This release is a pre-release and may not be stable for production use.
UVEX Transients
End-to-end simulations of transients from UVEX all-sky surveys.
UVEX Transients provides spectral and light-curve models for several transient classes (kilonovae, tidal disruption events, luminous fast blue optical transients, supernovae), built on a common cosmologically-aware SED framework, and tools to Monte Carlo sample populations of these transients against a real survey schedule to produce an event catalog of detections.
Installation
pip install uvex-transients
Or install from source:
git clone https://github.com/TransientsExtragalactic/uvex-transients
cd uvex-transients && pip install -e .
Quickstart
The uvex-transients CLI drives the full simulation pipeline (sample events, screen by
magnitude/SNR, run synthetic photometry) from a single YAML config file. Try it against the
bundled configs/quickstart_tde.yaml example:
uvex-transients run configs/quickstart_tde.yaml --out-dir results/quickstart/
See the file itself for what each section does, and uvex-transients --help for every command.
configs/full_run.yaml is a full-scale config covering every registered
transient class at once; run it directly or via make run (see the Makefile --
make help lists every target).
If you'd rather work interactively, notebooks/ has one self-contained, end-to-end
notebook per transient family (kilonovae, TDEs, LFBOTs, Type II supernovae -- IIP, IIP + early
excess and IIb together -- and Type I supernovae -- Ib and Ic); run them with make notebooks or
open them directly in Jupyter.
Full documentation, including the API reference, is available in the docs/ directory.
1 maintainer
Metadata
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Release files for uvex-transients 0.1.0a0
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