Last update of this page: Wed Jul 23 15:41:25 2008
Run State: COMPLETED
USD review status:
O.K.!
| Pre-Imaging? | Special-Calibration? | Time-Critical? | ToO/GTO/Large program? | Carry-Over? |
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Special Remarks:
NO REMARKS
Abstract for MTS:
In order to determine distances to OB stars in clusters, their stellar types will be determined from H and K spectra. From this, the spatial distribution of Galactic HII regions will be inferred.
One OB often covers several sub-regions of a finding chart, usually all withing 30" distance. In the cases where the AO is used (largest pixel scale for all OBs, nevertheless), the reference star is the R-band brightest target in the area, even though it sometimes looks faint on the K-band FC.
Preference for early A-star tellurics and to have one field finished in H and K before starting another.
README of this run:
Web version of approved README readme_75081200.html