README web version of /home/usg/OPS/MTS/readme_xml/readme_80062300
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.
EXECUTION CONSTRAINT: Please acquire the telluric immediately AFTER the science
(telluric OB 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 strongly
advisable (best effort basis) to observe both OBs fo a given star the same night.
The sequence should be: Science-1 -- CAL-1 -- Science-2 -- CAL-2.
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.
SPECIAL REQUEST: if the observations are carried out under better conditions, please
start with the fainter objects ( == the ones that will really benefit from better
conditions):
Kmag~7: LSS2063,HD93250, HD93130, HD57582
Kmag~6: HD93129A, HD76341, HD46150, HD54662, CPDm47d2963, muCol, HD73882
WARNING: For the brighest (lamOriA, CAL_muNor) objects, please check that we remain
within the linearity range
TELLURIC: All telluric standards are A0V-A1V star with K<6 and are aimed to be
observed immediately AFTER the science OB (doing it before will not always yield
the expected airmass match). 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 15:40:22 2009
If you have comments, please contact usd-help@eso.org