Eccentricity posteriors of dynamically captured binaries can be mapped to capture parameters and compared against environment velocity distributions to constrain host and infer decay time.
2025 c , , 995, L18, 10.3847/2041-8213/ae0c06
10 Pith papers cite this work, alongside 28 external citations. Polarity classification is still indexing.
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2026 10representative citing papers
Stable mass transfer produces two distinct peaks in merging binary black hole primary mass and mass ratio distributions via mass ratio reversal under conservative mass transfer.
Statistical framework ranks candidate frequencies by combined amplitude and phase uncertainty widths from empirical percentiles, selecting 244 Hz for KAGRA sensing calibration with reduced amplitude interval width.
A faint radio counterpart to SN 2025ulz was detected at 6-10 GHz, consistent with either supernova ejecta interacting with circumstellar material or an off-axis jet, supporting possible superkilonova scenarios.
No sub-solar-mass compact-binary mergers were found in LIGO O4a data, giving 90% merger-rate upper limits of 110-10000 Gpc^-3 yr^-1 and weak new dark-matter constraints.
cWB XP on LIGO O3/O4 data yields near-perfect SASI identification from GWs alone at O4 sensitivity (PD=0.97 at 10 kpc for PFI=0.01) and improves joint O3 detection over prior work.
Describes the methods for producing the fifth gravitational-wave transient catalog (GWTC-5.0) from O4b data of LIGO, Virgo and KAGRA.
Overview summarizing the projected impacts of SKAO telescopes on pulsar discoveries, neutron star physics, and tests of relativistic gravity and nano-Hz gravitational waves.
LIGO-Virgo-KAGRA releases calibrated strain time series, noise-subtraction channels, and GWOSC v5.0 analysis products covering April 2024 to January 2025.
citing papers explorer
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Inferring host environment properties and gravitational-wave decay time from the eccentricity measurement of dynamically captured binaries
Eccentricity posteriors of dynamically captured binaries can be mapped to capture parameters and compared against environment velocity distributions to constrain host and infer decay time.
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A Stellar Role Reversal: Multiple Features in the Mass and Mass Ratio Distributions of Merging Binary Black Holes from Stable Mass Transfer
Stable mass transfer produces two distinct peaks in merging binary black hole primary mass and mass ratio distributions via mass ratio reversal under conservative mass transfer.
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Statistical-Uncertainty-Driven Selection of Evaluation Frequency for Time-Dependent Sensing Calibration: A Demonstration with KAGRA Data
Statistical framework ranks candidate frequencies by combined amplitude and phase uncertainty widths from empirical percentiles, selecting 244 Hz for KAGRA sensing calibration with reduced amplitude interval width.
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Identification of a Radio Counterpart to SN 2025ulz in the S250818k Localization Area
A faint radio counterpart to SN 2025ulz was detected at 6-10 GHz, consistent with either supernova ejecta interacting with circumstellar material or an off-axis jet, supporting possible superkilonova scenarios.
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Searches for Binary Mergers with Sub-solar Mass Components in Data from the First Part of LIGO--Virgo--KAGRA's Fourth Observing Run
No sub-solar-mass compact-binary mergers were found in LIGO O4a data, giving 90% merger-rate upper limits of 110-10000 Gpc^-3 yr^-1 and weak new dark-matter constraints.
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Joint Detection and Characterization of the Standing Accretion Shock Instability for Core-Collapse Supernovae with cWB XP
cWB XP on LIGO O3/O4 data yields near-perfect SASI identification from GWs alone at O4 sensitivity (PD=0.97 at 10 kpc for PFI=0.01) and improves joint O3 detection over prior work.
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GWTC-5.0: Methods for Identifying and Characterizing Gravitational-wave Transients
Describes the methods for producing the fifth gravitational-wave transient catalog (GWTC-5.0) from O4b data of LIGO, Virgo and KAGRA.
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Pulsar Science with the SKAO
Overview summarizing the projected impacts of SKAO telescopes on pulsar discoveries, neutron star physics, and tests of relativistic gravity and nano-Hz gravitational waves.
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Open Data from LIGO, Virgo, and KAGRA through the Second Part of the Fourth Observing Run
LIGO-Virgo-KAGRA releases calibrated strain time series, noise-subtraction channels, and GWOSC v5.0 analysis products covering April 2024 to January 2025.
- No model-independent evidence for a peak in binary black hole spin (mis)alignments