Last update of this page: Wed Oct 7 15:41:04 2009
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:
Take telluric right before or after science OB. Take observations at low water vapour!
Abstract for MTS:
L-band spectroscopy of water and OH emission lines from 8 protoplanetary disks.
A waiver to use free settings with CRIRES was approved.
Each science OB has its corresponding telluric that has to be observed at similar
airmass right before or after the science OB.
Due to strong telluric counterparts of the water lines, please do your best to
observe this programme under dry conditions, i.e. ~< 25% humidity.
Time constraints: observe tn the beginning or end of the night, the RA ~16 hour
targets in the period August 1-September 15, the RA~10 hour targets in June/July,
and the RA ~ 11 hour, DEC ~ -77 targtes at any time.
The target HP Lup is a binary, for which both components should be placed in the
slit. For other binary sources, the brightest component is always the top priority.
README of this run:
Web version of approved README readme_82043200.html