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A Stellar Bar Hidden in an Extreme Gas-rich Disk Galaxy at z = 4.055

  • Authors: Leindert A. Boogaard, Luca Costantin, Thor Tepper-García, Joss Bland-Hawthorn, Jacqueline A. Hodge, Cheng-Lin Liao, Mahmoud Hamed, Luis Colina, Fabian Walter, Oscar Agertz, Arjan Bik, Alejandro Crespo Gómez, Emanuele Daddi, Georgios E. Magdis, Pablo G. Pérez-González, Hannah Übler, Axel Weiss

Leindert A. Boogaard et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 4.

Stellar bar identification at multiple wavelengths. Isophotal analysis of the stellar bar (same as in Figure 2, with the leftmost panels showing the isophotes), now for the NIRCam F444W (top panels), MIRI F560W (middle panels), and MIRI F770W filters (bottom panels), including an additional fit leaving the center of the isophotes free, yielding consistent results.

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