README web version of /home/usg/OPS/MTS/readme_xml/readme_60906200
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Pistol star in the Quintuplet cluster, Galactic Center.
This is the most luminous star known in the Galaxy, and possibly the most massive
(M~150-200 Msun).
We want to test the possibility that it is a binary by tracking spectroscopic signatures
of a companion.
Observation should be done in AO mode, with OB Pistol_NGS (3 settings: 1690, 1737
and 2156 nm)
However, the first attempt (SV #1 August 2006) failed due to the difficulty to find/close
the loop on the faint AO guide star.
If this happens again, non AO observations are possible with the OB Pistol_noAO.
! The region suffers from more than 30 mag of extinction in V ! Hence, the target
CANNOT be used as AO guide star (too faint). This is also why the R and K band images
in the finding chart are so different.
standard star: S/N=80 @ 1698.9 nm; SpTyp=B4V, rangs=B1V-B6V
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 15:40:06 2009
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