activity
20142026
most citedStar formation in the outskirts of DDO 154: A top-light IMF in a nearly dormant disc

39 citations · 273 across the 24 of their papers we have counts for

collaborators

26 papers

quant-ph2026

Anti-symmetrization is cheap and useful

Adam Bene Watts, John Bostanci, Matthias C. Caro +3

We consider the computational task of anti-symmetrization of an unknown mixed quantum state: Given iid copies of a rank- qudit state $ρ=\sum_{i=1}^r λ_i |φ_i\rangle\!\langleφ_i|…

astro-ph.GA2025★ 4 cited

Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE)

Barbara Catinella, Luca Cortese, Jiayi Sun +26

The Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE) project is a multi-facility programme exploring how dense environments transform galaxies. Combining a VLT/MUSE…

astro-ph.IM2025

GalProTE: Galactic Properties Mapping using Transformer Encoder

Omar Anwar, Brent Groves, Luca Cortese +1

This work presents GalProTE, a proof-of-concept Machine Learning model utilizing a Transformer Encoder to determine stellar age, metallicity, and dust attenuation from optical spec…

astro-ph.GA2024★ 22 cited

The GECKOS Survey: Identifying kinematic sub-structures in edge-on galaxies

A. Fraser-McKelvie, J. van de Sande, D. A. Gadotti +30

The vertical evolution of galactic discs is governed by the sub-structures within them. We examine the diversity of kinematic sub-structure present in the first 12 galaxies observe…

quant-ph2024★ 1 cited

Quantum advantage from measurement-induced entanglement in random shallow circuits

Adam Bene Watts, David Gosset, Yinchen Liu +1

We study random constant-depth quantum circuits in a two-dimensional architecture. While these circuits only produce entanglement between nearby qubits on the lattice, long-range e…

astro-ph.GA2024

MAUVE: A 6 kpc bipolar outflow launched from NGC 4383, one of the most HI-rich galaxies in the Virgo cluster

Adam B. Watts, Luca Cortese, Barbara Catinella +11

Stellar feedback-driven outflows are important regulators of the gas-star formation cycle. However, resolving outflow physics requires high resolution observations that can only be…