arXiv (All)
open access
Tracking the Evolution of Supermassive Black Hole Binaries with Pulsar Terms
Pulsar timing arrays will soon be able to resolve the loudest supermassive black hole binaries contributing to the stochastic gravitational wave background at nanohertz frequencies. While the few decades of observations are typically not enough to see these binaries evolve in frequency, the so-calle
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
- Detailed characterisation of the orbital parameters and eclipses of 'black widow' pulsars by radio timing and use of this new population of fast pulsars for the detection of the gravitational wave background#173060
- Prior volume effect inflates the gravitational-wave background in pulsar timing arrays#1412980
- Red noise and evolving signals: a complete frequentist approach to supermassive black hole binary searches with pulsar timing arrays#1063940
- Optimal Pulsar Timing Array Strategies with the Deep Synoptic Array#1155771
- Bridging the Population Synthesis of Supermassive Binary Black Holes and the Gravitational Wave Background#984606
Record · ID 1448252
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