Ultra-short-period planet formation around late M dwarfs occurs only in fixed close-in or inward-evolving inner disk edge scenarios, as planets follow the edge movement in simulations.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2representative citing papers
Machine learning classification of TESS data for 6 million stars in the LOPS2 field identifies 28% as candidate variables after filtering out 72% instrumental signals, producing one of the largest automated variability catalogs.
citing papers explorer
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The role of inner disk edges in shaping ultra-short-period planet systems around late M dwarfs
Ultra-short-period planet formation around late M dwarfs occurs only in fixed close-in or inward-evolving inner disk edge scenarios, as planets follow the edge movement in simulations.
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Variability classification of TESS targets in LOPS2, the first long-term pointing field of PLATO. Version 1 of the public variability catalogue
Machine learning classification of TESS data for 6 million stars in the LOPS2 field identifies 28% as candidate variables after filtering out 72% instrumental signals, producing one of the largest automated variability catalogs.