activity
20162025
most citedKuiper Belt-Like Hot and Cold Populations of Planetesimal Inclinations in the Pictoris Belt Revealed by ALMA

99 citations · 125 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2025

Recovering the structure of debris disks non-parametrically from images

Yinuo Han, Mark C. Wyatt, Sebastian Marino

Debris disks common around Sun-like stars carry dynamical imprints in their structure that are key to understanding the formation and evolution history of planetary systems. In thi…

astro-ph.EP20229 cited

Planetesimal/Debris discs

Sebastian Marino

This review chapter for young researchers presents our current understanding of debris discs. It introduces some of their basic properties and observables, and describes how we thi…

astro-ph.EP2020

Insights into the planetary dynamics of HD 206893 with ALMA

S. Marino, A. Zurlo, V. Faramaz +8

Radial substructure in the form of rings and gaps has been shown to be ubiquitous among protoplanetary discs. This could be the case in exoKuiper belts as well, and evidence for th…

astro-ph.EP201999 cited

Kuiper Belt-Like Hot and Cold Populations of Planetesimal Inclinations in the Pictoris Belt Revealed by ALMA

Luca Matrà, Mark C. Wyatt, David J. Wilner +4

The inclination distribution of the Kuiper belt provides unique constraints on its origin and dynamical evolution, motivating vertically resolved observations of extrasolar planete…

astro-ph.EP2018

A gap in the planetesimal disc around HD 107146 and asymmetric warm dust emission revealed by ALMA

S. Marino, J. Carpenter, M. C. Wyatt +9

While detecting low mass exoplanets at tens of au is beyond current instrumentation, debris discs provide a unique opportunity to study the outer regions of planetary systems. Here…

astro-ph.EP2018

An Empirical Planetesimal Belt Radius - Stellar Luminosity Relation

L. Matrà, S. Marino, G. M. Kennedy +3

Resolved observations of millimetre-sized dust, tracing larger planetesimals, have pinpointed the location of 26 Edgeworth-Kuiper belt analogs. We report that a belt's distance