arXiv (All)
open access
Global time-frequency search for stellar-mass binary black holes in LISA
We present a complete pipeline for detecting and characterizing gravitational waves (GWs) produced by the inspiral of stellar-mass binary black holes in data from the Laser Interferometer Space Antenna (LISA). The analysis framework relies on an efficient time-frequency implementation of an adaptive
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
- LISA data analysis: the search for long-lived gravitational wave signals#186648
- Reconstructing stochastic gravitational-wave signals from flavour deconstruction with LISA#820663
- Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method#997874
- Detection and characterization of instrumental transients in LISA Pathfinder and their projection to LISA#997882
- Probing Kerr symmetry breaking with LISA extreme-mass-ratio inspirals#1049798
Record · ID 987489
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