README web version of /home/usg/OPS/MTS/readme_xml/readme_80061901
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
This is a straightforward spectroscopic program with
two science OBs for observations of the same target
in Chamaeleon using two different wavelength set-ups.
Each science OB has an attached ThAr for
wavelength calibration.
For each science OB, there exist an additional
calibration OB that will observe a telluric standard.
The telluric standard should be observed immediately
after the science exposure.
The two science OBs can be executed independently,
however, the closer in time the better.
I recommend execution in the same night.
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 15:40:21 2009
If you have comments, please contact usd-help@eso.org