output
19922026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing 2025 · astro-ph.EPShow all

9 papers · 2 filters

astro-ph.EP2025

Rotational Light-curve Recovery and Predictions of the LSST Yield of Hildas

Alexander J. Fleming, Jacob A. Kurlander, Dmitrii E. Vavilov +4

The Hilda population occupies the stable 3:2 mean-motion resonance of Jupiter and provides a window into solar system evolution, including collisional processes. The National Scien…

astro-ph.EP2025

Synchronisation of a tidal binary by inward orbital migration. The case of Pluto and Charon

Michael Efroimsky, Michaela Walterova, Yeva Gevorgyan +3

It is usually taken for granted that mutual synchronisation of a tidal two-body system is attained through tidal recession, assuming the reduced Hill sphere is not reached. However…

astro-ph.EP2025★ 14 cited

Catastrophic disruption of asteroid 2023 CX1 and implications for planetary defense

Auriane Egal, Denis Vida, François Colas +94

Mitigation of the threat from airbursting asteroids requires an understanding of the potential risk they pose for the ground. How asteroids release their kinetic energy in the atmo…

astro-ph.EP2025

Different arrival times of CM and CI-like bodies from the outer Solar System to the asteroid belt

Sarah E. Anderson, Pierre Vernazza, Miroslav Brož

Understanding the provenance of CI and CM chondrites, the most primitive materials in our meteorite collections, is critical for shedding light on the Solar System's early evolutio…

astro-ph.EP2025

Multi-scale radiative-transfer model of the protoplanetary disc DoAr 44

Marco Souza de Joode, Miroslav Brož

We aim to construct a comprehensive global multi-scale kinematic equilibrium radiative-transfer model for the pre-transitional disc of DoAr 44 (Haro 1-16, V2062 Oph) in the Ophiuch…

astro-ph.EP2025★ 3 cited

A dynamical dichotomy in large binary asteroids

K. Minker, B. Carry, F. Vachier +20

No less than 15% of large (diameter greater than 140 km) asteroids have satellites. The commonly accepted mechanism for their formation is post-impact reaccumulation. However, the…

astro-ph.EP2025★ 4 cited

Resurgence of CO in a warm bubble around accreting protoplanets and its observability

O. Chrenko, S. Casassus, R. O. Chametla

The cold outer regions of protoplanetary disks are expected to contain a midplane-centered layer where gas-phase CO molecules freeze out and their overall abundance is low. The lay…

astro-ph.EP2025★ 4 cited

Confined tumbling state as the origin of the excess of slowly rotating asteroids

Wen-Han Zhou, Patrick Michel, Marco Delbo +4

The rotational distribution of asteroids as a function of their size is used {as a diagnostic of} their physical properties and evolution. Recent photometric surveys from the Gaia…

astro-ph.EP2025★ 19 cited

JWST sighting of decameter main-belt asteroids and view on meteorite sources

Artem Y. Burdanov, Julien de Wit, Miroslav Brož +19

Asteroid discoveries are essential for planetary-defense efforts aiming to prevent impacts with Earth, including the more frequent megaton explosions from decameter impactors. Whil…