README web version of /home/usg/OPS/MTS/readme_xml/readme_83067000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
K band (2329.3nm) spectra of TW Hya to measure RV. Spectral calibration
will be done with telluric lines. No standard star observation for calibration required.
Total execution time of one OB is 25:38 min (ETC). We need 25 such observations
of TW Hya, spread as evenly as possible over at 10-15 (possibly consecutive) nights
(see time-critical aspects). There are 25 identical OB available for 25 identical
observations.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
The 25 observations of TW Hya shall be spread as evenly as possible over
at least 10 (10-15) nights, which should be consecutive, if possible. Note that
the period of the expected RV variation, which we want to cover as good as possible,
is 3.56 days. Due to the day/night intervals, this cannot be done in less than 7
nights. Ideally, the two observations per night should separated by 4-5 hrs.
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 15:40:30 2009
If you have comments, please contact usd-help@eso.org