activity
20082025
most citedAn extremely primitive halo star

341 citations · 1.1k across the 26 of their papers we have counts for

collaborators

27 papers

astro-ph.CO2025

Euclid preparation. XCI. Validation method for the detections in the Euclid Catalogue of Galaxy Clusters using external data

Euclid Collaboration, J. -B. Melin, S. A. Stanford +315

We present our methodology for identifying known clusters as counterparts to objects in the Euclid Catalogue of Galaxy Clusters (ECGC). Euclid is expected to detect a large number…

astro-ph.HE2024★ 4 cited

Multi-wavelength study of OT 081: broadband modelling of a transitional blazar

MAGIC Collaboration, H. Abe, S. Abe +270

OT 081 is a well-known, luminous blazar that is remarkably variable in many energy bands. We present the first broadband study of the source which includes very-high-energy (VHE, $…

physics.flu-dyn2022

Formation and dynamics of a semi vortex ring connected to a free surface

Alexandre Vilquin, Samuel Hidalgo-Caballero, Vincent Pagneux +2

Playing a role in the locomotion of some animals such as the water strider, the formation and dynamics of a semi vortex ring connected to a free surface are experimentally investig…

astro-ph.HE2021

Southern African Large Telescope Spectroscopy of BL Lacs for the CTA project

E. Kasai, P. Goldoni, M. Backes +14

In the last two decades, very-high-energy gamma-ray astronomy has reached maturity: over 200 sources have been detected, both Galactic and extragalactic, by ground-based experiment…

astro-ph.GA2021★ 9 cited

Low star formation efficiency due to turbulent adiabatic compression in the Taffy bridge

B. Vollmer, J. Braine, B. Mazzilli-Ciraulo +1

The Taffy system (UGC 12914/15) consists of two massive spiral galaxies which had a head-on collision about 20 Myr ago. New sensitive, high-resolution CO(1-0) observations of the T…

astro-ph.SR2020★ 44 cited

PBjam: A Python package for automating asteroseismology of solar-like oscillators

M. B. Nielsen, G. R. Davies, W. H. Ball +14

Asteroseismology is an exceptional tool for studying stars by using the properties of observed modes of oscillation. So far the process of performing an asteroseismic analysis of a…