ARPES viewer
Version 1.2.1 (last modified 29 October 2026) — see
CHANGELOG.md for what changed. The version is in
arpes_viewer/version.py and is shown in the main window's title bar and at its foot,
with a link to this repository for bug reports and the latest version
(https://github.com/DingPei1995/ARPES-data-browser). Please quote it when
reporting a bug, and upload the error log with the report (below).
Terms of use. This program is for non-commercial use only (academic research and teaching); any commercial use is not permitted. New and updated loaders cover data from public large-scale facilities (synchrotrons and similar user facilities) only -- formats of individual laboratories' own set-ups are not supported. If you use this program for a paper on ARPES experiments, please cite this repository in its references (https://github.com/DingPei1995/ARPES-data-browser). A paper related to AI that uses this program or its code must first be discussed with the author by e-mail. For collaborations, or questions about the details, contact ding.pei@synchrotron-soleil.fr.
Licence and authorship. Copyright (c) 2026 Ding Pei. Licensed under the PolyForm Noncommercial License 1.0.0; see also NOTICE. This is the author's personal work, developed from the author's own earlier code; no institution funded it. The requirements, design decisions, trade-offs, physics, the testing on real experimental data and the feedback from it (drawing on Phys. Rev. B 103, 245121 (2021) and Phys. Rev. B 95, 125126 (2017)), and the review and acceptance of every change are Ding Pei's; the implementation was assisted by Claude (Anthropic), credited as co-author in the commits.
A Python/PyQt5 program for ARPES data: browse the measurements of a beamtime, open them in their own windows, convert to momentum, cut, fit, process, compare with a band-structure calculation, and lay the results out as a publication figure.
From raw data to a publication figure -- and an AI agent can drive it
These are not real experimental data. Every panel above is made from the program's synthetic demo data (
devtools/demo_data.py): an invented tight-binding toy model -- a triangular lattice, a = 3.3 Å, stacked with c = 6 Å, a few bands with orbital labels and a k_z dispersion -- turned into spectra with a Fermi-Dirac cut-off, the analyser resolution and Poisson counting noise, and written as beamline files. The "calculation" in panel (b) is the same toy Hamiltonian made deliberately 1/0.8 times wider and 50 meV higher, so that comparing it with the "measurement" has something to find. No published data or literature were used to generate them: the model and its parameters are invented, and names such as "Se-pxy" or "1T-TiSe₂-like" are labels for the toy, not a description of a real material. (The only tabulated values in the demo set are the X-ray line energies of its synthetic EDS spectrum, standard emission energies as listed in the X-ray Data Booklet; that spectrum is not part of this figure.)
Example figure 1 in the figure composer (top); the main panel and a Fermi-surface map in momentum, in its viewer (bottom) -- also on the synthetic demo data.
Every step from the files to the finished figure is the program's own, and every step is plain Python that a script -- or an AI agent -- can run, without a screen:
| Step | In the program | In code |
|---|---|---|
| 1. Raw data | the beamline files, as the main panel lists them | arpes_viewer.loader.registry.load(path, entry) |
| 2. To momentum | the Γ-plane Fermi-surface map → k-map | arpes_viewer.tools.momentum.kspace.convert_map(...) |
| 3. The calculation | Calculated bands: a Wannier Hamiltonian; Z and the shift fitted on a cut | BandsDialog.open_file(...), .fit_alignment() |
| 4. Measured vs calculated | constant-energy maps over the calculated contours, coloured by orbital weight (b) | BandsDialog.series_panels(...) |
| 5. 3-D views | the notched cube (a), the stacked contours (c) | VolumeWindow(...).figure_panel() |
| 6. The figure | the figure composer: arranged, lettered, exported as PNG / PDF, saved as .afig with the data and the files it came from |
FigureWindow(...), .arrange(...), .write(...) |
devtools/figure_tests.py is exactly this script -- it writes the demo
files, reads them back, and builds this figure (and its companion, example
figure 2) in under a minute:
python devtools/figure_tests.py out_png/ out_afig/
In the step 3 fit it recovers what was built into the demo calculation (Z = 0.798 ± 0.001 and a shift of −49.8 ± 0.4 meV, against 0.8 and −50 meV).
Why an AI agent can drive it. The computations live in arpes_viewer/tools/,
free of any user interface; the windows can run off-screen
(QT_QPA_PLATFORM=offscreen) and be driven call by call as a user drives
them; each step is documented in the user guide
and in the technical references beside the code; and a saved figure records
the data and the original files behind every panel. So a coding agent given
this repository and a folder of data can be asked in plain words -- "convert
the Γ-plane map to momentum, compare it with the Wannier calculation in
calc/, and make a figure like example figure 1, with constant-energy maps
at E_F, −0.3, −0.6 and −0.9 eV" -- write and run the script, look at the
PNG it made, and refine it, through to a figure ready for a manuscript. The
user guide's worked example
does the same by hand, step by step. As with any analysis, check what an
agent produced before you publish it -- and see the terms of use above for
papers related to AI.
