General goal: show ACS images in six bands: U, B, V, R, I, z.
Filter choice for all bands, in ranked order
U
B
V
R
I
z
Line
1st choice
F330W/HRC
F435W/WFC
F555W/WFC
F625W/WFC
F814W/WFC
F850LP/WFC
F658N/WFC
2nd choice
F250W/HRC
F475W/WFC
F606W/WFC
F625W/HRC
F775W/WFC
F850LP/HRC
F502N/WFC
3rd choice
F220W/HRC
F435W/HRC
F550M/WFC
F814W/HRC
F660N/WFC
4th choice
F475W/HRC
F555W/HRC
F775W/HRC
F892N/HRC
5th choice
F606W/HRC
F502N/HRC
6th choice
F550M/HRC
F660N/HRC
General Guidelines
Include all non-solar system objects with a preview which is non-proprietary.
Include Wide Field Channel (WFC) and High Resolution Channel (HRC) data, but do not include
Solar Blind Channel (SBC) observations.
When more than one image with the same filter is available,
pick WFC observations over HRC observations.
Then pick the one with the longest exposure time.
If that includes more than one image, pick the most recent one.
Definition of individual pointing
All observations within 50.5" from a given observing position for pointings based on the WFC
observations and 7" for those based on HRC observations.
Initially all observations for both cameras with in 50.5" of a WFC observation are assigned
a pointing first. All HRC observations within 7" not already assigned to a pointing are then assing4ed to pointings.
Observations of the same area will be more or less at the same observing
position for dithering/cosmic-ray removal purposes.