ADF22+: A declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z = 3.09

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Table A.1.

S/N> 4.2 sources detected in the deep SSA22 1.17 mm mosaic.

ID	RA	Dec	S/N	S_1.17mm	NIR^a	redshift^b	spectral feature^c	Reference	M_⋆	SFR
ID matches Umehata et al. (2017)^d				[mJy]					[10¹⁰ M_⊙]	[M_⊙/yr]

A1	22:17:32.42	00:17:43.8	178.1	6.149 ± 0.060	Y	3.090	CO(3−2), [O III]	(1)	$15 . 5_{- 7.5}^{+ 11.2}$ $15.5_{-7.5}^{+11.2}$	$551_{- 171}^{+ 351}$ $551_{-171}^{+351}$
A5	22:17:31.48	00:17:58.0	81.4	2.530 ± 0.055	Y	3.089	CO(3−2), [O III]	(1)	$4 . 5_{- 2.1}^{+ 3.1}$ $4.5_{-2.1}^{+3.1}$	$205_{- 75}^{+ 131}$ $205_{-75}^{+131}$
A4	22:17:36.96	00:18:20.7	80.2	2.212 ± 0.028	Y	3.090	CO(3−2), CO(9−8)	(2)	$7 . 9_{- 4.1}^{+ 5.9}$ $7.9_{-4.1}^{+5.9}$	$248_{- 91}^{+ 160}$ $248_{-91}^{+160}$
A3	22:17:35.15	00:15:37.2	74.4	2.230 ± 0.036	Y	3.096	CO(3−2), [CI](1−0)	(3)	$3 . 0_{- 1.4}^{+ 1.9}$ $3.0_{-1.4}^{+1.9}$	$145_{- 29}^{+ 42}$ $145_{-29}^{+42}$
A2	22:17:36.11	00:17:36.7	83.7	2.170 ± 0.042	Y	3.991	CO(4−3), [CI](1−0)	(4)	$12 . 3_{- 9.8}^{+ 43.2}$ $12.3_{-9.8}^{+43.2}$	$198_{- 97}^{+ 224}$ $198_{-97}^{+224}$
A7	22:17:32.20	00:17:35.6	70.2	2.033 ± 0.039	Y	3.094	CO(3−2)	(1)	$4 . 4_{- 2.5}^{+ 2.6}$ $4.4_{-2.5}^{+2.6}$	$146_{- 34}^{+ 39}$ $146_{-34}^{+39}$
A6	22:17:35.84	00:15:59.0	54.5	1.427 ± 0.042	Y	3.095	CO(3−2), [O III]	(1), (5)	$4 . 6_{- 1.9}^{+ 2.0}$ $4.6_{-1.9}^{+2.0}$	$140_{- 40}^{+ 50}$ $140_{-40}^{+50}$
A8	22:17:37.11	00:17:12.3	43.9	1.137 ± 0.043	Y	3.090	[O III]	(5)	$8 . 8_{- 2.8}^{+ 3.3}$ $8.8_{-2.8}^{+3.3}$	$87_{- 31}^{+ 44}$ $87_{-31}^{+44}$
A11	22:17:37.05	00:18:22.2	28.9	0.853 ± 0.029	Y	3.091	CO(3−2), [O III]	(5)	$7 . 7_{- 3.3}^{+ 3.6}$ $7.7_{-3.3}^{+3.6}$	$142_{- 67}^{+ 98}$ $142_{-67}^{+98}$
