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.
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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.
tPIC2.2 supplies a list of 217,741 stars for PLATO's LOPS2 field, including 202,315 FGK dwarfs/subgiants and 15,037 M dwarfs with uniformly estimated temperatures, radii, and masses.
citing papers explorer
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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.
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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.
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The PLATO Input Catalogue of targets (tPIC) for the first Long Pointing Field
tPIC2.2 supplies a list of 217,741 stars for PLATO's LOPS2 field, including 202,315 FGK dwarfs/subgiants and 15,037 M dwarfs with uniformly estimated temperatures, radii, and masses.