MB
M. Baes
astro-ph.GAastro-ph.COastro-ph.IMastro-phastro-ph.HEastro-ph.SRastro-ph.EPgr-qcmath.MPmath-ph
On Valency
published · living versionsW_utts5s39·v1 · currentpublished
A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios
with P. De Vis, A. Jones, S. Viaene, V. Casasola +15
1 version
W_3ukvwsjm·v1published
Preprints & journals
434 papers in the corpus · 1999–2026Euclid Quick Data Release (Q1). A systematic study of the intracluster light fraction at 0.2 < z < 1.52610.29684v1 · H. Gully, N. A. Hatch, H. Gao et al.2026 · 0 citationsarXivon Valency
Euclid Bypass end-to-end simulations for spectroscopic galaxy clustering performance assessment2610.26990v1 · B. R. Granett, S. de la Torre, M. Moresco et al.2026 · 0 citationsarXiv
Angular momentum in isolated disc galaxies: Insights from TNG1002608.21139v1 · A. Sorgho, L. Verdes-Montenegro, M. Baes et al.2026 · 0 citationsarXiv
3D Radiative Transfer of Lyman-series Lines with SKIRT2608.12527v1 · N. Sameshima, A. Lauwers, B. Vander Meulen et al.2026 · 0 citationsarXiv
MIGHTEE-HI: Environmental effects of cosmic filaments on extragalactic HI detections in the COSMOS and XMM-LSS fields2608.04656v1 · Seoyoung Lyla Jung, Madalina N. Tudorache, Matt J. Jarvis et al.2026 · 0 citationsarXiv
MIGHTEE-HI / LADUMA: Investigating the link between baryons and dynamics with 130 resolved HI-selected galaxies2608.03576v1 · Andreea A Varasteanu, Matt J. Jarvis, Harry Desmond et al.2026 · 0 citationsarXiv
The TNG50-SKIRT Atlas: Spatially resolved synthetic galaxies from the ultraviolet to the submillimetre (DR2)2608.01908v1 · Maarten Baes, Paul Vauterin, Abdurro'uf et al.2026 · 0 citationsarXiv
Visual analytics for cosmological simulation results2607.29426v1 · Paul Vauterin, Maarten Baes2026 · 1 citationarXiv
The evolution of galaxy dust scaling relations in the COLIBRE simulations2607.26058v1 · Aswin P. Vijayan, James W. Trayford, Joop Schaye et al.2026 · 0 citationsarXiv
Cosmological simulations of the high-redshift galaxy population adopting a variable stellar initial mass function2607.16404v1 · Anna Durrant, Robert A. Crain, Cedric G. Lacey et al.2026 · 0 citationsarXiv
The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations2607.14901v1 · Andrea Gebek, Maarten Baes, Nick Andreadis et al.2026 · 0 citationsarXiv
Predicting ionised gas emission in 3D with SKIRT. I. Framework and validation2607.09961v1 · Anand Utsav Kapoor, Maarten Baes, Aaron Smith et al.2026 · 0 citationsarXiv
Constraining the Physical Properties of Quadruply Lensed Quasars using Optical-to-X-Ray Data2606.25028v2 · Kriti Kamal Gupta, Dominique Sluse, Maarten Baes et al.2026 · 0 citationsarXiv
TODDLERS 2.0: Stellar feedback and observables across diverse IMFs, binary populations, and cloud environments2606.15184v1 · Anand Utsav Kapoor, Andrea Gebek, Maarten Baes et al.2026 · 0 citationsarXiv
Euclid: Disky titans - surprisingly high star formation activity and gas content in two brightest group galaxies at z~0.752606.02687v2 · F. Gentile, E. Daddi, D. Elbaz et al.2026 · 0 citationsarXiv
MIGHTEE-HI: HI catalogue of 293 sources for the COSMOS field and comparative study of 3-dimensional source finding methods2605.28731v1 · Michalina Maksymowicz-Maciata, Natasha Maddox, Catherine Hale et al.2026 · 0 citationsarXiv
Survival of very small carbonaceous dust grains in the inner-CGM of NGC 891 from JWST/MIRI MRS2605.26864v1 · J'er'emy Chastenet, Ilse De Looze, Karl D. Gordon et al.2026 · 0 citationsarXiv
