output
20052026
most citedThe TESS Objects of Interest Catalog from the TESS Prime Mission

392 citations

388 papers

cs.RO2026

Robots Influencing Humans to Reveal their Goals during Collaboration and Competition

Debasmita Ghose, Oz Gitelson, Michal Lewkowicz +3

We propose a unified strategy for fast goal inference in human-robot interaction. The core idea is to drive the human toward Critical Decision Points (CDPs)-states where competing…

physics.flu-dyn2026★ 6 cited

Construction of flexible wing models by combined manufacturing of additive and subtractive processes for transonic wind tunnel testing

Natsuki Tsushima, Kensuke Soneda, Kenichi Saitoh +1

This study presents a systematic manufacturing approach that combines metal additive manufacturing and subtractive machining to construct flexible wing models for transonic wind tu…

astro-ph.EP2026★ 1 cited

ASTEP confirmation of a pair of long-period Jupiter-sized planets with extremely low densities transiting TOI-791

Georgina Dransfield, Antoine C. Petit, Amaury H. M. J. Triaud +45

Gas giant planets with periods orbiting Sun-like stars are a relatively uncommon outcome of planetary formation, and key questions about the nature and form…

nlin.PS2026

Formation of mechanical rogue waves

Yasuhiro Miyazawa, Christopher Chong, Panayotis G. Kevrekidis +1

Rogue waves, characterized by their abrupt and extreme localization in space and time, have evolved from maritime folklore to subjects of intense study across diverse fields, from…

astro-ph.GA2026

The Dyson Minds 2025 Workshop: SETI around Black Holes

Olivia Curtis, Van Hunter Adams, Daniel Angerhausen +9

The Dyson Minds 2025 Workshop, held at the Center for Brains, Minds & Machines at MIT and organized by Penn State, MIT, and The Ultraintelligence Foundation, brought together resea…

astro-ph.EP2026★ 1 cited

Direct Images of CO2 Absorption in the Atmosphere of a Super-Jupiter: Enhanced Metallicity Suggestive of Formation in a Disk

William O. Balmer, Laurent Pueyo, Ashley Messier +15

It is unclear how directly imaged substellar companions with masses near the deuterium burning limit form, because these objects are rare and their bulk properties are not diagnost…