arXiv (OAI Expanded)
open access
The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters
Of the > 500 confirmed transiting hot jupiters and approximately 2000 additional candidates today, only ten are known to have nearby companion planets. The survival of nearby companions means that these hot jupiters cannot have migrated to their present location via dynamically disruptive high-eccen
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 Occurrence Rate of Nearby Planetary Companions to Hot Jupiters#925094
- New and Updated Rossiter-McLaughlin Measurements for Three Hot Jupiter-Hosting M Dwarfs#925400
- New and Updated Rossiter-McLaughlin Measurements for Three Hot Jupiter-Hosting M Dwarfs#921164
- Migration and Evolution of giant ExoPlanets (MEEP). III. Twenty-Nine Giant Planets from the TESS Mission#1143069
- Marginalized planet-to-star radius ratio posteriors for low-SNR transiting planets via dimensionality reduction#1048904
Record · ID 920860
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