083.B-0265E
Feltzing/ Johnson/ Ad\'en/ Asplund/ Bensby/ Gal-Yam/ Gould/ Lucatello/ Mel\'endez/ Simmerer
UVES
Last update of this page: Wed Oct 7 15:41:04 2009
Run State: TERMINATED/EP_TOO
USD review status:
O.K.!
| Pre-Imaging? |
Special-Calibration? |
Time-Critical? |
ToO/GTO/Large program? |
Carry-Over? |
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|
 |
|
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Special Remarks:
NO REMARKS
Abstract for MTS:
RRM/TOO observations of leansed stars provided by MOA and OGLE.
Triggering observations when UVES red-arm is available
- ToO_BulgeDwarf. ToO OB to be used to observe the lensed star.
Due to the field crowdeness, it is likely that the PI will indicate the PA
in the trigger message.
- ToO_Bstar. ToO OB to be used to observe the telluric standard.
The telluric std should be observed within 2 hours from the science
OB.
- RRM_BulgeDwarf. RRM OB of a lensed star. However, since the PA cannot be
specified in RRM mode, it is unlikely that the PI trigger observations via RRM. The telluric std will be triggered by the ToO OB.
Triggering observations during the red-arm upgrade
- ToO_BulgeDwarf-blue. ToO OB to be used to observe the lensed star.
Due to the field crowdness, it is likely that the PI will indicate the PA
in the trigger messege.
- RRM_BulgeDwarf-blue. RRM OB to be used to observe the lensed star.
- No telluric standard is going to be observed if only the blue arm is used.
Run status page 083.B-0265E
README of this run:
Web version of approved README readme_83026504.html