README web version of /home/usg/OPS/MTS/readme_xml/readme_80076000
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Absorption spectra in four wavelength settings.
All science objects in this run are long period variables. The given magnitudes
and
corresponded S/N are thus only estimates.
In allmost all OBs, two science targets are placed in the slit simultaneously.
The target coordinates given in these OBs are the coordinates in the middle between
the two targets.
The SVGS are chosen to be the brightest of these targets while the faintest target
determines the exposure time.
The S/N given in the comment refers to the fainter object, exept in four OBs (listed
below).
NGC 1846 LE 13 + LE 14 OBS-1
NGC 1846 LE 13 + LE 14 OBS-2
NGC 1846 LE 8 + LE 9 OBS-1
NGC 1846 LE 8 + LE 9 OBS-2
(In these OBs the S/N refeers to the brightest target. In all others to the faintest).
S/N are given for each individual wavelength setting and nod position.
In the finding charts the slit orientations are correct but the slit lengths are
46".
All OBs can however be executed in a 31" slit.
The priorities are given under the assumption that priority 1 OBs are executed first.
NEW: The center of slit coordinates of OB's 293753, 293755, 293757, 289692 and
289687 have been adjusted to ensure that both stars fall on the
illuminated part of the science detector. The finding charts for these
OB's have not been corrected for these adjustments and the arrow
indicating the center of slit is therefore slightly ofset with respect to
the coordinates of the OB's.
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