Combined TESS-CHEOPS data on 5620 flares shows ED-based FFDs follow power laws but bolometric-energy FFDs are best described by a truncated power law with break at 1.8e35 erg, with low-energy flattening attributed to detection biases rather than intrinsic lognormal behavior.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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New ESPRESSO transmission spectroscopy of GJ 436 b shows no detectable atmospheric features from H I, Na I, Fe I or other species, producing upper limits consistent with a featureless optical spectrum.
citing papers explorer
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Extending TESS flare frequency distributions with CHEOPS: Power-law versus lognormal
Combined TESS-CHEOPS data on 5620 flares shows ED-based FFDs follow power laws but bolometric-energy FFDs are best described by a truncated power law with break at 1.8e35 erg, with low-energy flattening attributed to detection biases rather than intrinsic lognormal behavior.
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The atmosphere of the warm Neptune GJ 436 b probed with ESPRESSO
New ESPRESSO transmission spectroscopy of GJ 436 b shows no detectable atmospheric features from H I, Na I, Fe I or other species, producing upper limits consistent with a featureless optical spectrum.