The TNG50-SKIRT Atlas: Multi-wavelength nonparametric galaxy morphology2605.20886v1 · Sena Bokona Tulu, Maarten Baes, Angelos Nersesian et al.2026 · 1 citationarXiv
Euclid: Early Release Observations -- The formation of peanutty dwarf galaxies in Perseus2605.21342v1 · A. U. Kapoor, R. Smith, A. J. Zuiderwijk et al.2026 · 0 citationsarXiv
Summary of Discussion Sessions from "The Dusty Universe 2025: The Fifth Pandust Conference"2605.18992v1 · Marjorie Decleir, Karl D. Gordon, Annalisa De Cia et al.2026 · 0 citationsarXiv
The galaxy ultraviolet luminosity function from to in the COLIBRE simulations2605.06782v2 · Shengdong Lu, Carlos S. Frenk, Cedric G. Lacey et al.2026 · 0 citationsarXiv
Galaxy luminosity functions from far-UV to submillimetre at in the COLIBRE simulations2605.02022v2 · Shengdong Lu, Carlos S. Frenk, Cedric G. Lacey et al.2026 · 0 citationsMon Not R Astron Soc (2026)
The core of the problem: Physical limits of the core-Sérsic model2604.20344v1 · Maarten Baes (UGent)2026 · 0 citationsarXiv
Euclid: Scaled-up little red dots and other sources with v-shaped spectral energy distributions at z>42604.16178v1 · A. A. Tumborang, K. I. Caputi, P. Rinaldi et al.2026 · 0 citationsarXiv
JWST observations of photodissociation regions. IV. Carbonaceous emission band sub-components in NGC 7023 have distinct spatial distributions2604.12860v1 · D. Van De Putte, K. D. Gordon, K. Misselt et al.2026 · 1 citationA&A 710, A60 (2026)
VST-SMASH: VST Survey of Mass Assembly and Structural Hierarchy I. Survey presentation and deep photometry of IC 5332: tracing the mass assembly in the challenging faintest-end regime2604.07083v2 · R. Ragusa, C. Tortora, L. Hunt et al.2026 · 1 citationA&A 710, A42 (2026)
MICONIC: JWST/MIRI-MRS reveals heavily reprocessed PAH emission in the circum-nuclear disc of Centaurus A2603.23674v1 · L. Pantoni, M. Baes, L. Decin et al.2026 · 1 citationA&A 709, A237 (2026)
Spatially-resolved interstellar dust properties in the face-on spiral galaxy M 99 as observed by NIKA22602.20393v1 · L. Pantoni, F. Galliano, S. C. Madden et al.2026 · 0 citationsA&A 709, A1 (2026)
MIGHTEE HI observations of low surface brightness and ultra-diffuse galaxies in the XMM-LSS field2602.18128v1 · Elizabeth A. K. Adams, Barbara Siljeg, Anastasia Ponomareva et al.2026 · 0 citationsarXiv
Euclid: Early Release Observations -- The star-formation history of massive early-type galaxies in the Perseus cluster2601.20948v1 · S. Martocchia, A. Boselli, J.-C. Cuillandre et al.2026 · 0 citationsarXiv
Euclid: Early Release Observations -- The extended stellar component of the IC10 dwarf galaxy2601.11997v2 · F. Annibali, A. M. N. Ferguson, P. M. Sanchez-Alarcon et al.2026 · 0 citationsarXiv
Self-consistent dynamical models with a finite extent -- V. Smooth radial truncations and phase-space consistency2601.08361v1 · Maarten Baes (UGent)2026 · 0 citationsarXiv
Euclid preparation: LXXXI. The impact of nonparametric star formation histories on spatially resolved galaxy property estimation using synthetic Euclid images2511.22399v1 · A. Nersesian, Abdurro'uf, M. Baes et al.2025 · 0 citationsarXiv
Evidence for the Keplerian orbit of a close companion around a giant star2511.11247v1 · Mats Esseldeurs, Leen Decin, Joris De Ridder et al.2025 · 5 citationsarXiv
