The Citing articles tool gives a list of articles citing the current article. The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
This article has been cited by the following article(s):
Unveiling dust, molecular gas, and high star-formation efficiency in extremely UV bright star-forming galaxies at z ∼ 2.1–3.6
M. Dessauges-Zavadsky, R. Marques-Chaves, D. Schaerer, M.-Y. Xiao, L. Colina, J. Alvarez-Marquez and I. Pérez-Fournon Astronomy & Astrophysics 693 A17 (2025) https://doi.org/10.1051/0004-6361/202451832
Witnessing an extreme, highly efficient galaxy formation mode with resolved Lyman-α and Lyman-continuum emission
R. Marques-Chaves, D. Schaerer, E. Vanzella, A. Verhamme, M. Dessauges-Zavadsky, J. Chisholm, F. Leclercq, A. Upadhyaya, J. Álvarez-Márquez, L. Colina, T. Garel and M. Messa Astronomy & Astrophysics 691 A87 (2024) https://doi.org/10.1051/0004-6361/202451667
Evidence for very massive stars in extremely UV-bright star-forming galaxies at z ∼ 2.2–3.6
A. Upadhyaya, R. Marques-Chaves, D. Schaerer, F. Martins, I. Pérez-Fournon, A. Palacios and E. R. Stanway Astronomy & Astrophysics 686 A185 (2024) https://doi.org/10.1051/0004-6361/202449184
Nuclear high-ionisation outflow in the Compton-thick AGN NGC 6552 as seen by the JWST mid-infrared instrument
An extreme blue nugget, UV-bright starburst at z = 3.613 with 90 per cent of Lyman continuum photon escape
R Marques-Chaves, D Schaerer, J Álvarez-Márquez, et al. Monthly Notices of the Royal Astronomical Society 517(2) 2972 (2022) https://doi.org/10.1093/mnras/stac2893
The UV-brightest Lyman continuum emitting star-forming galaxy
R Marques-Chaves, D Schaerer, J Álvarez-Márquez, et al. Monthly Notices of the Royal Astronomical Society 507(1) 524 (2021) https://doi.org/10.1093/mnras/stab2187
Destruction of Galaxies as a Cause of the Appearance of Stellar Streams