Code to compute scintillation velocity and scintillation arcs from bursts/pulses which are unevenly distributed in time. Applications to Fast Radio Bursts, and certain pulsars (e.g. giant pulse emitters, RRATs))
If you use this code in a publication, please reference https://ui.adsabs.harvard.edu/abs/2022MNRAS.509.3172M/abstract where the code was first used, with a link to this repository.
https://ui.adsabs.harvard.edu/abs/2022MNRAS.509.3172M/abstract https://ui.adsabs.harvard.edu/abs/2023arXiv230414697W/abstract https://ui.adsabs.harvard.edu/abs/2023MNRAS.522L..36M/abstract