Population modeling of 50 tidally locked gas giants predicts cloud-driven evening-to-morning transit asymmetries reaching 500 ppm in optical bands for ultra-hot Jupiters, with regime-specific patterns from warm to ultrahot climates.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
verdicts
UNVERDICTED 2representative citing papers
Simulations show Plato can recover relativistic photometric signatures of supermassive black hole binaries in bright quasars (G≤18) via Bayesian inference on mock light curves.
citing papers explorer
-
Exoplanet climate characterization with transit asymmetries -- A comprehensive population study from the optical to the infrared
Population modeling of 50 tidally locked gas giants predicts cloud-driven evening-to-morning transit asymmetries reaching 500 ppm in optical bands for ultra-hot Jupiters, with regime-specific patterns from warm to ultrahot climates.
-
Plato's view on supermassive black hole binaries: Exploring the faint limit of ESA's Plato space mission
Simulations show Plato can recover relativistic photometric signatures of supermassive black hole binaries in bright quasars (G≤18) via Bayesian inference on mock light curves.