leonarski_fandClaude Opus 5
406c406988
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Each Miller index is bounded by its OWN axis - |h| <= a/d_min, |k| <= b/d_min, |l| <= c/d_min - so a single half-width has to be sized for the longest axis and then walks the short ones far past anything the resolution cut can keep. Give the predictor max_h, max_k and max_l instead, in all four implementations (CPU and GPU, stills and rotation), and derive each from its own axis. On a 149/83/226 A cell that is 23.1M candidates per frame instead of 94.2M, 4.1x fewer. Results are bit-identical, as they must be - the candidates removed are only ones the |q| <= 1/d_min cut rejected anyway: over six rotation crystals every merged observation count, high-shell CC1/2 and space group matches the cube exactly, 6/6 space groups correct. It buys almost no time, and the earlier claim that the cube cost 22% of that crystal's wall clock was wrong. Removing 4.1x of the candidates moves it 1m58s -> 1m57s, so the whole prediction sweep is ~1% of the run. The 22% that crystal costs relative to a fixed max_hkl of 100 is genuine extra work at max_l = 227: real reflections inside the resolution sphere along the long axis, predicted and integrated either way. Per-axis limits do not reduce that and cannot. The user-facing setting stays a single number: it exists to bound the work, not to describe the crystal, and applies to all three indices when set. Co-Authored-By: Claude Opus 5 (1M context) <noreply@anthropic.com>
Jungfraujoch
Application to receive data from the PSI JUNGFRAU and EIGER detectors.
All documentation is now placed in docs/ subdirectory and for the current version hosted on Jungfraujoch Read The Docs page.