High-contrast imaging with PACO and REXPACO reveals a new candidate companion at ~14 au and a tightly wound H-alpha spiral in the inner disk of HD 142527, suggesting ongoing companion-disk interactions.
M., Kalas, P., Fitzgerald, M
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.EP 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Multi-band optical imaging and modeling of the HR 4796A debris disk show highly forward-scattering dust consistent with large absorptive grains plus a possible clump and exterior halo.
Gaia astrometric quality metrics and a machine-learning classifier trained on known exoplanet hosts identify candidate stars with debris disks likely to host undetected planets.
citing papers explorer
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Exploration of the inner region of the system HD 142527
High-contrast imaging with PACO and REXPACO reveals a new candidate companion at ~14 au and a tightly wound H-alpha spiral in the inner disk of HD 142527, suggesting ongoing companion-disk interactions.
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A Multiband Study of the HR 4796A Disk in the Optical Using MagAO-X
Multi-band optical imaging and modeling of the HR 4796A debris disk show highly forward-scattering dust consistent with large absorptive grains plus a possible clump and exterior halo.
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An astrometric search for planets in debris disk systems
Gaia astrometric quality metrics and a machine-learning classifier trained on known exoplanet hosts identify candidate stars with debris disks likely to host undetected planets.