A10	22:17:37.10	00:18:26.8	22.3	0.821 ± 0.054	Y	3.091	CO(3−2)	(1)	$1 . 2_{- 0.6}^{+ 1.2}$ $1.2_{-0.6}^{+1.2}$	$66_{- 26}^{+ 52}$ $66_{-26}^{+52}$
A14	22:17:31.33	00:16:39.6	24.1	0.805 ± 0.040	Y	3.098	CO(3−2), [O III]	(1)	$3 . 4_{- 1.8}^{+ 2.5}$ $3.4_{-1.8}^{+2.5}$	$84_{- 34}^{+ 58}$ $84_{-34}^{+58}$
A13	22:17:37.43	00:17:32.4	23.5	0.706 ± 0.039	Y	3.090	CO(3−2), [O III]	(1)	$5 . 3_{- 1.7}^{+ 1.8}$ $5.3_{-1.7}^{+1.8}$	$74_{- 28}^{+ 46}$ $74_{-28}^{+46}$
A9	22:17:36.54	00:16:22.6	29.1	0.689 ± 0.025	Y	3.094	CO(3−2), [O III]	(1), (5)	$15 . 5_{- 4.0}^{+ 4.4}$ $15.5_{-4.0}^{+4.4}$	$226_{- 81}^{+ 103}$ $226_{-81}^{+103}$
A17	22:17:37.67	00:18:14.6	13.8	0.675 ± 0.052	Y	3.091	CO(3−2)	(1)	$2 . 1_{- 1.1}^{+ 1.8}$ $2.1_{-1.1}^{+1.8}$	$67_{- 24}^{+ 44}$ $67_{-24}^{+44}$
A12	22:17:32.01	00:16:55.5	20.6	0.573 ± 0.030	Y	3.090	[O III]	(5)	$8 . 0_{- 1.8}^{+ 2.0}$ $8.0_{-1.8}^{+2.0}$	$54_{- 19}^{+ 39}$ $54_{-19}^{+39}$
A18	22:17:32.24	00:15:27.8	10.6	0.562 ± 0.061	Y	2.105	Lyα, N V, C IV, He II	(6)	$4 . 1_{- 1.8}^{+ 4.9}$ $4.1_{-1.8}^{+4.9}$	$148_{- 54}^{+ 48}$ $148_{-54}^{+48}$
A16	22:17:36.81	00:18:18.0	9.3	0.410 ± 0.058	Y	3.087	CO(3−2), [O III]	(1), (5)	$2 . 4_{- 1.1}^{+ 1.3}$ $2.4_{-1.1}^{+1.3}$	$63_{- 22}^{+ 36}$ $63_{-22}^{+36}$
A15	22:17:32.76	00:17:27.6	12.0	0.326 ± 0.036	Y	3.086	CO(3−2)	this work	$4 . 6_{- 2.1}^{+ 2.3}$ $4.6_{-2.1}^{+2.3}$	$79_{- 33}^{+ 48}$ $79_{-33}^{+48}$
A20	22:17:34.65	00:16:35.4	8.3	0.305 ± 0.037	Y	1.399	CO(2−1)	this work	$3 . 9_{- 1.2}^{+ 1.0}$ $3.9_{-1.2}^{+1.0}$	$43_{- 10}^{+ 45}$ $43_{-10}^{+45}$
A21	22:17:33.08	00:17:18.7	6.5	0.267 ± 0.039	Y	0.709	[O II], Hβ, [O III]	this work	$5 . 3_{- 1.2}^{+ 1.7}$ $5.3_{-1.2}^{+1.7}$	$46_{- 19}^{+ 49}$ $46_{-19}^{+49}$
A28	22:17:32.50	00:17:29.4	6.9	0.161 ± 0.029	Y	0.641	[O II], Hβ, [O III]	this work	$4 . 9_{- 1.1}^{+ 2.0}$ $4.9_{-1.1}^{+2.0}$	$11_{- 9}^{+ 20}$ $11_{-9}^{+20}$

