activity
20212026
most citedThe Gaia alerted fading of the FUor-type star Gaia21elv

18 citations · 37 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Milky Way Mapper decoded abundances -- II: From patterns to paths

Melissa K. Ness, Sarah Aquilina, Jennifer Mead +15

The element abundances of Milky Way disc stars encode entangled imprints of multiple enrichment processes, making it difficult to uncover the underlying chemical evolution. Here we…

astro-ph.GA2026★ 2 cited

Milky Way Mapper decoded abundances -- I. Shared disc enrichment patterns

Melissa K. Ness, Sarah Aquilina, Jennifer Mead +15

Elemental abundances in the Milky Way disc trace its star-formation and enrichment history, but predicting these abundances from theory is limited by uncertain nucleosynthetic yiel…

astro-ph.SR2023★ 18 cited

The Gaia alerted fading of the FUor-type star Gaia21elv

Zsófia Nagy, Sunkyung Park, Péter Ábrahám +26

FU Orionis objects (FUors) are eruptive young stars, which exhibit outbursts that last from decades to a century. Due to the duration of their outbursts, and to the fact that only…

astro-ph.IM2023★ 2 cited

Toward a Spectral Foundation Model: An Attention-Based Approach with Domain-Inspired Fine-Tuning and Wavelength Parameterization

Tomasz Różański, Yuan-Sen Ting, Maja Jabłońska

Astrophysical explorations are underpinned by large-scale stellar spectroscopy surveys, necessitating a paradigm shift in spectral fitting techniques. Our study proposes three enha…

astro-ph.SR2022

Early recognition of Microlensing Events from Archival Photometry with Machine Learning Methods

I. Gezer, Ł. Wyrzykowski, P. Zieliński +6

Gravitational microlensing method is a powerful method to detect isolated black holes in the Milky Way. During a microlensing event brightness of the source increases and this feat…

astro-ph.SR2021★ 15 cited

Lens parameters for Gaia18cbf -- a long gravitational microlensing event in the Galactic plane

Katarzyna Kruszyńska, Ł. Wyrzykowski, K. A. Rybicki +29

Context: The timescale of a microlensing event scales as a square root of a lens mass. Therefore, long-lasting events are important candidates for massive lenses, including black h…