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Table C.1.

List of protocluster and cluster galaxies from the literature.

Member zCO Line S​COΔv FWHM Tel. a LIR αCO Mgas Reference
Name (Jy km s−1) (km s−1) (1010 K km s−1 pc2) (1012 L⊙) (1010 M⊙)
Protoclusters
J1030+0524 (z = 1.694)
a0b 1.6984 2–1 0.88± 0.06 818±144 ALMA 3.36± 0.02 2.64±0.22 4.30 19.30± 0.10 1
a1 1.6966 2–1 0.07± 0.02 133± 38 ALMA 0.26± 0.07 0.11±0.03 4.30 1.50± 0.40 1
a2 1.6925 2–1 0.12± 0.03 447± 89 ALMA 0.47± 0.11 0.23±0.07 4.30 2.70± 0.60 1
a3 1.6864 2–1 0.22± 0.04 304±182 ALMA 0.84± 0.14 0.48±0.10 4.30 4.80± 0.75 1
GOODS-N (z = 1.990)
DSFG J123618+621550b 1.996 4–3 0.77± 0.12 ... PdBI 0.995±0.155 2.05±0.59 1.00 26.0± 6.0 2,3
DSFG J123618+621550 2.001 4–3 0.50± 0.08 ... PdBI 0.649±0.104 1.42±0.41 1.00 18.0± 4.0 2,3
DSFG J123711+621331b 1.988 4–3 1.02± 0.16 558±121 PdBI 1.308±0.205 2.06±1.07 1.00 3.6± 0.8 3,4
DSFG J123711+621331 1.996 4–3 0.61± 0.08 318± 86 PdBI 0.788±0.103 1.24±0.64 1.00 2.2± 0.5 3,4
DSFG J123711+621331b 1.995 3–2 0.70± 0.22 ... PdBI 1.606±0.505 2.38±1.23 1.00 3.4± 1.2 3,4
DSFG J123712+621322 1.996 3–2 1.20± 0.40 350±100 PdBI 2.756±0.919 1.60±1.09 1.00 1.9± 0.5 3,5
DSFG J123632+620800 1.994 3–2 1.80± 0.50 310±110 PdBI 4.127±1.146 0.38±0.92 1.00 8.9± 2.8 3,5
MRC1138−262 (z = 2.160)
HAE229b 2.1478 1–0 0.22± 0.02 359± 34 ATCA 5.00± 0.70 3.20 4.00 18.00± 2.00 6
1138.42 2.163 3–2 0.19± 0.04 185 ALMA 0.51± 0.11 0.43±0.13 10.81 16.22± 3.24 7
1138.48 2.157 3–2 0.42± 0.03 232 ALMA 1.12± 0.08 1.52±0.69 5.55 9.77± 0.56 7
1138.54b 2.148 3–2 0.88± 0.04 328 ALMA 2.34± 0.11 4.91±2.25 4.41 16.98± 0.88 7
1138.56 2.144 3–2 0.20± 0.04 224 ALMA 0.53± 0.11 0.38±0.12 9.64 12.02± 1.93 7
HELAISS02 (z = 2.171)
HELAISS02 S0b 2.17350 3–2 3.13± 0.30 931± 58 ALMA 7.90± 0.70 7.59±1.23 3.50 40.60± 3.85 8
HELAISS02 S1b 2.16434 3–2 0.53± 0.21 910±230 ALMA 1.30± 0.50 2.69±0.37 9.70 6.79± 1.94 8
HELAISS02 S2b 2.16850 3–2 0.91± 0.16 575± 78 ALMA 2.30± 0.40 3.02±0.49 5.60 11.76± 1.12 8
HELAISS02 S3 2.17397 3–2 0.51± 0.19 610±160 ALMA 1.30± 0.50 2.00±0.32 6.70 6.70± 1.34 8
HS 1700+64 (z = 2.30)
