369 citations · 4.5k across the 75 of their papers we have counts for
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Exo-zodi modelling for the Large Binocular Telescope Interferometer
Grant M. Kennedy, Mark C. Wyatt, Vanessa Bailey +18
Habitable zone dust levels are a key unknown that must be understood to ensure the success of future space missions to image Earth analogues around nearby stars. Current detection…
Herschel/PACS photometry of transiting-planet host stars with candidate warm debris disks
Bruno Merín, David R. Ardila, Álvaro Ribas +4
Dust in debris disks is produced by colliding or evaporating planetesimals, remnants of the planet formation process. Warm dust disks, known by their emission at < 24 micron, are r…
Disk Radii and Grain Sizes in Herschel-Resolved Debris Disks
Nicole Pawellek, Alexander V. Krivov, Jonathan P. Marshall +5
(Abridged) The radii of debris disks and the sizes of their dust grains are tracers of the formation mechanisms and physical processes operating in these systems. We use a sample o…
Correlations between the stellar, planetary and debris components of exoplanet systems observed by
J. P. Marshall, A. Moro-Martín, C. Eiroa +18
The DEBRIS, DUNES and GT programmes observed 37 exoplanet host stars within 25 pc at 70, 100 and 160 m with the sensitivity to detect far-infrared excess emi…
How dusty is alpha Centauri? Excess or non-excess over the infrared photospheres of main-sequence stars
J. Wiegert, R. Liseau, P. Thébault +19
[Abridged] Debris discs around main-sequence stars indicate the presence of larger rocky bodies. The components of the nearby binary aCentauri have higher than solar metallicities,…
Observations, Modeling and Theory of Debris Disks
Brenda C. Matthews, Alexander V. Krivov, Mark C. Wyatt +2
Main sequence stars, like the Sun, are often found to be orbited by circumstellar material that can be categorized into two groups, planets and debris. The latter is made up of ast…