Figure 4 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 4.

Probability density distribution of the ALMA source redshift based on lensing analysis (Caminha et al. 2021). This redshift distribution indicates that it is very likely that the ALMA source belongs to the same galaxy group as the MUSE galaxies at z = 4.32.

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