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Table C.1.

Visual classification for each object in our sample, ordered by X-ray ID from Luo et al. (2017).

ID Class Class_ref Morphological categories identified in each object
Disc Spheroid Irregular Extended Point_Source Notes
[c]
667 AGN Luo17 likely likely yes: psf
668 AGN Lyu22 likely yes yes 00923 [a]
689 AGN Luo17 yes likely yes interacting?
690 Galaxy Luo17 likely yes likely yes interacting?
694 Galaxy Luo17 likely likely yes interacting?
695 AGN Lyu22 likely likely likely interacting?
698 AGN Lyu22 yes yes
700 AGN Lyu22 yes yes yes: psf
703 AGN Lyu22 yes yes yes likely 01520 [a]
709 Galaxy Luo17 likely likely likely likely likely interacting?; East IR source is X-ray source
715 AGN Luo17 yes: psf
718 AGN Luo17 likely likely likely interacting?
724 Galaxy Luo17 yes: psf
727 AGN Lyu22 likely likely likely yes: psf
735 AGN Luo17 yes: psf
745 AGN Luo17 likely likely yes: psf
748 AGN Luo17 yes likely yes yes: psf
749 Galaxy Luo17 yes likely yes yes
751 AGN Lyu24 yes yes interacting?; 00272 [a]; complex morphology
754 AGN Luo17 yes yes yes likely interacting?
756 AGN Lyu22 yes yes likely
758 AGN Luo17 yes yes interacting?
767 AGN Lyu22 likely yes yes likely
788 AGN Luo17 likely likely likely yes interacting?; [b]
797 AGN Luo17 yes yes yes interacting?
799 Galaxy Luo17 yes yes yes
801 AGN Lyu22 yes likely yes likely interacting?
805 AGN Luo17 yes: psf interacting?
809 AGN Luo17 likely likely likely likely interacting?
840 AGN Luo17 likely likely yes: psf
S-36 Galaxy Luo17 yes yes yes likely 00862 [a]

Notes. a. NGDEEP_nnnnn (Shen+24 H-alpha map)

b. also in z > 3 massive galaxies sample (CANDELS 14587; Costantin+24)

c. yes: psf – indicates PSF characteristic diffraction pattern is visible

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