README web version of /home/usg/OPS/MTS/readme_xml/readme_75037701
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Goal: measuring the redshift of the lensing galaxy in lensed quasars.
We will use deconvolution techniques in order to remove the spectrum of the quasar
images, using PSF stars. Their centering is as important as the centering of the
quasar itself.
The centering of the quasar is optimized to have the deconvolution procedure to
work well. The centering in the zoomed finding chart IS the correct one. Use the
PSF stars to check that the mask is well aligned, not the quasar itself, because
it has a complex shape, in many cases.
There are 3 OBs per object, each one with 2 times 1400 seconds exposures = 6 x 1400
sec. Some objects have only 5 such exposures.
The minimum useful data to successfully carry out the project is with 2 executed
OBs per object = 4 x 1400 sec.
Note: Please check that the width of all FORS1 slits is the same. We had in the
past some data with slits of different width although this was not specified in
the masks.
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 ?
If you have prepared your finding charts with tools other than FIMS,
do they comply with the specifications on the FORS1 Phase 2 web page ?
Last creation of page: Tue Oct 6 15:40:07 2009
If you have comments, please contact usd-help@eso.org