[HTML][HTML] Assessing the similarity of continuous gravitational-wave signals to narrow instrumental artifacts
R Jaume, R Tenorio, AM Sintes - Universe, 2024 - mdpi.com
Continuous gravitational-wave (CW) signals are long-lasting quasi-monochromatic
gravitational-wave signals expected to be emitted by rapidly rotating non-axisymmetric …
gravitational-wave signals expected to be emitted by rapidly rotating non-axisymmetric …
[PDF][PDF] Assessing the Similarity of Continuous Gravitational-Wave Signals to Narrow Instrumental Artifacts. Universe 2024, 10, 121
R Jaume, R Tenorio, AM Sintes - 2024 - inspirehep.net
Continuous gravitational-wave (CW) signals are long-lasting quasi-monochromatic
gravitational-wave signals expected to be emitted by rapidly rotating non-axisymmetric …
gravitational-wave signals expected to be emitted by rapidly rotating non-axisymmetric …
Distinguishing transient signals and instrumental disturbances in semi-coherent searches for continuous gravitational waves with line-robust statistics
D Keitel - Journal of Physics: Conference Series, 2016 - iopscience.iop.org
Non-axisymmetries in rotating neutron stars emit quasi-monochromatic gravitational waves.
These long-duration'continuous wave'signals are among the main search targets of ground …
These long-duration'continuous wave'signals are among the main search targets of ground …
New veto for continuous gravitational wave searches
SJ Zhu, MA Papa, S Walsh - Physical Review D, 2017 - APS
We present a new veto procedure to distinguish between continuous gravitational wave
(CW) signals and the detector artifacts that can mimic their behavior. The veto procedure …
(CW) signals and the detector artifacts that can mimic their behavior. The veto procedure …
Toward inference of overlapping gravitational-wave signals
Merger rates of binary black holes, binary neutron stars, and neutron-star–black-hole
binaries in the local Universe (ie, redshift z= 0), inferred from the Laser Interferometer …
binaries in the local Universe (ie, redshift z= 0), inferred from the Laser Interferometer …
Detectability of stochastic gravitational wave background from weakly hyperbolic encounters
M Kerachian, S Mukherjee… - Astronomy & …, 2024 - aanda.org
We compute the stochastic gravitational wave (GW) background generated by black hole–
black hole (BH–BH) hyperbolic encounters with eccentricities close to one and compare …
black hole (BH–BH) hyperbolic encounters with eccentricities close to one and compare …
[HTML][HTML] Search methods for continuous gravitational-wave signals from unknown sources in the advanced-detector era
Continuous gravitational waves are long-lasting forms of gravitational radiation produced by
persistent quadrupolar variations of matter. Standard expected sources for ground-based …
persistent quadrupolar variations of matter. Standard expected sources for ground-based …
Gravitational wave detection without boot straps: a Bayesian approach
In order to separate astrophysical gravitational-wave signals from instrumental noise, which
often contains transient non-Gaussian artifacts, astronomers have traditionally relied on …
often contains transient non-Gaussian artifacts, astronomers have traditionally relied on …
Interpreting gravitational-wave burst detections: constraining source properties without astrophysical models
B Bécsy, P Raffai, K Gill, TB Littenberg… - … and Quantum Gravity, 2020 - iopscience.iop.org
We show that for detections of gravitational-wave transients, constraints can be given on
physical parameters of the source without using any specific astrophysical models. Relying …
physical parameters of the source without using any specific astrophysical models. Relying …
Gravitational-wave geodesy: Defining false alarm probabilities with respect to correlated noise
Future searches for a gravitational-wave background using Earth-based gravitational-wave
detectors might be impacted by correlated noise sources. A well-known example are the …
detectors might be impacted by correlated noise sources. A well-known example are the …