Skip to content
Snippets Groups Projects

Link to 2306.09234

Merged Michael William Coughlin requested to merge michael-coughlin/userguide:arxiv into main
All threads resolved!
Files
2
+ 7
4
@@ -63,10 +63,8 @@ O5, based on a Monte Carlo simulation of detection and localization of events.
We note that these numbers assume Virgo's participation, and so are optimistic
relative to what is expected early in O4.
The methodology of the simulation is the same as described in [#LivingReview]_
and [#DataDrivenExpectations]_, although the GW detector network
configurations, sensitivity curves, astrophysical rates, and mass and spin
distributions have been updated.
The methodology and results of the simulation are described in
[#Kiendrebeogo2023]_ (also see [#LivingReview]_ and [#DataDrivenExpectations]_).
**Source code to reproduce these simulations** is available at
https://github.com/lpsinger/observing-scenarios-simulations/tree/v2 or
@@ -524,6 +522,11 @@ volume, and luminosity distance of detectable events in O3, O4, and O5.
Petrov, P., Singer, L. P., Coughlin, M. W., et al. 2022, |ApJ| 924, 54.
:doi:`https://doi.org/10.3847/1538-4357/ac366d`
.. [#Kiendrebeogo2023]
Kiendrebeogo, R. W., Farah, A. M., Foley E. M, et al. 2023, *Updated
observing scenarios and multi-messenger implications for the International
Gravitational-wave Network's O4 and O5*. :arxiv:`2306.09234`
.. [#O3b_pop]
LIGO Scientific Collaboration & Virgo Collaboration 2021, *The population of
merging compact binaries inferred using gravitational waves through GWTC-3*.
Loading