| DDT |
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:
This programme should be executed before mid of August
Abstract for MTS:
This is a simple LSS programme that attempts to recover an old supernova.
The target is very faint and not visible in the acquisition and through slit image.
The acquisition is done via a blind offset from a reference star. Note that the
user has rotated the instrument so that both the SN position and the reference
target will be in the slit once the rotation is done.
The programme is composed by 3 OBs, which are practically identical. Only the
offset pattern is slightly different. Each OB takes 3x15 minute spectra.
OB execution is totally independent and the OBs do not need to be executed in arow, even though this might save some time to the night astronomer.
The user requires airmass lower than 1.3. Given the coordinates of the target, this gives more than 3 hours per night if the OBs are executed before mid of August.
README of this run:
Web version of approved README readme_75503900.html