danielreardon / scintools

Tools for the analysis of pulsar scintillation data
MIT License
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=============================== Scintools

SCINTOOLS (SCINtillation TOOLS) is a package for the analysis and simulation of pulsar scintillation data. This code can be used for: processing observed dynamic spectra, computing secondary spectra and ACFs, measuring scintillation arcs, simulating dynamic spectra, and modelling pulsar transverse velocities through scintillation arcs or diffractive timescales.

=============================== Referencing

If your work makes use of Scintools, please cite Reardon et al. (2020) <https://ui.adsabs.harvard.edu/abs/2020arXiv200912757R> or the Astrophysics Source Code Library record <https://ui.adsabs.harvard.edu/abs/2020ascl.soft11019R> and provide a url link to this github page. If utilising scintools for scintillation timescale, bandwidth, or phase gradient measurements via the autocorrelation function, also cite Reardon et al. (2023) <https://ui.adsabs.harvard.edu/abs/2023arXiv230316338R> . If you use the ththmod.py module, cite Sprenger et al. (2021) <https://ui.adsabs.harvard.edu/abs/2021MNRAS.500.1114S> and Baker et al. (2022) <https://ui.adsabs.harvard.edu/abs/2022MNRAS.510.4573B>_ . If using the electromagnetic simulation software (Simulation class in scint_sim.py), also cite Coles et al. (2010) <https://ui.adsabs.harvard.edu/abs/2010ApJ...717.1206C>_

Below is a list of works that use Scintools\: