commit c3cd02a9f5355a646021a7299ea8bb26d892e55f
parent 7de48cec74832cd5021cc51828398e16586911b3
Author: Nicholas Farrow <nicholas.w.farrow@gmail.com>
Date: Tue, 30 Apr 2019 21:55:50 +1000
Update README.md
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1 file changed, 2 insertions(+), 2 deletions(-)
diff --git a/README.md b/README.md
@@ -1,5 +1,5 @@
# The mass distribution of Galactic double neutron stars
-See [Farrow et al. (2019)](https://iopscience.iop.org/article/10.3847/1538-4357/ab12e3/meta) for details.
+We highly recommend reading [*The Mass Distribution of Galactic Double Neutron Stars*; (Farrow, Zhu, & Thrane 2019)](hhttps://iopscience.iop.org/article/10.3847/1538-4357/ab12e3/) for details along with this demonstraion.
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.
@@ -7,7 +7,7 @@ You can take a look at the [demo here](https://github.com/NicholasFarrow/Galacti
`git clone https://github.com/NicholasFarrow/GalacticDNSMass`.
-We highly recommend reading [*The mass distribution of Galactic double neutron stars*; Nicholas Farrow, Xing-Jiang Zhu, Eric Thrane,](https://arxiv.org/abs/1902.03300) along with this demonstraion.
+
## Requirements
### Without running inference (just demonstration & data analysis):