New sources (S/N ≥ 5.0)

A34	22:17:31.12	00:17:15.7	14.4	0.424 ± 0.040	Y	$2 . 93_{- 0.66}^{+ 0.57}$ $2.93_{-0.66}^{+0.57}$	…	…	$2 . 4_{- 1.2}^{+ 1.8}$ $2.4_{-1.2}^{+1.8}$	$55_{- 22}^{+ 39}$ $55_{-22}^{+39}$
A35	22:17:30.55	00:18:33.6	5.1	0.366 ± 0.076	Y	$2 . 67_{- 0.20}^{+ 0.07}$ $2.67_{-0.20}^{+0.07}$	…	…	$4 . 5_{- 1.3}^{+ 0.9}$ $4.5_{-1.3}^{+0.9}$	$39_{- 16}^{+ 20}$ $39_{-16}^{+20}$
A36	22:17:38.63	00:15:40.1	6.4	0.360 ± 0.096	Y	1.397	CO(2−1)	this work	$9 . 7_{- 1.9}^{+ 1.6}$ $9.7_{-1.9}^{+1.6}$	$63_{- 30}^{+ 37}$ $63_{-30}^{+37}$
A37	22:17:29.74	00:17:15.0	6.4	0.349 ± 0.073	Y	$2 . 08_{- 0.02}^{+ 0.04}$ $2.08_{-0.02}^{+0.04}$	…	…	$2 . 1_{- 0.7}^{+ 0.9}$ $2.1_{-0.7}^{+0.9}$	$78_{- 27}^{+ 50}$ $78_{-27}^{+50}$
A38	22:17:30.52	00:18:05.5	12.5	0.372 ± 0.038	Y	3.087	CO(3−2)	this work	$2 . 5_{- 1.3}^{+ 2.6}$ $2.5_{-1.3}^{+2.6}$	$57_{- 22}^{+ 32}$ $57_{-22}^{+32}$
A41	22:17:31.76	00:17:43.7	6.9	0.298 ± 0.044	Y	3.098	CO(3−2)	this work	$1 . 2_{- 0.4}^{+ 0.3}$ $1.2_{-0.4}^{+0.3}$	$67_{- 19}^{+ 32}$ $67_{-19}^{+32}$
A42	22:17:31.06	00:15:38.5	5.4	0.248 ± 0.062	Y	$2 . 34_{- 0.05}^{+ 0.07}$ $2.34_{-0.05}^{+0.07}$	…	…	$2 . 0_{- 0.5}^{+ 0.5}$ $2.0_{-0.5}^{+0.5}$	$24_{- 10}^{+ 14}$ $24_{-10}^{+14}$
A43	22:17:32.11	00:17:28.4	7.4	0.262 ± 0.045	Y	0.641	[O II], Hβ, [O III]	this work	$3 . 8_{- 1.0}^{+ 0.8}$ $3.8_{-1.0}^{+0.8}$	$29_{- 10}^{+ 15}$ $29_{-10}^{+15}$
A44	22:17:38.05	00:17:59.9	8.7	0.259 ± 0.025	Y	$1 . 72_{- 0.07}^{+ 0.12}$ $1.72_{-0.07}^{+0.12}$	…	…	$2 . 8_{- 0.7}^{+ 1.1}$ $2.8_{-0.7}^{+1.1}$	$37_{- 9}^{+ 18}$ $37_{-9}^{+18}$
A45	22:17:33.75	00:15:29.9	5.8	0.234 ± 0.061	Y	$2 . 35_{- 0.12}^{+ 0.19}$ $2.35_{-0.12}^{+0.19}$	…	…	$4 . 8_{- 0.9}^{+ 0.6}$ $4.8_{-0.9}^{+0.6}$	$7_{- 4}^{+ 8}$ $7_{-4}^{+8}$
A46	22:17:34.59	00:17:54.5	8.6	0.241 ± 0.041	Y	1.511	Fe II, Mg II, Mg I	this work	$3 . 3_{- 0.9}^{+ 1.1}$ $3.3_{-0.9}^{+1.1}$	$61_{- 25}^{+ 46}$ $61_{-25}^{+46}$
A48	22:17:32.68	00:18:08.8	5.0	0.191 ± 0.041	Y	2.688	C II, C IV, C III]	this work	$7 . 8_{- 0.8}^{+ 0.9}$ $7.8_{-0.8}^{+0.9}$	$28_{- 10}^{+ 14}$ $28_{-10}^{+14}$
A49	22:17:30.74	00:17:06.5	8.0	0.209 ± 0.043	Y	$2 . 67_{- 0.38}^{+ 0.58}$ $2.67_{-0.38}^{+0.58}$	…	…	$6 . 5_{- 2.9}^{+ 3.5}$ $6.5_{-2.9}^{+3.5}$	$33_{- 18}^{+ 31}$ $33_{-18}^{+31}$
A50	22:17:37.45	00:17:00.7	5.3	0.187 ± 0.036	Y	$3 . 92_{- 0.13}^{+ 0.10}$ $3.92_{-0.13}^{+0.10}$	…	…	$1 . 6_{- 0.5}^{+ 0.6}$ $1.6_{-0.5}^{+0.6}$	$41_{- 14}^{+ 22}$ $41_{-14}^{+22}$
A52	22:17:30.50	00:17:36.8	6.8	0.195 ± 0.035	Y	$2 . 28_{- 0.03}^{+ 0.06}$ $2.28_{-0.03}^{+0.06}$	…	…	$3 . 8_{- 1.2}^{+ 0.7}$ $3.8_{-1.2}^{+0.7}$	$26_{- 9}^{+ 12}$ $26_{-9}^{+12}$
A54	22:17:37.58	00:16:10.3	5.0	0.175 ± 0.036	Y	$1 . 53_{- 0.03}^{+ 0.06}$ $1.53_{-0.03}^{+0.06}$	…	…	$0 . 2_{- 0.1}^{+ 0.1}$ $0.2_{-0.1}^{+0.1}$	$12_{- 5}^{+ 5}$ $12_{-5}^{+5}$
A55	22:17:34.80	00:17:02.7	5.8	0.158 ± 0.031	Y	$3 . 71_{- 1.36}^{+ 2.49}$ $3.71_{-1.36}^{+2.49}$	…	…	$2 . 3_{- 1.3}^{+ 1.7}$ $2.3_{-1.3}^{+1.7}$	$26_{- 13}^{+ 24}$ $26_{-13}^{+24}$

