README web version of /home/usg/OPS/MTS/readme_xml/readme_80073800
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The observations are aimed at spectrally (and eventually spatially) resolving
molecular emission
lines (CO, H2 and H20) around 6 bright pre-main-sequence stars (Herbig AeBe stars).
We want to obtain K- and M-band spectra for 3 stars (51 Oph, HD 58647, HD87643)
in order to study
both the fundamental and first overtone CO emission. For the remaining 3 stars (HD
101412, HD 135344,
HD 179218) we need only K-band spectroscopy.
Correction for telluric absorption and emission is needed and calibration OBs were
created.
The science OBs are named with the prefix "SCI-". The associated calibration OB
is named with the
prefix "CAL-" and equal suffix. A calibration OB consists of a spectrum of an early
type star with the
same wavelength setting of the science OB. Please execute the calibration OB as
close as possible in airmass
to the associated science OB.
All targets are very bright and can be used as AO and SV guide star.
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
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