arXiv (All)
open access
Companions of Hot Jupiters: two decades of radial velocity monitoring with CORALIE
Hot Jupiters are thought to form through multiple pathways, some of which can leave observable signatures in the architecture of their planetary systems. Massive outer companions, in particular, can provide important constraints on the dynamical histories of hot Jupiters. We aim to characterize the
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
- NGC 1901: A new benchmark cluster for gyrochronology in the TESS Southern continuous viewing zone#925653
- Juno spacecraft gravity measurements provide evidence for normal modes of Jupiter#153715
- ROSE (Red-giant Oscillations Spectra Estimator): A Modular Machine-Learning Framework for Automated Asteroseismic Characterisation. I. $ν_{\max}$ and $Δν$ from TESS#1234679
- Reconstructing Dark-Matter Inference via STT-CR: An Empirical Calibration Law for Low-Acceleration Dynamics#724216
- Fast Radio Burst Community Newsletter - Volume 7, Issue 09#1369032
Record · ID 1399985
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