arXiv (All)
open access
Time-Correlated Profile Variability in the MeerKAT Pulsar Timing Array
Long-term pulse-profile variability has emerged as a potentially important source of uncertainty for high-precision pulsar timing, as changes in the integrated pulse shape can bias pulse times of arrival and affect the sensitivity of pulsar timing arrays to nanohertz gravitational waves. We present
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
- Finite velocity effect of ultralight vector dark matter in pulsar timing arrays#820160
- Bias from small-scale leakage in Pulsar Timing Array maps#996876
- Searching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array#453426
- Testing Gravity with Binary Pulsars in the SKA Era#635703
Record · ID 996731
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