The first informative astrophysical calibration of gravitational-wave detectors is reported using GW240925 and GW250207.
Coherent WaveBurst, a pipeline for unmodeled gravitational-wave data analysis
4 Pith papers cite this work. Polarity classification is still indexing.
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gr-qc 4years
2026 4representative citing papers
Presents a practical fully time-domain end-to-end likelihood for gravitational-wave inference with structured linear algebra and GPU acceleration.
A framework using scale separation in the Isaacson description defines observable gravitational memory rise for compact binary coalescences, providing a basis for hypothesis testing in LISA data.
An explicit, GPU-ready WDM wavelet-packet package reproduces frequency-domain LISA galactic-binary posteriors under stationary noise and documents the full discrete construction.
citing papers explorer
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GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors
The first informative astrophysical calibration of gravitational-wave detectors is reported using GW240925 and GW250207.
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Accelerated Time-domain Analysis for Gravitational Wave Astronomy
Presents a practical fully time-domain end-to-end likelihood for gravitational-wave inference with structured linear algebra and GPU acceleration.
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Toward claiming a detection of gravitational memory
A framework using scale separation in the Isaacson description defines observable gravitational memory rise for compact binary coalescences, providing a basis for hypothesis testing in LISA data.
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An explicit and differentiable Wilson-Daubechies-Meyer transform for gravitational-wave data analysis
An explicit, GPU-ready WDM wavelet-packet package reproduces frequency-domain LISA galactic-binary posteriors under stationary noise and documents the full discrete construction.