README web version of /home/usg/OPS/MTS/readme_xml/readme_76060701
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The goal is to get the velocity map and velocity dispersion map of the
lensing galaxy in the Einstein Cross: Q2237+030.
Good image quality is required (We use AO, but natural seeing of 0.5-0.6 (on the
seeing monitor) will translate to 0.3-0.4 in the IR. AO is therefore *NOT* mandatory
to the success of the project as long as the final image quality is below 0.4 arcsec.).
The goal is to achieve images as good as the ones done during on Q2237+030 during
the commissionning of SINFONI (fig. 1 of our phase I proposal) but much deeper,
using the target itself as the AO guide. The spaxel used is always 0.1 arcsec and
the H-band grating.
If the project is started at all, it is estimated that the minimum amount of data
leading to useful science is at least 50% of the total planned exp time (in this
case we will be able to
measure velocities, but no velocity dispersions).
The observations of the two stars HD16640 HD22997 are essential, as velocity calibrators.
Flux calibration is desirable but not mandatory.
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 15:40:10 2009
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