README web version of /home/usg/OPS/MTS/readme_xml/readme_81072300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This run is aimed at deep spectroscopy of the host galaxy of GRB 060218.
The aim is to detect the faint emission features produced by Wolf-Rayet stars in
this
host. These features we expect to find around 4842 A (at the redshift of the
galaxy), which is why we pick the 600B grism on the blue-sensitive FORS1.
This is interesting, as this host has an extrenmely low metallicity, at which one
would not expect to find large numbers of WR stars. However, the evolution mechanism
that led to the GRB should also produce an over-abundance of WR stars, which we
aim to measure.
The lines we look for are faint, so we need to go deep. Unfortunately the target
is not
visible for long at low airmass from Paranal. However, the 3.5 hours total of the
OBs in this run should allow us to set a decent limit on the WR star population
also at slighty adverse conditions, which is why we left the observing constraints
relatively wide.
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 15:40:25 2009
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