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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 11.

3D large-scale structure of the overdense environment in the GOODS-N field at z = 5.17–5.30. Coordinates of galaxies are with respect to that of HDF850.1 in units of comoving Mpc. All galaxies are color-coded by their redshifts, and galaxies in less dense regions (suggested by Gaussian kernel density estimation) are shown as transparent symbols. Spectroscopically confirmed galaxies in Walter et al. (2012), Calvi et al. (2021) that are not part of our sample are denoted as upward triangles. Through our clustering analysis, we identify four galaxy groups in the overdensities, potentially consisting of three filamentary structures over a volume of 16 × 18 × 64 cMpc³. The massive SMGs HDF850.1 and GN10 (shown as colored plus signs) reside in our proposed Filament-1 and -3, respectively.

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