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An accurate measure of the size of dark matter haloes using the size of galaxies
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Evolution of the radial interstellar medium metallicity gradient in the Milky Way disk since redshift ≈3
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M. Mondelin, F. Bournaud, J.-C. Cuillandre, S. Codis, C. Stone, M. Bolzonella, J. G. Sorce, M. Kluge, N. A. Hatch, F. R. Marleau, M. Schirmer, H. Bouy, F. Buitrago, C. Tortora, L. Quilley, K. George, M. Baes, T. Saifollahi, P. M. Sanchez-Alarcon, J. H. Knapen, N. Aghanim, A. Amara, S. Andreon, C. Baccigalupi, A. Balestra, et al. Astronomy & Astrophysics 699 A214 (2025) https://doi.org/10.1051/0004-6361/202554838
The Growth of Galaxy Stellar Haloes over 0.2 ≤ z ≤ 1.1
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H i content at cosmic noon – a millimetre-wavelength perspective
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Detecting the edges of galaxies with deep learning
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The impact of environment on size: Galaxies are 50% smaller in the Fornax Cluster compared to the field
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