README web version of /home/usg/OPS/MTS/readme_xml/readme_77048601
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Our programme requests VIMOS/MOS spectroscopy of galaxies in 4 VIMOS fields
in
a ~ 30' x 30' region around a z=0.8 galaxy cluster.
An overall finding chart showing these 4 fields can be found at
http://www.mpe.mpg.de/~milvang/tmp/cl1216_VIMOS_footprints3.ps.gz
In P75 this programme was first approved, as 075.A-0649. Our pre-imaging was
acquired (run A) done and the masks and OBs designed etc., but sadly not a
single MOS OB (run B, 28.4 hours) was ever executed.
In P77 we reapplied and were awarded an almost identical time allocation,
077.A-0486. We have been informed that our P75 pre-imaging can still be used
in P77 and we have not used the 2 hours allocated to our P77 pre-imaging
run, 077.A-0486(A).
Description of our MOS observations, 077.A-0486(B):
For each field we have 4 identical OBs each doing 1 hour 7.5 min of
integration (split in 5 x 13.5 min), giving a total exposure time of 4.5 hour
per field. Each OB has an execution time of 1 hour 43 min, for which we have
a phase 2 waiver. The OBs include night time arcs and flats.
Our targets have total I-band magnitude in the range 19-22. In each quadrant
we have 2-3 reference "slits" (4" x 4" boxes) with stars that were bright but
unsaturated in our 100 sec R-band pre-images. In each OB we give the exact
number of reference slits to look for.
We take 5 exposures (of 13.5 min) at offset positions -1.6 +1.6 -0.8 +0.8 0
arcsec, where 0 is the preset position, to be able to correct for fringing.
The OBs should be observed within 2 hours of culmination. This corresponds to
an airmass below 1.17, but we had to enter 1.1 in the constraints set, since
only 1 decimal was allowed.
We have two night time calibration OBs, called MOS_CAL_*, which
each observes a hot star (spectral type O or B). The OBs include night time
arcs.
The total execution time for the run is 28.5 hours. This is 0.5 hours more
than allocated for this run (run B), but since we will not be using the 2
hours allocated for run A, we hope that this is acceptable. If it is not, one
of our hot star calibration OBs (MOS_CAL_*) that has observations for only one
VIMOS quadrant can be removed. Many thanks.
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
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 specify suitable guide stars for all your OBs using Guidecam
?
Did you check that the chosen guide stars are suitable for all the offset
positions and that they do not produce unacceptable vignetting of the field of view
?
Last creation of page: Tue Oct 6 15:40:13 2009
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