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| author | Thomas White <taw@physics.org> | 2014-11-26 17:33:53 +0100 |
|---|---|---|
| committer | Thomas White <taw@physics.org> | 2014-11-26 17:33:53 +0100 |
| commit | 8c94491c9e941b7e4f645c1d68d90e95c615baae (patch) | |
| tree | f20112e0091c297b352ef8a9161b73f668396557 /version.sh | |
| parent | 1c7d1b67182bf3eb44c6860916c57fd502a10cc8 (diff) | |
Do not predict reflections beyond the resolution limit in the first place
This is significantly faster than predicting to the edge then applying the resolution cutoff.
With the "new" way of estimating the resolution limit, there's no need to integrate first.
Diffstat (limited to 'version.sh')
0 files changed, 0 insertions, 0 deletions