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).
For the results of that run, the documentation's report page has a summary of every transient family (kilonovae, TDEs, LFBOTs, Type I and Type II supernovae, SLSNe): its detection funnel, expected number of events and the distributions of the selected events, all built from the data products attached to the latest release.
Full documentation, including the API reference, is available in the docs/ directory.
1 maintainer
Metadata
1 maintainer
Release files for uvex-transients 0.3.0a0
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