v0.7.2

This is a supplementary package for pyglotaran with convenience plotting functions.

This minor release is specifically intended to cater to the needs for some new (complex) case studies in the form of so called STAR protocol papers, for which the accompanying repositories can be found here:

• pyglotaran STAR protocol for analysis of transient absorption spectra of photosystem I
• pyglotaran STAR protocol for analysis of time-resolved fluorescence spectra of photosystem I

For use with the pyglotaran package, pyglotaran version v0.7.2 or later is recommended.

Can be installed as a python package from PyPI via pip, from Anaconda's conda-forge using conda, or directly from sources on github.

What's Changed

• 🧰👌 Switch tooling to ruff by @s-weigand in #197
• 🩹 Fix crash when plotting spectral model result by @s-weigand in #200
• 🧰 Use black-pre-commit-mirror for 2x speedup by @s-weigand in #205
• 🧰🚀 Use ruff for formatting by @s-weigand in #214
• 👌 Use weighted residual instead of residual plots if present by @s-weigand in #216
• 👌 Add color map arguments to plot_data_overview by @s-weigand in #217
• 👌 Add das_cycler and svd_cycler to plot collection functions by @s-weigand in #218
• 👌 Add use_svd_number switch to use SV number instead of index as label by @s-weigand in #219
• 🩹 Fix use_svd_number not being passed on to plot_sv_data in plot_data_overview by @s-weigand in #221
• 📦 Use trusted publisher workflow for publishing to PyPI by @s-weigand in #222

Full Changelog: v0.7.1...v0.7.2