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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 9.

On-sky distribution of 146 Hα-emitting galaxies at z = 5.1–5.5 selected with JADES photometry and confirmed with FRESCO. Galaxies at z = 5.17–5.30 are shown in filled circles color-coded by their redshifts, and the redshift distribution (bin size Δz = 0.005) is shown as the inset panel in the upper left corner. Galaxies at z = 5.10–5.17, and z = 5.30–5.50 are denoted by downward and upward black triangles, respectively. Spectroscopically confirmed galaxies in the z ∼ 5.2 overdensity before the JWST (Walter et al. 2012; Calvi et al. 2021) are shown in open squares, color-coded by their redshifts. HDF850.1 and another luminous SMG, GN10 at z = 5.30 (Wang et al. 2004; Pope et al. 2005; Riechers et al. 2020), are shown in blue and red plus signs, respectively. The footprint of JADES and FRESCO are shown in dashed gray and magenta polygons, respectively. A scale bar of 5 comoving Mpc at z = 5.2 is shown in the lower left corner for comparison.

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