HAL (France)
open access
TOI-4552 b: A new ultra-short-period rocky world revealed by NIRPS and TESS
Context. A particularly intriguing subclass of rocky exoplanets are the ultra-short period (USP) worlds that orbit their host stars in less than a day. These planets are particularly rare around M dwarf stars, with so far only ten that have a constrained mass and radius. Aims. We present 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
- Migration and Evolution of giant ExoPlanets (MEEP). III. Twenty-Nine Giant Planets from the TESS Mission#1143069
- The Birth and Early Feedback of Massive Star Clusters Across the Local Universe#1356548
- Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess#1367281
- The Occurrence Rate of Planets Around Subgiant Stars from TESS Photometric Survey#1141839
- Euclid : Quick Data Release (Q1) – A photometric search for ultracool dwarfs in the Euclid Deep Fields#405784
Record · ID 1492772
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