MIGHTEE-HI: The HI mass-stellar mass relation of massive galaxies and the HI mass function at 0.25<z<0.52510.23406v1 · Hengxing Pan, Matt J. Jarvis, Ian Heywood et al.2025 · 1 citationarXiv
JWST observations of photodissociation regions: II. Warm molecular Hydrogen spectroscopy in the Horsehead nebula2510.06812v1 · M. Zannese, P. Guillard, A. Abergel et al.2025 · 5 citationsA&A 704, A202 (2025)
Euclid preparation LXXIX. Using mock low surface brightness dwarf galaxies to probe Euclid Wide Survey detection capabilities2509.13163v2 · M. Urbano, P.-A. Duc, M. Poulain et al.2025 · 0 citationsarXiv
PRIMA survey of the Virgo cluster2509.04678v1 · Jacopo Fritz, Maarten Baes, Diego Alejandro Vasquez Torres et al.2025 · 0 citationsarXiv
The radial variation of the silicate-to-carbon ratio in M31 probed by PRIMA2509.01990v1 · J'er'emy Chastenet, Ilse De Looze, Maarten Baes et al.2025 · 0 citationsarXiv
The PRIMA promise of deciphering interstellar dust evolution with observations of the nearby Universe2509.01692v1 · Fr'ed'eric Galliano, Maarten Baes, L'eo Belloir et al.2025 · 0 citationsJ. Astron. Telesc. Instrum. Syst. 11(3) 031612 (6 May 2025)
Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions2508.21157v1 · Kosei Matsumoto, Laura Sommovigo, Andrea Gebek et al.2025 · 7 citationsarXiv
How Dust Models Shape High-z Galaxy Morphology: Insights from the NewCluster Simulation2508.18374v1 · Gyeong-Hwan Byun, J. K. Jang, Zachary P. Scofield et al.2025 · 6 citationsarXiv
Atomic hydrogen reservoirs in quiescent galaxies at z = 0.42507.16917v3 · A. Bianchetti, G. Rodighiero, D. Donevski et al.2025 · 0 citationsA&A 704, A162 (2025)
JWST Observations of Photo-dissociation Regions. II. Aliphatic/Aromatic Carbonaceous Dust, Ices, and Gas Phase Spectral Line Inventory2506.20468v2 · K. Misselt, A.N. Witt, K.D. Gordon et al.2025 · 9 citationsA&A 700, A158 (2025)
MICONIC: JWST/MIRI MRS reveals a fast ionized gas outflow in the central region of Centaurus A2506.15286v1 · A. Alonso-Herrero, L. Hermosa Munoz, A. Labiano et al.2025 · 8 citationsarXiv
MIGHTEE-HI: The direct detection of neutral hydrogen in galaxies at 2506.11935v2 · Matt J. Jarvis, Madalina N. Tudorache, I. Heywood et al.2025 · 6 citationsMon Not R Astron Soc (2025) 193-210
Euclid: Early Release Observations -- The surface brightness and colour profiles of the far outskirts of galaxies in the Perseus cluster2506.02745v1 · M. Mondelin, F. Bournaud, J.-C. Cuillandre et al.2025 · 8 citationsarXiv
Towards an observationally motivated AGN dusty torus model -- II. The roles of density distribution and chemical composition of the dust2505.23981v1 · Omar Ulises Reyes-Amador, Omaira Gonz'alez-Mart'in, Jacopo Fritz et al.2025 · 2 citationsMon Not R Astron Soc (2025) 813-840
Euclid: Early Release Observations of ram-pressure stripping in the Perseus cluster. Detection of parsec scale star formation with in the low surface brightness stripped tails of UGC 2665 and MCG +07-07-0702505.23342v1 · Koshy George, A. Boselli, J.-C. Cuillandre et al.2025 · 5 citationsA&A 701, A40 (2025)
Euclid preparation. Estimating galaxy physical properties using CatBoost chained regressors with attention2504.13020v1 · A. Humphrey, P. A. C. Cunha, L. Bisigello et al.2025 · 0 citationsA&A 702, A74 (2025)
Career total: at least 757 works. 434 are in this corpus.Showing the 50 most recent.
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