DRG55 2.296 3–2 1.14± 0.31 680±141 PdBI 3.60±1.00 2.09 4.36 32.0 ± 8.7 9
BOSS 1441 (z = 2.317)
G1A 2.3088 3–2 0.298±0.044 180±30 NOEMA 7.1±1.1 1.30±0.26 ... ... 10
G1A 2.3088 1–0 0.044±0.010 170±35 VLA 1.2±0.3 1.30±0.26 3.6 4.3±1.1 11
G2B 2.3123 3–2 0.237±0.051 370±90 NOEMA 6.7±1.4 0.51±0.11 ... ... 10
G2B 2.3123 1–0 0.042±0.006 85±20 VLA 1.1±0.2 0.51±0.11 3.6 4.0±0.7 11
G6C 2.3067 3–2 0.245±0.056 280±70 NOEMA 5.4±1.2 0.32±0.09 ... ... 10
G6C 2.3067 1–0 0.039±0.014 230±55 VLA 1.0±0.4 0.32±0.09 3.6 3.6±1.4 11
HATLAS J084933 (z = 2.410)
J084933 Wb 2.4066 1–0 0.49± 0.06 825±115 JVLA 13.80± 1.70 33.10±3.00 0.80 11.04± 1.36 12
J084933 Tb 2.4090 1–0 0.56± 0.07 610± 55 JVLA 15.70± 2.00 14.50±1.70 0.80 12.56± 1.60 12
J084933 Mb 2.4176 1–0 0.06± 0.01 320± 70 JVLA 1.60± 0.40 7.90±3.80 0.80 1.28± 0.32 12
J084933 Cb 2.4138 1–0 0.08± 0.01 250±100 JVLA 2.20± 0.40 6.30±3.00 0.80 1.76± 0.32 12
4C 23.56 (z = 2.490)
4C23.3 2.488 3–2 0.45± 0.08 482 ALMA 1.54± 0.27 1.92±0.88 4.6 12.88± 2.29 7
4C23.4b 2.490 3–2 0.33± 0.05 281 ALMA 1.13± 0.17 3.99±1.83 4.2 8.51± 1.29 7
4C23.8 2.486 3–2 0.50± 0.05 197 ALMA 1.71± 0.17 1.75±0.80 4.8 14.79± 1.48 7
4C23.9b 2.485 3–2 0.77± 0.11 739 ALMA 2.63± 0.38 3.35±1.54 5.1 23.99± 3.43 7
4C23.10 2.485 3–2 0.47± 0.09 303 ALMA 1.61± 0.31 1.04±0.34 5.5 15.85± 3.03 7
4C23.16 2.484 3–2 0.70± 0.12 544 ALMA 2.39± 0.41 2.16±0.99 5.6 23.99± 4.11 7
HAE3 2.4861 3–2 0.35± 0.06 500 ALMA 1.20± 0.20 1.85±0.82 4.71 10.36± 1.88 13
HAE4b 2.4780 3–2 0.25± 0.03 300 ALMA 0.84± 0.10 4.35±1.84 4.41 7.06± 0.88 13
HAE5b 2.4873 3–2 0.09± 0.02 100 ALMA 0.31± 0.07 3.93±1.47 5.48 3.29± 0.55 13
HAE8 2.4861 3–2 0.26± 0.03 300 ALMA 0.90± 0.10 1.64±0.66 5.19 8.82± 1.04 13
HAE9 2.4861 3–2 0.54± 0.06 1000 ALMA 1.85± 0.20 0.94±0.42 5.35 18.19± 2.14 13
HAE10 2.4861 3–2 0.36± 0.06 500 ALMA 1.24± 0.20 1.21±0.49 5.72 13.16± 2.29 13
HAE16 2.4826 3–2 0.49± 0.07 600 ALMA 1.68± 0.24 0.80±0.34 5.94 18.41± 2.38 13
CL J1001 (z = 2.510)c
S6 2.49391 1–0 0.078±0.006 519± 71 ALMA 2.24± 0.20 ... 3.5 7.84± 0.70 8
S8 2.50400 1–0 0.025±0.009 370±100 ALMA 0.72± 0.30 ... 3.5 2.52± 1.05 8
