activity
20172026
most citedPredicting the kinematic evidence of gravitational instability

48 citations · 102 across the 12 of their papers we have counts for

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Showing astro-ph.EPShow all

6 papers · 1 filter

astro-ph.EP2026★ 1 cited

exoALMA XXIII. Estimating Disk and Planet Properties from Dust Morphologies with DBNets2.0

Alessandro Ruzza, Giuseppe Lodato, Giovanni Rosotti +21

The exoALMA large program provided an unprecedented view of the morphology and kinematics of 15 circumstellar disks, offering a biased but homogenous and well-characterized sample…

astro-ph.EP2026★ 1 cited

A Collective Trigger for Widespread Planetesimal Formation Revealed by Accretion Ages

James Bryson, Hannah Sanderson, Francis Nimmo +4

The formation of planetesimals was an integral part of the cascading series of processes that built the terrestrial planets. To illuminate planetesimal formation, here we develop a…

astro-ph.EP2026

Dust Morphology Under Changing Dust Mass Ratios in Protoplanetary Discs

Matthew Murray, Cassandra Hall, Hans Baehr +1

Protoplanetary disc mass is one of the most fundamental properties of a planet-forming system, as it sets the total mass budget available for planet formation. However, obtaining d…

astro-ph.EP2024

A Machine Learning Approach to Detecting Albedo Anomalies on the Lunar Surface

Sofia Strukova, Sergei Gleyzer, Patrick Peplowski +1

This study introduces a data-driven approach using machine learning (ML) techniques to explore and predict albedo anomalies on the Moon's surface. The research leverages diverse pl…

astro-ph.EP2023★ 3 cited

Kinematic Evidence of an Embedded Protoplanet in HD 142666 Identified by Machine Learning

J. P. Terry, C. Hall, S. Abreau +1

Observations of protoplanetary disks have shown that forming exoplanets leave characteristic imprints on the gas and dust of the disk. In the gas, these forming exoplanets cause de…

astro-ph.EP2022★ 8 cited

Locating Hidden Exoplanets in ALMA Data Using Machine Learning

Jason Terry, Cassandra Hall, Sean Abreau +1

Exoplanets in protoplanetary disks cause localized deviations from Keplerian velocity in channel maps of molecular line emission. Current methods of characterizing these deviations…