15:40:19 2009
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