README web version of /home/usg/OPS/MTS/readme_xml/readme_79056900
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
High resolution spectroscopy of the M8/T6 binary SCR 1845. The binary
is separated by ~1" at a position angle of ~184 in May 2007. The precise orientation
of the binary axis should be checked before the exposure since orbital motion during
one year is significant and only extrapolated to May 2007.
The goal of the observation is the determination of the relative radial velocities
of both components. Hence, the position of the objects with respect to the slit
is very important and should be carried out at sub-pixel level. Very useful in this
context are the slit viewer images after alignment since they can be used to determine
the relative positions of both componenets in the slit. Ideally, slit viewer images
should be recorded regularly during the observations.
Each object OB should be followed by an OB for the telluric calibrator.
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 15:40:19 2009
If you have comments, please contact usd-help@eso.org