The MUSE eXtremely Deep Field: Individual detections of Ly<i>;1</i> haloes around rest-frame UV-selected galaxies at <i>z</i>  2.9–4.4
H. Kusakabe, A. Verhamme, J. Blaizot, T. Garel, L. Wisotzki, F. Leclercq, R. Bacon, J. Schaye, S.G. Gallego, J. Kerutt, J.J. Matthee, M. Maseda, T. Nanayakkara, R. Pelló, J. Richard, L. Tresse, T. Urrutia, E. Vitte, Astronomy &; Astrophysics 660 (2022).

Equivalent widths of Lyman ;1 emitters in MUSE-Wide and MUSE-Deep
J. Kerutt, L. Wisotzki, A. Verhamme, K.B. Schmidt, F. Leclercq, E.C. Herenz, T. Urrutia, T. Garel, T. Hashimoto, M. Maseda, J.J. Matthee, H. Kusakabe, J. Schaye, J. Richard, B. Guiderdoni, V. Mauerhofer, T. Nanayakkara, E. Vitte, Astronomy &; Astrophysics 659 (2022).

Differences in galaxy colours are not just about the mass
J.J. Matthee, Nature Astronomy 5 (2021) 984–985.

The MUSE Hubble Ultra Deep field survey: XIII. Spatially resolved spectral properties of Lyman ;1 haloes around star-forming galaxies at z > 3
F. Leclercq, R. Bacon, A. Verhamme, T. Garel, J. Blaizot, J. Brinchmann, S. Cantalupo, A. Claeyssens, S. Conseil, T. Contini, T. Hashimoto, E.C. Herenz, H. Kusakabe, R.A. Marino, M. Maseda, J.J. Matthee, P. Mitchell, G. Pezzulli, J. Richard, K.B. Schmidt, L. Wisotzki, Astronomy &; Astrophysics 635 (2020).

Exploring HefII;b1640 emission line properties at z c24
T. Nanayakkara, J. Brinchmann, L. Boogaard, R. Bouwens, S. Cantalupo, A. Feltre, W. Kollatschny, R.A. Marino, M. Maseda, J.J. Matthee, M. Paalvast, J. Richard, A. Verhamme, Astronomy &; Astrophysics 648 (2019).

Predicting Ly;1 escape fractions with a simple observable: Ly;1 in emission as an empirically calibrated star formation rate indicator
D. Sobral, J.J. Matthee, Astronomy &; Astrophysics 623 (2019).

ALMA reveals metals yet no dust within multiple components in C
J.J. Matthee, D. Sobral, F. Boone, H. Röttgering, D. Schaerer, M. Girard, A. Pallottini, L. Vallini, A. Ferrara, B. Darvish, B. Mobasher, The Astrophysical Journal 851 (2017).