Ultra-thick warm absorbers form a new subclass of AGN ionized outflows with exceptionally high column densities and moderate ionization that drive strong variability and may connect to ultra-fast outflows.
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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.
citing papers explorer
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Ultra-thick warm absorbers: Enlarging the parameter space of AGN ionised outflows
Ultra-thick warm absorbers form a new subclass of AGN ionized outflows with exceptionally high column densities and moderate ionization that drive strong variability and may connect to ultra-fast outflows.
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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.