arXiv (All)
open access
Probing Two-dimensional Asymmetries of an Exoplanet Atmosphere from Chromatic Transit Variation
We propose a new method for investigating atmospheric inhomogeneities in exoplanets through transmission spectroscopy. Our approach links chromatic variations in conventional transit model parameters (central transit time, total and full durations, and transit depth) to atmospheric asymmetries. By s
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
- K-dwarf starspot hunters: how to directly characterize spot and faculae properties with UV-IR panchromatic transit spectra#1130328
- Steepening Optical Slopes in Exoplanet Transmission Spectra with Charged Hazes#1000202
- A Stellar-Type Dependence in the Rocky and Volatile Composition of Small Exoplanets#987080
- Ultraviolet Radiation Effects on the Optical Properties of Water-dominated Exoplanet Hazes#415003
- Exoplanet Atmosphere Spectral Sensitivity Analysis with PICASO: Jacobians, Linear-Gaussian Approximations, and Information Content#1037317
Record · ID 999646
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