README web version of /home/usg/OPS/MTS/readme_xml/readme_82069000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The purpose of these observations is to measure or provide an upper limit
for the sulphur abundance by using the SI lines at 1045nm, for star HE1327-2326.
The OBs FS1..to FS7 are on top priority and should provide each S/N=80. FS8 is on
low priority and should provide S/N=20. We are using standard setting 54/0/n, the
radial velocity of the star is 68 km/s, all the three lines should fall on detector
3 for any observation from January 2009 to March 2009. The vacuum wavelengths of
the three lines are: 1045.8314nm, 1045.9622nm, 1046.2272nm.
There is a single OB for a telluric standard star, star HIP 66657, which should
provide a S/N ratio of 800
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 15:40:27 2009
If you have comments, please contact usd-help@eso.org