Reference differential imaging of archival MIRI F1500W TSO data reaches 5σ contrasts of ~10^{-3} at 1" and ~2×10^{-4} beyond 3", enabling sensitivity to ~4–10 MJup planets at tens of AU around old M-dwarfs.
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2 Pith papers cite this work, alongside 42 external citations. Polarity classification is still indexing.
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representative citing papers
Reports 23.5% ±2.0% stellar multiplicity rate and 28.8% ±2.1% companion rate for M dwarfs in a 15 pc volume-limited sample from speckle imaging plus literature, with separation peaks at 198 au for planet hosts vs 5.57 au otherwise.
citing papers explorer
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A Search for Wide-orbit Planets Around M-dwarfs using Deep MIRI 15-micron Images
Reference differential imaging of archival MIRI F1500W TSO data reaches 5σ contrasts of ~10^{-3} at 1" and ~2×10^{-4} beyond 3", enabling sensitivity to ~4–10 MJup planets at tens of AU around old M-dwarfs.
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The POKEMON Speckle Survey of Nearby M Dwarfs. III. The Stellar Multiplicity Rate of M Dwarfs within 15 pc
Reports 23.5% ±2.0% stellar multiplicity rate and 28.8% ±2.1% companion rate for M dwarfs in a 15 pc volume-limited sample from speckle imaging plus literature, with separation peaks at 198 au for planet hosts vs 5.57 au otherwise.