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2025
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Self Consistent Modeling of the Dust Emission from HD 100546: Evidence for Simultaneous Grain Evolution and Disk Disruption?
2025
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Searching for low-mass companions at small separations in transition disks with aperture masking interferometry
2024
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Sulphur monoxide emission tracing an embedded planet in the HD 100546 protoplanetary disk
2023
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The Doppler-flip in HD100546 as a disk eruption: the elephant in the room of kinematic protoplanet searches
2022
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H2O distribution in the disc of HD 100546 and HD 163296: the role of dust dynamics and planet--disc interaction
2022
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An inherited complex organic molecule reservoir in a warm planet-hosting disk
2021
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ALMA 870 micron continuum observations of HD 100546. Evidence of a giant planet on a wide orbit
2021
FEDELE D., TOCI C., MAUD L. & LODATO G.
Astron. & Astrophys.
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New Mid-Infrared Imaging Constraints on Companions and Protoplanetary Disks around six Young Stars
2021
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Constraining the properties of the potential embedded planets in the disk around HD 100546
2021
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Spatial distribution of the aromatic and aliphatic carbonaceous nano-grain features in the protoplanetary disk around HD 100546
2020
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Astron. & Astrophys.
, accepted
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High-resolution ALMA Observations of HD 100546: Asymmetric Circumstellar Ring and Circumplanetary Disk Upper Limits
2019
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X-ray Emission and Disk Irradiation of HL Tau and HD 100546
2019
SKINNER S. & GUEDEL M.
arxiv
Long Baseline Observations of the HD 100546 Protoplanetary Disk with ALMA
2019
PÉREZ S., CASASSUS S., HALES A., MARINO S., CHEETHAM A., et al.
ApJ. Letters
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Gaia Data Release 2. Summary of the contents and survey properties
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An Optical/near-infrared investigation of HD 100546 b with the Gemini Planet Imager and MagAO
2017
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Clarifying the Status of HD 100546 as Observed by the Gemini Planet Imager
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2014
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Recovery of the Candidate Protoplanet HD 100546 b with Gemini/NICI and Detection of Additional (Planet-Induced?) Disk Structure at Small Separations
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ApJ Letters
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Planet or Brown Dwarf? Inferring the Companion Mass in HD 100546 from the Wall Shape using Mid-Infrared Interferometry
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