@@ -26,6 +26,78 @@ A technical note deriving the Monte Carlo sums used to estimate the various prob
...
@@ -26,6 +26,78 @@ A technical note deriving the Monte Carlo sums used to estimate the various prob
*[mmms.pdf](https://git.ligo.org/reed.essick/mmax-model-selection/-/blob/gw-distributions/technical-note/mmms.pdf)(**Update this link once merge request is accepted**)
*[mmms.pdf](https://git.ligo.org/reed.essick/mmax-model-selection/-/blob/gw-distributions/technical-note/mmms.pdf)(**Update this link once merge request is accepted**)
---
## comparison to previous results
Below, we compare results obtained for previous (published) LVK analyses with the output from the new version of the code. We focus on results published as part of the "exceptional event paper" describing the first detections of NSBH systems [[ApJ 915 L5 (2021)](https://iopscience.iop.org/article/10.3847/2041-8213/ac082e)].
Previous results are stored [here](https://git.ligo.org/reed.essick/o3-nsbh-mmax-model-selection/-/tree/master/data) and results obtained with the updated code are stored [here](https://git.ligo.org/reed.essick/mmax-model-selection/-/tree/gw-distributions/test/o3-nsbh/data). **Update link once merge request has been accepted**
Below, I compare the main output of the calculation: the probability that an object is consistent with a NS. Links point to where the (old/new) results are stored. I provide a comparison to all previous results computed for both GW200105 and GW200115.
*[original review used for GW190814](GW190814-Review)
*[updated version used for GW200105, GW200115](General-Review-(post-GW190814))
## library structure
## library structure
### executables
### executables
...
@@ -272,78 +344,6 @@ Declares some basic utilities, including default values and how the results of t
...
@@ -272,78 +344,6 @@ Declares some basic utilities, including default values and how the results of t
---
---
## comparison to previous results
Below, we compare results obtained for previous (published) LVK analyses with the output from the new version of the code. We focus on results published as part of the "exceptional event paper" describing the first detections of NSBH systems [[ApJ 915 L5 (2021)](https://iopscience.iop.org/article/10.3847/2041-8213/ac082e)].
Previous results are stored [here](https://git.ligo.org/reed.essick/o3-nsbh-mmax-model-selection/-/tree/master/data) and results obtained with the updated code are stored [here](https://git.ligo.org/reed.essick/mmax-model-selection/-/tree/gw-distributions/test/o3-nsbh/data). **Update link once merge request has been accepted**
Below, I compare the main output of the calculation: the probability that an object is consistent with a NS. Links point to where the (old/new) results are stored. I provide a comparison to all previous results computed for both GW200105 and GW200115.