README web version of /home/usg/OPS/MTS/readme_xml/readme_82011301
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Long slit spectroscopy to obtain redshifts and diagnostic spectra for
an unusual class of galaxy that appear to be ellipticals with ultraluminous far-IR
emission.
Spectra need to have good enough S/N not only for z-measurement but also for stellar
population model fitting, so S/N >10 for most of the spectrum is required.
Standard calibration observations will be enough.
The optical (R-band) finders in most cases show the position of the source but are
not deep enough to show the source itself.
The 3.6 micron images show the target sources clearly, lying at the centre of the
20 arcsecond diameter circles at the centre of the finding charts.
The 60s R-band optical acquisition images should be deep enough to show the optical
source matching the 3.6 micron source even for our faintest target (ETC estimates
9 sigma per pixel detection for our faintest target).
The slit should be centred on the source that matches the source at the centre of
the circle in the 3.6 micron images.
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 15:40:26 2009
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