collaborators

5 papers

astro-ph.GA2026

Predicting ionised gas emission in 3D with SKIRT. I. Framework and validation

Anand Utsav Kapoor, Maarten Baes, Aaron Smith +7

Emission lines from ionised gas are key diagnostics of star formation, metallicity, and ionisation conditions in galaxies. Interpreting spatially resolved observations from integra…

astro-ph.GA2026

TODDLERS 2.0: Stellar feedback and observables across diverse IMFs, binary populations, and cloud environments

Anand Utsav Kapoor, Andrea Gebek, Maarten Baes +4

Modeling the feedback-driven evolution of star-forming regions and their multi-wavelength emission is essential for interpreting galaxy observations across cosmic time. TODDLERS co…

astro-ph.GA2026

Euclid: Early Release Observations -- The formation of peanutty dwarf galaxies in Perseus

A. U. Kapoor, R. Smith, A. J. Zuiderwijk +133

Dwarf galaxies in dense cluster environments are susceptible to tidal interactions that can alter their morphology and kinematics. Boxy isophotes are well studied in massive galaxi…

astro-ph.IM2025

Unlocking the physics of dwarf galaxies in the 2040s: The case for a next-generation wide-field spectroscopic facility with fibres and IFUs

Crescenzo Tortora, Daniela Carollo, Leslie Hunt +25

Dwarf galaxies () are the most numerous galaxies in the Universe and critical probes of dark matter, baryonic feedback, and galaxy formation. D…

astro-ph.GA2025

Constraints on asteroid-mass primordial black holes in dwarf galaxies using Hubble Space Telescope photometry

Nicolas Esser, Carrie Filion, Sven De Rijcke +4

Primordial black holes (PBHs) in the asteroid-mass range remain a viable and until now unconstrained dark matter (DM) candidate. If such PBHs exist, they could be captured by stars…