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This article has been cited by the following article(s):
The MAGPI Survey: radial trends in star formation across different cosmological simulations in comparison with observations at z ~ 0.3
Marcie Mun, Emily Wisnioski, Katherine E Harborne, Claudia D P Lagos, Lucas M Valenzuela, Rhea-Silvia Remus, J Trevor Mendel, Andrew J Battisti, Sara L Ellison, Caroline Foster, Matias Bravo, Sarah Brough, Scott M Croom, Tianmu Gao, Kathryn Grasha, Anshu Gupta, Yifan Mai, Anilkumar Mailvaganam, Eric G M Muller, Gauri Sharma, Sarah M Sweet, Edward N Taylor and Tayyaba Zafar Monthly Notices of the Royal Astronomical Society 538(2) 976 (2025) https://doi.org/10.1093/mnras/staf342
The impact of morphological quenching mechanisms on star formation activity at 0.2 < z < 1.2 in the COSMOS field