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Cited article:

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A Decade of Radial-velocity Monitoring of Vega and New Limits on the Presence of Planets

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Dust Populations in the Iconic Vega Planetary System Resolved by ALMA

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Inner mean-motion resonances with eccentric planets: a possible origin for exozodiacal dust clouds

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DEBRIS DISKS IN THE SCORPIUS–CENTAURUS OB ASSOCIATION RESOLVED BY ALMA

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RESOLVED MILLIMETER-WAVELENGTH OBSERVATIONS OF DEBRIS DISKS AROUND SOLAR-TYPE STARS

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MAMBO image of the debris disk aroundϵEridani: robustness of the azimuthal structure

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Correlations between the stellar, planetary, and debris components of exoplanet systems observed byHerschel

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MILLIMETER EMISSION STRUCTURE IN THE FIRST ALMA IMAGE OF THE AU Mic DEBRIS DISK

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The Astrophysical Journal 762 (2) L21 (2013)
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CONFIRMING THE PRIMARILY SMOOTH STRUCTURE OF THE VEGA DEBRIS DISK AT MILLIMETER WAVELENGTHS

A. Meredith Hughes, David J. Wilner, Brian Mason, et al.
The Astrophysical Journal 750 (1) 82 (2012)
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RESOLVED SUBMILLIMETER OBSERVATIONS OF THE HR 8799 AND HD 107146 DEBRIS DISKS

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