Tentative new sources (4.2 < S/N < 5.0)

A33	22:17:38.83	00:18:21.5	4.5	0.498 ± 0.140	L/N	…	…	…	…	…
A39	22:17:34.63	00:18:32.3	4.9	0.314 ± 0.079	Y	$0 . 47_{- 0.19}^{+ 0.91}$ $0.47_{-0.19}^{+0.91}$	…	…	$1 . 2_{- 1.1}^{+ 11.6}$ $1.2_{-1.1}^{+11.6}$	$21_{- 21}^{+ 41}$ $21_{-21}^{+41}$
A40	22:17:29.34	00:16:25.3	4.4	0.289 ± 0.079	N	…	…	…	…	…
A47	22:17:37.29	00:16:39.2	4.4	0.184 ± 0.040	Y	$2 . 85_{- 0.08}^{+ 0.13}$ $2.85_{-0.08}^{+0.13}$	…	…	$2 . 3_{- 0.4}^{+ 0.4}$ $2.3_{-0.4}^{+0.4}$	$19_{- 6}^{+ 12}$ $19_{-6}^{+12}$
A51	22:17:29.83	00:15:55.7	4.3	0.172 ± 0.049	N	…	…	…	…	…
A53	22:17:33.80	00:17:02.7	4.2	0.166 ± 0.059	Y	0.876	[O II]	this work	$2 . 6_{- 0.6}^{+ 0.7}$ $2.6_{-0.6}^{+0.7}$	$24_{- 8}^{+ 11}$ $24_{-8}^{+11}$
A56	22:17:30.22	00:18:02.0	4.6	0.135 ± 0.035	N	…	…	…	…	…
A57	22:17:35.00	00:15:29.6	4.8	0.135 ± 0.037	N	…	…	…	…	…
A58	22:17:37.04	00:18:02.0	4.5	0.119 ± 0.029	L/N	…	…	…	…	…
A59	22:17:31.58	00:17:01.8	4.3	0.116 ± 0.027	N	…	…	…	…	…
A60	22:17:35.80	00:17:28.8	4.7	0.100 ± 0.038	N	…	…	…	…	…
A61	22:17:32.12	00:18:23.9	4.3	0.078 ± 0.028	Y	$2 . 34_{- 0.07}^{+ 0.09}$ $2.34_{-0.07}^{+0.09}$	…	…	$2 . 2_{- 0.6}^{+ 0.5}$ $2.2_{-0.6}^{+0.5}$	$18_{- 7}^{+ 13}$ $18_{-7}^{+13}$
A62	22:17:36.35	00:17:50.1	4.4	0.074 ± 0.028	Y	$2 . 02_{- 1.57}^{+ 0.22}$ $2.02_{-1.57}^{+0.22}$	…	…	$0 . 6_{- 0.3}^{+ 0.2}$ $0.6_{-0.3}^{+0.2}$	$11_{- 5}^{+ 7}$ $11_{-5}^{+7}$
A63	22:17:34.74	00:16:20.1	4.6	0.072 ± 0.044	N	…	…	…	…	…
A64	22:17:31.56	00:17:06.1	4.3	0.065 ± 0.017	L/N	…	…	…	…	…

References. (1) Umehata et al. (2019); (2) Hayatsu et al. (2017); (3) Alaghband-Zadeh et al. (2013); (4) Umehata et al. (2020); (5) Steidel et al. (2014); (6) Chapman et al. (2004b)

^(a)

S/N> 3 in any of the NIR Ks or Spitzer IRAC1/2 bands, L indicates potential lensed source.

^(b)

When a spectral line detection is not available, we report photometric redshifts from the EAZY code.

^(c)

For SSA22 member galaxies with multiple spectral lines observed, we report the line(s) from which the redshift is measured.

^(d)

A* is the abbreviation of ADF22.

in Umehata et al. (2017).

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