README web version of /home/usg/OPS/MTS/readme_xml/readme_84063401
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Observations of He I 10830 A emission. The observations are ToO, to be
triggered for when HST observations occur.
Three OBs/sets of TOOs are included in this observation. Each visit includes one
observation of TW Hya (PA=0), a second observation of TW Hya (PA=180), and a telluric
standard (HR4494). This ToO will be activated three different times.
On the finding chart, the target is marked with the red square and the arrow. It's
the only bright star in the area.
Telluric standard should be taken immediately before or after this observation.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
HST will schedule observations during Period 84. We will trigger a ToO
1-2 weeks prior to the observation. The CRIRES observation should occur very close
in time to the HST observation to minimize the effect of variability.
THIS OBSERVATION INCLUDES THREE SEPARATE OBs, TO BE ACTIVATED AT THREE DIFFERENT
TIMES.
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 15:40:32 2009
If you have comments, please contact usd-help@eso.org