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Table B.1.

Rest-Frame 2 μm GALFIT and STATMORPH outputs, ordered by X-ray ID from Luo et al. (2017).

X-ray ID log10(LPSF) log10(LSersic) PSF Lum. Sérsic Index Sérsic Size Gini M20 Extended Point Source
[erg s−1] [erg s−1] Fraction (n) (Re) [kpc]
667 43.26 43.13 0.57 0.69 2.85 0.51 −1.81 likely yes: psf
668 43.20 43.87 0.18 0.76 2.42 0.48 −1.55 yes
689A 42.68 43.45 0.15 0.30 4.18 0.52 −1.75 yes
690 43.03 42.90 0.57 3.31 1.46 0.61 −2.09 yes
694 43.62 43.04 0.79 0.30 2.18 0.51 −1.72 likely yes
695 36.99 40.93 < 0.01 0.50 2.02 0.40 −1.39 likely
698 43.56 44.27 0.16 2.25 4.32 0.58 −2.06 yes
700 43.05 43.81 0.15 2.69 3.00 0.57 −2.03 yes yes: psf
703A 43.43 44.10 0.18 0.37 4.51 0.46 −1.75 yes likely
709A 42.51 43.31 0.14 0.30 6.09 0.44 −1.04 likely likely
715A 44.66 44.96 0.33 2.01 0.44 0.39 −1.55 yes: psf
718A 43.55 44.27 0.16 0.56 1.76 0.47 −1.53 likely
724A 42.65 42.89 0.37 2.61 0.60 0.50 −1.74 yes: psf
727 42.54 43.04 0.24 5.07 2.22 0.58 −1.95 likely yes: psf
735 44.43 43.76 0.83 0.57 5.37 0.56 −1.82 yes: psf
745 43.57 43.84 0.35 1.45 3.18 0.57 −1.98 likely yes: psf
748A 43.91 44.36 0.26 0.96 3.70 0.52 −1.90 yes yes: psf
749A 42.97 43.77 0.14 0.59 4.94 0.47 −1.88 yes yes
751A 43.70 44.42 0.16 0.87 2.16 0.56 −1.60 yes
754 42.22 42.33 0.44 0.76 1.57 0.51 −1.85 yes likely
756 43.56 43.71 0.41 2.74 1.30 0.49 −1.77 yes likely
758 42.19 43.27 0.08 0.77 2.06 0.39 −0.81 yes
767 42.49 43.35 0.12 3.78 2.14 0.56 −1.92 yes likely
788 43.73 43.67 0.54 1.16 0.79 0.41 −1.56 likely yes
797A 43.87 43.96 0.45 1.48 2.73 0.58 −1.92 yes yes
799 42.45 42.98 0.23 0.80 2.26 0.50 −1.78 yes
801 43.51 43.56 0.47 0.57 3.35 0.52 −1.78 yes likely
805A 44.38 44.44 0.46 1.66 0.68 0.47 −1.47 yes: psf
809 43.11 43.09 0.51 0.86 1.15 0.51 −1.72 likely likely
840 43.40 42.78 0.81 0.39 6.33 0.55 −1.76 likely yes: psf
S-36 41.36 42.23 0.12 0.51 1.65 0.45 −1.70 yes likely

Notes. Column 1 lists the IDs adopted from Luo et al. (2017), where an ‘A’ indicates the source is detected in the ASPECS ALMA survey of the HUDF (Boogaard et al. 2024). Columns 2 and 3 indicate the rest-frame 2 μm luminosities for the PSF and Sérsic model, converted to units of erg s−1 using the rest-frame frequency, whilst column 4 details the PSF to total luminosity fraction of the source from the GALFIT modelling. The Sérsic index, effective radius, Gini and M20 parameters are given in columns 5, 6, 7 and 8. In columns 9 and 10 we list the visual classification of extended and point-source components, for ease of comparison with the quantitative results (see Appendix C for details).

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