No gravitational waves were detected from the 2024 Vela glitch, but the new upper limits are the first to beat the indirect energy-scale benchmark from the glitch itself.
A nested sampling code for targeted searches for continuous gravitational waves from pulsars
1 Pith paper cite this work, alongside 6 external citations. Polarity classification is still indexing.
1
Pith paper citing it
6
external citations · Pith
abstract
This document describes a code to perform parameter estimation and model selection in targeted searches for continuous gravitational waves from known pulsars using data from ground-based gravitational wave detectors. We describe the general workings of the code and characterise it on simulated data containing both noise and simulated signals. We also show how it performs compared to a previous MCMC and grid-based approach to signal parameter estimation. Details how to run the code in a variety of cases are provided in Appendix A.
fields
gr-qc 1years
2025 1verdicts
ACCEPT 1representative citing papers
citing papers explorer
-
Constraints on gravitational waves from the 2024 Vela pulsar glitch
No gravitational waves were detected from the 2024 Vela glitch, but the new upper limits are the first to beat the indirect energy-scale benchmark from the glitch itself.