arXiv (All)
open access
Addressing leakage and mode suppression in angular power spectrum estimation for gravitational-wave backgrounds using pulsar timing arrays
Mapping gravitational-wave background (GWB) anisotropy with pulsar timing arrays (PTAs) is affected by harmonic-space mode suppression and mode coupling arising from an array's nonuniform sky response. Spherical harmonic expansions must be truncated at finite multipole l_max^rec, often set to l_max^
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
- The MeerKAT Pulsar Timing Array: Maps of the gravitational wave sky with the 4.5-yr data release#196902
- GW240925 and GW250207: Astrophysical Calibration of Gravitational Wave Detectors#1120768
- Gravitational-Wave Detection Using Pulsars: Status of the Parkes Pulsar Timing Array Project#779222
- Basic Data Processing of Gravitational Waves#987390
- Bridging the Population Synthesis of Supermassive Binary Black Holes and the Gravitational Wave Background#984606
Record · ID 1104968
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