ALMA observations of super-early galaxies: Attenuation-free model predictions

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Table 1.

Relevant properties of the selected super-early galaxies at z > 10.

ID	redshift	A_V [mag]	SFR [M_⊙ yr⁻¹]	log(M_⋆/M_⊙)	r_e [pc]	$F_{88}^{fid}$ $F_{88}^{\mathrm{fid}}$ [μJy]	$F_{88}^{\max}$ $F_{88}^{\mathrm{max}}$ [μJy]	log(r_d^fid/r_e)
GS-z14-0 ^(a)	14.32	$0 . 31_{- 0.07}^{+ 0.14}$ $0.31^{+0.14}_{-0.07}$	$22_{- 6}^{+ 6}$ $22^{+6}_{-6}$	$8 . 60_{- 0.2}^{+ 0.7}$ $8.60^{+0.7}_{-0.2}$	$260_{- 2}^{+ 2}$ $260^{+2}_{-2}$	14.9	40.1	0.73
GS-z14-1 ^(a)	13.90	$0 . 20_{- 0.07}^{+ 0.11}$ $0.20^{+0.11}_{-0.07}$	$2_{- 0.4}^{+ 0.7}$ $2^{+0.7}_{-0.4}$	$8 . 00_{- 0.4}^{+ 0.4}$ $8.00^{+0.4}_{-0.4}$	< 160	2.0	3.8	0.70
UNCOVER-z12 ^(b)	12.39	$0 . 19_{- 0.10}^{+ 0.17}$ $0.19^{+0.17}_{-0.10}$	$3 . 08_{- 0.68}^{+ 1.81}$ $3.08^{+1.81}_{-0.68}$	$8 . 35_{- 0.16}^{+ 0.21}$ $8.35^{+0.21}_{-0.16}$	$426_{- 42}^{+ 40}$ $426^{+40}_{-42}$	4.4	8.5	0.47
GS-z11-0 ^(c)	11.58	$0 . 18_{- 0.06}^{+ 0.06}$ $0.18^{+0.06}_{-0.06}$	$2 . 20_{- 0.22}^{+ 0.28}$ $2.20^{+0.28}_{-0.22}$	$8 . 67_{- 0.13}^{+ 0.08}$ $8.67^{+0.08}_{-0.13}$	77 ^( † )	5.2	7.8	1.38
GHZ2 ^(d)	12.34	$0 . 04_{- 0.03}^{+ 0.07}$ $0.04^{+0.07}_{-0.03}$	$5 . 2_{- 0.6}^{+ 1.1}$ $5.2^{+1.1}_{-0.6}$	$9 . 05_{- 0.25}^{+ 0.10}$ $9.05^{+0.10}_{-0.25}$	$105_{- 9}^{+ 9}$ $105^{+9}_{-9}$	3.4	4.0	1.76

Notes. The measured values are taken from the following references: ^(a)Carniani et al. (2024a), Robertson et al. (2024), ^(b)Wang et al. (2023), Fujimoto et al. (2023a), Atek et al. (2023), ^(c)Curtis-Lake et al. (2023), Robertson et al. (2024), ^(d)Castellano et al. (2024), ^( † )Error not provided. The last three columns show the predictions of the model for the fiducial (maximum) 88 μm observed flux, and the fiducial dust-to-stellar radius ratio for which A_V matches the observed value, respectively.

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