README web version of /home/usg/OPS/MTS/readme_xml/readme_78064300
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The programme consists of simple UVES observations of the most iron-deficient
star known, HE0107-5240 ([Fe/H]=-5.7), and a comparison star, CD -38 245 ([Fe/H]=-4.0),which
is used as radial velocity standard. The aim of the program is radial velocity monitoring
of HE0107-5240. If the star is a binary, this would have important consequences
for the interpretation of its abundance pattern; i.e., it would be likely that it
is a Population III star.
In order to stay below the maximum execution time of 1h per OB, a 2880s exposure
of HE0107-5240 with the 390+564 setting and a 1'' slit in the blue and 0.6'' slit
in the red arm shall be taken. A 1080s minute exposure of CD-38 245 shall be taken
with the same setting immediately afterwards. We use a 1x1 pixel binning because
we are not readout-noise limited; the reduced spectra will be re-binned by a factor
of 2 in order to increase the S/N.
A ThAr should be taken directly after both observations in order to increase the
radial velocity accuracy, since the expected radial velocity variations are only
of the order of a few km/s.
For avoiding slit losses due to atmospheric differential refraction, the slit is
put to the parallactic angle, and the derotator mode is set to "ELEV" in the OBs.
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 need secondary guiding, are there suitable objects within 30 arcsec
from your target ?
Last creation of page: Tue Oct 6 15:40:16 2009
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