What shapes the bright end of the UV luminosity function? Stellar mass, star-formation variability, and dust in JADES

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Published October 23, 2026 | Version v1

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tableC_full_cut_sensitivity.csv md5:158951395adce158208ba45c8db4c912	3.4 kB	Preview Download
tableC_full_prior_sensitivity.csv md5:20aafb99f5ec11f74c8f0a83ebe6bcb9	3.9 kB	Preview Download
tableC_full_subset_sensitivity.csv md5:c94911a8f5aaa24b743d6f0b57e2565f	3.1 kB	Preview Download
tableC_injection.csv md5:9a7871ae607133132ee13b301505ebc0	1.5 kB	Preview Download
tableC_nulltests.csv md5:ef18e83ecb051a048f458a2f9c464cab	3.6 kB	Preview Download
tableC_robustness.csv md5:662504a1fa65095dcc5c1aba804c37cc	5.9 kB	Preview Download
tableH_data.csv md5:aa8b253553278c579095a3238685e1d3	7.2 kB	Preview Download
tableH_dust.csv md5:52041f3d768513ef4a87aa18bab1b78f	7.9 kB	Preview Download
tableH_results.csv md5:3bebca8a4e8de47e76b33ad49a082ce8	5.9 kB	Preview Download
tableH_uvlf.csv md5:0338ffa0b186e8ce62977575d0080a29	2.7 kB	Preview Download

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Zenodo

License: Creative Commons Attribution 4.0 International

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