leonarski_fandClaude Opus 4.8
e45a1577d6
Build Packages / build:rpm (ubuntu2404_nocuda) (push) Successful in 13m18s
Build Packages / build:rpm (rocky8_nocuda) (push) Successful in 14m31s
Build Packages / build:rpm (rocky8_sls9) (push) Successful in 14m57s
Build Packages / build:rpm (rocky8) (push) Successful in 14m6s
Build Packages / build:rpm (ubuntu2204_nocuda) (push) Successful in 15m15s
Build Packages / build:rpm (rocky9_nocuda) (push) Successful in 15m23s
Build Packages / build:rpm (rocky9_sls9) (push) Successful in 15m34s
Build Packages / XDS test (neggia plugin) (push) Successful in 8m55s
Build Packages / XDS test (JFJoch plugin) (push) Successful in 9m17s
Build Packages / XDS test (durin plugin) (push) Successful in 9m25s
Build Packages / Create release (push) Skipped
Build Packages / Generate python client (push) Successful in 28s
Build Packages / Build documentation (push) Successful in 57s
Build Packages / build:rpm (ubuntu2204) (push) Successful in 11m31s
Build Packages / build:rpm (rocky9) (push) Successful in 12m45s
Build Packages / build:rpm (ubuntu2404) (push) Successful in 11m44s
Build Packages / DIALS test (push) Successful in 13m3s
Build Packages / Unit tests (push) Successful in 58m30s
Build Packages / build:windows:cuda (push) Successful in 20m21s
Build Packages / build:windows:nocuda (push) Successful in 10m30s
Adds an opt-in smooth absorption correction for rotation scaling. After the rot3d fulls are scaled, --absorption[=num] fits a multiplicative surface A(s1_crystal) - a degree<=4 monomial basis (real spherical harmonics up to l=4, as XDS/DIALS) of the diffracted-beam direction in the crystal/goniometer frame, by ridge-regularized log-linear least-squares of I_scaled/I_ref weighted by (I/sigma)^2, over num iterations (default 3); the surface divides image_scale_corr and the fulls are re-merged. Off by default and a no-op without rot3d. On the test panel (~13 keV, thin crystals) it is metric-neutral - fitted rms(log A) ~3-4%, ISa/CC1/2 unchanged - because absorption is negligible there and the per-frame scale G(phi) already absorbs the angular part. It is kept as a lever for low-energy data (e.g. 6 keV) where absorption becomes significant. Stored as ScalingSettings::absorption_iter. Co-Authored-By: Claude Opus 4.8 (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.