Figure 5 from ALMA Lensing Cluster Survey: An ALMA Galaxy Signposting a MUSE Galaxy Group at z = 4.3 Behind “El Gordo”

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ALMA Lensing Cluster Survey: An ALMA Galaxy Signposting a MUSE Galaxy Group at z = 4.3 Behind “El Gordo”

Authors: K. I. Caputi, G. B. Caminha, S. Fujimoto, K. Kohno, F. Sun, E. Egami, S. Deshmukh, F. Tang, Y. Ao, L. Bradley, D. Coe, D. Espada, C. Grillo, B. Hatsukade, K. K. Knudsen, M. M. Lee, G. E. Magdis, K. Morokuma-Matsui, P. Oesch, M. Ouchi, P. Rosati, H. Umehata, F. Valentino, E. Vanzella, W.-H. Wang, J. F. Wu, and A. Zitrin

2021 The Astrophysical Journal 908 146.

Provider: AAS Journals

Caption: Figure 5.

Best-fit SEDs for the four MUSE sources in the galaxy group at z = 4.32, in all the lensing components in which we have performed the SED fitting (those with photometry that is not significantly contaminated by the foreground cluster).

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