Unnamed repository; edit this file 'description' to name the repository.
Log | Files | Refs | README

commit 7de48cec74832cd5021cc51828398e16586911b3
parent d4b1d933d7ddc71de1087fd51c177ea7d48c311f
Author: Nicholas Farrow <>
Date:   Tue, 30 Apr 2019 21:49:29 +1000

Diffstat: | 2+-
1 file changed, 1 insertion(+), 1 deletion(-)

diff --git a/ b/ @@ -1,5 +1,5 @@ # The mass distribution of Galactic double neutron stars -See [Farrow et al. (2019)](Farrow et al 2019) for details. +See [Farrow et al. (2019)]( 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.