arXiv (OAI Expanded)
open access
A semicoherent resampling method for long-transient gravitational wave searches with applications to subsolar-mass primordial black-hole binaries
Resampling removes the modeled phase evolution of a frequency-evolving signal, transforming it into a monochromatic one. We introduce a novel implementation for long-transient gravitational-wave searches that evaluates the Fourier spectrum of the resampled data using a type-I non-uniform fast Fourie
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Multi-messenger and multi-band signal from first-order phase transitions in proto-neutron stars#1077688
- GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients#1090419
- Black Holes as Frequency-Dependent Filters of Stochastic Gravitational Waves#1037327
- DANSur_HM: Modularly incorporating higher modes in a deep learning based gravitational-wave surrogate#1123199
- NRSur7dq4v2: A multi-domain precessing surrogate model with improved accuracy#984764
Record · ID 1069974
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive