README web version of /home/usg/OPS/MTS/readme_xml/readme_82062600
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
The goal of our CRIRES observing program is to obtain high-quality (R
~ 50000, S/N ~ 200) K-band spectra of our targets in order to derive F abundances
from the R9 HF feature at 2.3358 microns. The instrumental set-up we have described
in the attached OBs will place this feature on the second ccd, where according to
the CRIRES ETC signal is maximized. We request that a telluric standard be observed
after each science object OB, and OBs for suggested telluric standards have been
included. There are three stars (HE 0253-6024, HE 0520-5012, G 77-61) for which
the total execution time required to achieve S/N ~ 200 is greater than 1 hour, so
two OBs have been generated for these stars. Similarly, two OBs for the associated
telluric standards have also been generated.
Waiver Requests
Three Waiver Requests (WaiverID: 082.D-0626A.01) have been approved for
our program. The initial Waiver Request was submitted on 23 July 2008, which was
acknowledged on the same day. Two of the requests- to use AO and to use a free
wavelength setting (lambda_ref = 2350 nm and order = 24)- were approved on 24 July
2008. The third request- to include an additional target in our target list, the
extra time gained from using AO in our observations- was re-requested through the
programme change request web form on 24 July 2008. Approval of our target addtion
request was granted on 27 July 2008.
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 15:40:27 2009
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