REVIEW 6 cited by
The MBTA Pipeline for Detecting Compact Binary Coalescences in the Third LIGO-Virgo Observing Run
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
We describe the Multi-Band Template Analysis (MBTA) search for gravitational waves signals from coalescences of compact objects in the LIGO-Virgo data, at the time of the third observing run (2019-2020), both for low-latency detections and for offline analysis. Details are given on the architecture and functioning of the pipeline, including transient noise mitigation strategies, parameter space for the searched signals, detection of candidates and evaluation of a false alarm rate associated to them. The performance of the low-latency search is demonstrated based on the LIGO-Virgo third observing run, during which MBTA has contributed to 42 alerts, submitting candidates with a median latency of 36 seconds. The performance of the offline search is illustrated on a subset of data collected during the second LIGO-Virgo observation run in 2017, and are quantified based on injections of simulated signal events on the same data.
Forward citations
Cited by 6 Pith papers
-
Detectability of Gravitational-wave counterparts of EP-FXTs observed during the O4b LIGO-Virgo-KAGRA Observing Run
No gravitational-wave counterpart is statistically associated with any of 47 Einstein Probe fast X-ray transients in the O4b run; 90% exclusion distances of ~178 Mpc (BNS) and ~349 Mpc (NSBH) disfavor nearby compact-b...
-
Likelihood Reconstruction for Radio Detectors of Neutrinos and Cosmic Rays
A multivariate-normal likelihood with a circulant noise covariance, derived from the noise spectrum, improves radio-detector reconstruction of neutrino and cosmic-ray parameters and yields correctly covered event-by-e...
-
Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency
A new toy inspiral waveform parameterized directly by precession amplitude and frequency predicts that precession is most detectable at 'plus nulls' and in a majority of isotropic maximal-spin black-hole binaries out ...
-
A neural network for estimating compact binary coalescence parameters of gravitational-wave events in real time
A quantile regression neural network produces real-time credible intervals for chirp mass, mass ratio, and total mass of compact binary mergers, with coverage mostly above 90%, and these intervals serve as priors that...
-
Parameter Estimation on LIGO-Virgo-KAGRA O4a Binary Merger Triggers with Sub-solar Mass Components
Bayesian re-analysis of the seven LVK O4a sub-solar-mass triggers finds three that are compatible with a sub-solar-mass component, though none rises to detection significance.
-
Robustness of Sensitivity Evaluations for Gravitational Wave Detection Algorithms
AresGW model 1's injection detection count at a false-alarm rate of 1/month varies with noise dataset by up to 39% coefficient of variation, while sensitive distance varies by only a few percent.
Discussion (0). Continue with ORCID to comment.