README web version of /home/usg/OPS/MTS/readme_xml/readme_79043400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
We aim to measure Sulphur abundance in metal poor stars ([Fe/H]~-2) by
means of multiplet 3 around 1045 nm. Finding charts have been derived from 2MASS
J images with the exception of G186-026 for which a DSS2 Infrared image has been
used, and HD140283 for which 2MASS H image had to be used. Most stars are high proper
motions stars.
HIP28910telluric: HIP 28910 is a telluric line standard. We need for it ONE SINGLE
exposure, if possible taken during the same night as one of the science target.
Concerning the recent discovery of possible vignetting problems in detectors #1
and #4, we confirm that our science is in no way dependent on the spectral coverage
of these detectors, being the features of interest located in detector #2 (around
1045 nm in setting 54/0/i).
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Do the README file and the instrument comments of the telluric stars
OBs include the required S/N/pixel of the spectrum of the telluric star, its spectral
type and allowed spectral range?
Do any OBs include wavelength or flatfield calibrations?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If the slit viewer guide star is different from the target, are the RA
and DEC offsets accurate to within 0.05 arcsec and do they take into account the
relative proper motion between the two objects?
If you have preferences which OBs should be executed first for objects
at similar RA, did you make use of the User Priority field in the OBs?
Last creation of page: Tue Oct 6 15:40:19 2009
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