commit 7de48cec74832cd5021cc51828398e16586911b3
parent d4b1d933d7ddc71de1087fd51c177ea7d48c311f
Author: Nicholas Farrow <nicholas.w.farrow@gmail.com>
Date: Tue, 30 Apr 2019 21:49:29 +1000
Update README.md
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# The mass distribution of Galactic double neutron stars
-See [Farrow et al. (2019)](Farrow et al 2019) for details.
+See [Farrow et al. (2019)](https://iopscience.iop.org/article/10.3847/1538-4357/ab12e3/meta) for details.
Here we provide code which performs Bayesian inference on a sample of 17 Galactic double neutron stars (DNS) in order to investigate their mass distribution. Each DNS is comprised of two neutron stars (NS), a recycled NS and a non-recycled (slow) NS. We compare two hypotheses: A - recycled NS and non-recycled NS follow an identical mass distribution, and B - they are drawn from two distinct populations. Within each hypothesis we also explore three possible functional models: gaussian, two-gaussian (mixture model), and uniform mass distributions.
