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JADES: Resolving the Stellar Component and Filamentary Overdense Environment of Hubble Space Telescope (HST)-dark Submillimeter Galaxy HDF850.1 at z = 5.18

  • Authors: Fengwu Sun, Jakob M. Helton, Eiichi Egami, Kevin N. Hainline, George H. Rieke, Christopher N. A. Willmer, Daniel J. Eisenstein, Benjamin D. Johnson, Marcia J. Rieke, Brant Robertson, Sandro Tacchella, Stacey Alberts, William M. Baker, Rachana Bhatawdekar, Kristan Boyett, Andrew J. Bunker, Stephane Charlot, Zuyi Chen, Jacopo Chevallard, Emma Curtis-Lake, A. Lola Danhaive, Christa DeCoursey, Zhiyuan Ji, Jianwei Lyu, Roberto Maiolino, Wiphu Rujopakarn, Lester Sandles, Irene Shivaei, Hannah Übler, Chris Willott, Joris Witstok

Fengwu Sun et al 2024 The Astrophysical Journal 961 .

  • Provider: AAS Journals

Caption: Figure 10.

NIRCam F444W-F200W-F090W RGB image (left) and F444W grism spectrum (right) of five Hα-emitting galaxies at z = 5.220–5.222, obtained through the JADES and FRESCO surveys, respectively. The NIRCam image is rotated to align with the dispersion direction. The brightest galaxy in the center (F444W = 25.3 AB mag) is at R.A. = 12:37:03.699, decl. = +62°11′57.″7. Hα redshifts of the five galaxies are noted in the right panel, and the two galaxies on the right (northwest) were spectroscopically confirmed previously at z Lyα = 5.224 (Calvi et al. 2021).

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