collaborators

6 papers

astro-ph.SR2025

Exploring Young Stellar Variability with Gaia DR3 light curves

Chloé Mas, Julia Roquette, Marc Audard +5

Context: Photometric variability is a defining characteristic of young stellar objects (YSO), which can be traced back to a range of physical processes taking place at different st…

astro-ph.SR2025

Linking Young Stellar Object Morphology to Evolutionary Stages with Self-Organizing Maps

David Hernandez, Odysseas Dionatos, Marc Audard +5

Studies in the past few decades have investigated young stellar object evolution based on their spectral energy distribution (SED). The SED is heavily influenced not only by evolut…

astro-ph.IM2025

Learning novel representations of variable sources from multi-modal data via autoencoders

P. Huijse, J. De Ridder, L. Eyer +18

Gaia Data Release 3 (DR3) published for the first time epoch photometry, BP/RP (XP) low-resolution mean spectra, and supervised classification results for millions of variable sour…

astro-ph.SR2025

The NEMESIS Catalogue of Young Stellar Objects for the Orion Star Formation Complex. I. General description of data curation

J. Roquette, M. Audard, D. Hernandez +5

The past decade has seen a rise in the use of Machine Learning methods in the study of young stellar evolution. This trend has led to a growing need for a comprehensive database of…

astro-ph.IM2025

A Deep Neural Network Approach to Compact Source Removal

M. Madarász, G. Marton, I. Gezer +5

Analysing extended emission in photometric observations of star-forming regions requires maps free from compact foreground, embedded, and background sources, which can interfere wi…

astro-ph.SR2025

SED Modeling of Young Stellar Objects in the Orion Star Formation Complex

Ilknur Gezer, Gábor Marton, Julia Roquette +4

We performed a large-scale spectral energy distribution (SED) fitting analysis for young stellar objects (YSOs) in the Orion star formation complex (OSFC) to derive key physical pa…