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Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach

, and . (2017)cite arxiv:1702.04371Comment: 27 pages including 20 color figures, revised in response to referee's report.

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Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach, and . (2017)cite arxiv:1702.04371Comment: 27 pages including 20 color figures, revised in response to referee's report.CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST, , , , , , , , , and 49 other author(s). (2022)cite arxiv:2208.14480Comment: Submitted to ApJ; 12 Pages, 6 Figures.$Łambda$CDM not dead yet: massive high-z Balmer break galaxies are less common than previously reported, , , , , , , , , and 8 other author(s). (2023)cite arxiv:2310.03063Comment: Submitted to MNRAS, 10 pages (+4 in Appendix), 5 figures (+4), 1 table (+1).