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. 2023 Nov 18;14:7525. doi: 10.1038/s41467-023-42824-z

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© The Author(s) 2023

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

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Fig. 5 — a Two-sided Pearson correlation of CODE-MFA-derived fluxes for HeLa and A549. b Two-sided Pearson correlation of CODE-MFA-derived fluxes for HeLa and HCT116. c Two-sided Pearson correlation of CODE-MFA-derived fluxes for HeLa and LN229. d Two-sided Pearson correlation of CODE-MFA-derived fluxes for A549 and HCT116. e Two-sided Pearson correlation of CODE-MFA-derived fluxes for A549 and LN229. f Pearson correlation of CODE-MFA-derived fluxes for HCT116 and LN229. g CODE-MFA-derived net fluxes for fluxes with large difference per (f) (HCT116 vs. LN229).