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Researcher
Conny Aerts
- Disciplines:Astronomy and space sciences
Projects
1 - 10 of 64
- Unveiling Noncanonical Stellar Evolution with Misaligned Rotational AsteroseismologyFrom1 Oct 2025 → TodayFunding: FWO junior postdoctoral fellowship
- MercatObs: The Mercator Observatory in the context of large space missionsFrom1 Jan 2025 → TodayFunding: FWO International research infrastructure (IRI)
- The temporal evolution of the multiplicity properties as massive stars age and interactFrom16 Sep 2024 → TodayFunding: Own budget, for example: patrimony, inscription fees, gifts
- Machine Learning Methods for Variable Star ResearchFrom16 Sep 2024 → TodayFunding: Own budget, for example: patrimony, inscription fees, gifts
- Modelling of the observed extended main-sequence turn-off of young open clusters from calibrations from asteroseismology and binarity.From22 Aug 2024 → TodayFunding: Own budget, for example: patrimony, inscription fees, gifts
- SOUL: Stellar evOlution in fUll gLory: rotation, magnetism, oscillations, outflows, tides, and binarityFrom1 Jan 2024 → TodayFunding: BOF - Methusalem
- Characterization of evolved planetary systems around pulsating white dwarfsFrom1 Oct 2023 → TodayFunding: FWO junior postdoctoral fellowship
- The use of artificial intelligence and machine learning in astrophysicsFrom25 Sep 2023 → 24 Sep 2025Funding: Foreign private sponsor - undefined
- Lifting stellar structure and evolution to higher dimensions in the era of space asteroseismologyFrom1 Sep 2023 → TodayFunding: HORIZON.1.1 - European Research Council (ERC)
- Upscaling and Industrialising Asteroseismic Modelling of Gravity-Mode PulsatorsFrom26 Aug 2023 → TodayFunding: BOF - doctoral mandates
Publications
1 - 10 of 374
- Automated all-sky detection of γ Doradus/δ Scuti hybrids in TESS data from positive unlabelled (PU) learning(2025)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 703
- Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars(2025)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 702
- Hot subluminous stars: Time-series analysis and pulsation mode identification(2025)
- Structure and Internal Rotation of Pulsating Stars(2025)
- Learning novel representations of variable sources from multi-modal Gaia data via autoencoders(2025)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 701
- Interior rotation modelling of the β Cep pulsator HD 192575 including multiplet asymmetries(2025)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 701
- Mode identification and ensemble asteroseismology of 119 β Cep stars detected by Gaia light curves and monitored by TESS(2025)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 698
- Discerning internal conditions of pulsating hot subdwarf B-type stars: Modeling multiple trapped modes in KIC 10001893(2025)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 698
- Evolution of the near-core rotation frequency of 2497 intermediate-mass stars from their dominant gravito-inertial mode ( vol 695 , 10.1051/0004-6361/202452691 , 2025 )(2025)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 698
- Asteroseismic predictions for a massive main-sequence merger product(2025)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 698