README web version of /home/usg/OPS/MTS/readme_xml/readme_81009601
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
A spectroscopic observation of AB Dor B. One exposure is taken without
the N2O gas cell, followed by a dithering sequence with the cell. The telluric standard
OB should preferrably be executed directly after the science OB. For a telluric
star, we choose Hip 27534, a B6 star. The SNR should be higher than 100 (this has
been confirmed in the CRIRES ETC).
Both the components of AB Dor B (they can be distinguished in the second finding
chart) should be placed within the slit. Due to the coarse pixel scale of CRIRES,
we expect that this will be difficult to distinguish during operations. However,
from our knowledge of the orbit we beleive that the expected P.A. is sufficiently
well known, and will change sufficiently little during September, that the quoted
P.A. of 285 degrees should work in any case (as long as the observations are indeed
carried out in September).
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 15:40:23 2009
If you have comments, please contact usd-help@eso.org