README web version of /home/usg/OPS/MTS/readme_xml/readme_81085400
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
SCIENCE: HiRes IR spectroscopy of bright (Kmag=3-7) O-type stars.
CRITICAL ASPECT : SNR better than 150 should be reached in all settings (exposure
time computed to reach it under seeing=1.2"--CLR--airmass<1.5). Better SNR will
not arm.
EXECUTION CONSTRAINT: OBs for telluric standard stars have been submitted. Telluric
OBs are identified by CAL_xxxxxx-n where 'xxxxxx' is the name of the science target
and 'n'=1 or 2 according to the list of settings observed. It is advisable (best
effort basis) to observe both OBs fo a given star the same night, or as close as
possible in time. If not possible, please complete one object before starting the
next one.
SCIENCE-TELLURIC SEQUENCE: Given the limited bright A0-1V stars suitable for telluric
correction in that direction of the sky, some of the CAL stars should be observed
*BEFORE* the science for proper AIRMASS MATCH.
TELLURIC *BEFORE* the corresponding SCIENCE OB:
CAL_HD319718A+B-n
CAL_HD167263-n
CAL_HD167771-n
CAL_HD168076-n
TELLURIC *AFTER* the corresponding SCIENCE OB:
CAL_HD151804-n
CAL_HD150958-n
TELLURIC: All telluric standards are A0V-A1V star with K<6. If for any reason
the provided telluric can not be
observed, it can be replaced with a similar type star with similar magnitude as
far as a SNR>150 is obtained in all settings (WARNING=1mag difference will already
required to modified the exp. time compared to the provided target).
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 15:40:25 2009
If you have comments, please contact usd-help@eso.org