ASCL.net

Astrophysics Source Code Library

Making codes discoverable since 1999

ASCL Code Record

[ascl:1806.005] Indri: Pulsar population synthesis toolset

Indri models the population of single (not in binary or hierarchical systems) neutron stars. Given a starting distribution of parameters (birth place, velocity, magnetic field, and period), the code moves a set of stars through the time (by evolving spin period and magnetic field) and the space (by propagating through the Galactic potential). Upon completion of the evolution, a set of observables is computed (radio flux, position, dispersion measure) and compared with a radio survey such as the Parkes Multibeam Survey. The models' parameters are optimised by using the Markov Chain Monte Carlo technique.

Code site:
https://github.com/cieslar/Indri
Described in:
https://ui.adsabs.harvard.edu/abs/2020MNRAS.492.4043C
Bibcode:
2018ascl.soft06005C

Views: 3834

ascl:1806.005
Add this shield to your page
Copy the above HTML to add this shield to your code's website.