|
|
PIPE2D-82
|
PIPE2D-10
Turn on applying flats in IsrTask
|
aritter
|
swinbank
|
|
Won't Fix |
Won't Fix
|
|
|
|
|
|
|
PIPE2D-81
|
PIPE2D-10
Design access mechanism, dataset types for accessing flats from Butler
|
aritter
|
swinbank
|
|
Done |
Done
|
|
|
|
|
|
|
PIPE2D-80
|
PIPE2D-10
Task-ify code for creating normalized flats
|
aritter
|
swinbank
|
|
Done |
Done
|
|
|
|
|
|
|
PIPE2D-79
|
PIPE2D-10
Compare photometric flats to the output of PIPE2D-78
|
aritter
|
swinbank
|
|
Won't Fix |
Won't Fix
|
|
|
|
|
|
|
PIPE2D-78
|
PIPE2D-10
Use imaging flats to generated dithered spectral flats
|
cloomis
|
swinbank
|
|
Done |
Done
|
|
|
|
|
|
|
PIPE2D-77
|
PIPE2D-10
Make sure there are no systematics in the normalized flat
|
aritter
|
swinbank
|
|
Done |
Done
|
|
|
|
|
|
|
PIPE2D-76
|
PIPE2D-10
Write a brief summary of the approach being taken to flat fielding
|
aritter
|
swinbank
|
|
Done |
Done
|
|
|
|
|
|
|
PIPE2D-75
|
PIPE2D-10
Confirm & supply latest valid amplifier gains & sources thereof
|
cloomis
|
swinbank
|
|
Done |
Done
|
|
|
|
|