What it does
- Reads SOLEIL ANTARES and CASSIOPEE (including whole folders and the spin end station), ALS MAESTRO, ALBA LOREA, Diamond I05 and I05-1, MAX IV Bloch, Elettra APE, BESSY One Cube / One Square, SOLARIS URANOS, ASTRID2 SGM4, and its own saved format (loading data).
- Shows cuts, Fermi-surface maps, photon-energy scans, spatially resolved scans and spin-resolved curves, each in its own window with linked cursors (the viewers).
- Converts maps and cuts to momentum, photon-energy scans to k_z, with the Brillouin zone drawn over them (§13, §14, §15).
- Analyses: Fermi-edge fits, Fermi-surface correction, MDC / EDC fits, ridge detection, curvature and second derivatives, dichroism, core levels, spin, de-gridding, detector corrections (§7–§24).
- Compares with theory: crystal structures, tight-binding fits, and calculated bands from Wien2k, VASP, Quantum ESPRESSO, Wannier90 and the FPLO + Wannier tools -- along a path, as constant-energy contours on any (hkl) plane, or as a 3-D Fermi surface (§25–§27).
- Makes figures: the figure composer, laid out like a manuscript page, exported as PNG, PDF or SVG, and saved with its data (§28–§30).
- Loses nothing: every derived dataset is autosaved, a crash is recovered from, and long steps show a progress bar (§31).
Installing and starting
Needs Python 3.9+. With pip, which installs PyQt5, pyqtgraph, numpy, h5py and scipy with it:
pip install arpes-viewer
arpes-viewer
(python -m arpes_viewer does the same; for the latest, unreleased
version: pip install git+https://github.com/DingPei1995/ARPES-data-browser.)
Installed this way, the error logs go to ~/.arpes_viewer/error_logs/.
From a downloaded copy of this repository, with those packages installed:
python ARPES_viewer.py
- Windows: double-click
ARPES viewer.pywin this folder: no console window to close by mistake (the output goes to~/.arpes_viewer/launcher.log). - macOS: double-click
ARPES viewer.appin this folder. It finds a Python that has the packages (conda included), remembers it, and says what to install if none has. The first time, if macOS calls it an app from an unidentified developer: System Settings → Privacy & Security → Open Anyway. - No beamtime at hand?
python devtools/demo_data.pywrites the synthetic demo data above todemo_data/(trying it with demo data).
Bug reports
The program saves what went wrong by itself, in
error_logs/errors_<date>_<time>.txt in its folder (in ~/.arpes_viewer/ when installed with pip), and keeps running. With
a bug report on GitHub Issues,
upload that file (drag it into the text box) or paste its text -- the
main panel's foot has Copy the newest error log and Open the error
logs -- and give the version number.
Documentation
- User guide, with screenshots: English · 中文 · Français; as PDF: English · 中文 · Français.
- What changed, and why: CHANGELOG.md.
- Technical references, beside the code they describe -- the formulas,
the file layouts, the assumptions and the tests behind each step:
- Reading data -- every facility's files, the data kinds, adding a beamline, the assumptions the formats force;
- The windows -- the main panel, the viewers, autosave and recovery, long operations;
- Analysis -- what each tool does and what it assumes; the tools ported from the MATLAB programs;
- Momentum conversion -- k conversion, k_z maps;
- Spectra -- core levels, curves, curve fits, spin;
- Processing -- de-gridding, cut arithmetic;
- Figures, export and the experiment log;
- For developers -- the layout of the code, and the
tests (
python -m pytest).
Metadata
Release files for arpes-viewer 1.2.1
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Source distribution (sdist)
| File | Size | Uploaded | Provenance | Actions |
|---|---|---|---|---|
| arpes_viewer-1.2.1.tar.gz | 927.0 kB | With provenance | Details for arpes_viewer-1.2.1.tar.gz |
Built distribution (wheel)
| File | Interpreter | ABI | Platform | Actions Reset |
|---|---|---|---|---|
| arpes_viewer-1.2.1-py3-none-any.whl | Python 3 | none | any | Details for arpes_viewer-1.2.1-py3-none-any.whl |
Total release size: 1.9 MB
Release files / arpes_viewer-1.2.1.tar.gz
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