S12 2.51225 1–0 0.031±0.013 720±230 ALMA 0.91± 0.40 ... 3.5 3.19± 1.40 8
3 (S5) 2.514 1–0 ... 280±120 JVLA 0.60± 0.10 0.76±0.44 4.08 2.45± 0.41 14
4 2.501 1–0 ... 690±160 JVLA 0.60± 0.10 1.23±0.55 4.08 2.45± 0.41 14
5 (S11) 2.508 1–0 ... 240± 40 JVLA 2.70± 0.40 2.75±0.96 4.08 11.02± 1.63 14
6b 2.494 1–0 ... 550± 40 JVLA 4.90± 0.40 7.41±2.59 4.09 20.04± 1.64 14
7 (S10) 2.505 1–0 ... 680±160 JVLA 2.80± 0.80 1.20±0.62 4.09 11.45± 3.68 14
8b 2.513 1–0 ... 340± 20 JVLA 3.20± 0.30 4.17±1.45 4.10 13.12± 1.23 14
9 2.500 1–0 ... 90± 40 JVLA 0.50± 0.10 0.93±0.51 4.10 2.05± 0.41 14
10 2.506 1–0 ... 690±370 JVLA 1.00± 0.30 0.60±0.47 4.10 4.10± 1.23 14
11 2.506 1–0 ... 600±190 JVLA 12.70± 4.20 1.86±0.83 4.10 52.07±17.22 14
12 (S7) 2.515 1–0 ... 90± 30 JVLA 0.30± 0.10 0.13±0.07 4.11 1.23± 0.41 14
13 (S9) 2.505 1–0 ... 530± 80 JVLA 2.00± 0.30 2.04±1.19 4.11 8.22± 1.23 14
14 2.515 1–0 ... 140± 30 JVLA 13.40± 2.70 0.89±0.69 4.12 54.80±11.12 14
ID1 (S0)b 2.494 1–0 0.1220±0.0064 486± 36 ALMA 3.55± 0.16 7.41±2.25 6.5 22.96± 0.74 15
ID1 (S0)b 2.494 3–2 1.2610±0.1430 532± 78 ALMA 4.07± 0.47 7.41±2.25 6.5 0.00± 0.00 15
ID2 2.496 1–0 0.0390±0.0039 532± 54 ALMA 1.12± 0.13 ... 6.5 7.35± 0.45 15
ID3 (S3) 2.503 1–0 0.0463±0.0069 1271±143 ALMA 1.35± 0.22 1.23±0.46 6.5 8.76± 0.81 15
ID4 (S2)b 2.504 1–0 0.0926±0.0126 1095±135 ALMA 2.69± 0.37 4.17±1.27 6.5 17.53± 1.47 15
ID5 2.507 1–0 0.0374±0.0051 172± 71 VLA 1.10± 0.15 ... 6.5 7.10± 0.59 15
ID6 (S4) 2.509 1–0 0.0500±0.0070 981±145 ALMA 1.45± 0.23 1.10±0.55 6.5 9.50± 0.82 15
ID7 (S1)b 2.511 1–0 0.0641±0.0064 619± 56 ALMA 1.86± 0.21 4.17±1.27 6.5 12.19± 0.75 15
USS 1558−003 (z = 2.510)
bHAE-191 2.5145 1–0 0.052±0.008 251 JVLA 1.50± 0.00 2.50 0.80 1.20± 0.00 16
rHAE-193 2.5134 1–0 0.096±0.015 437 JVLA 2.80± 0.00 5.10 0.80 2.24± 0.00 16
rHAE-213 2.5300 1–0 0.026±0.007 294 JVLA 0.80± 0.00 1.70±1.70 0.80 0.64± 0.00 16
1558.43 2.528 3–2 0.26± 0.04 698 ALMA 0.92± 0.14 0.69±0.22 4.18 6.92± 1.06 7
1558.54 2.515 3–2 0.23± 0.02 242 ALMA 0.80± 0.07 0.71±0.21 6.94 10.00± 0.87 7
1558.59 2.513 3–2 0.49± 0.02 420 ALMA 1.71± 0.07 0.93±0.27 4.92 15.14± 0.62 7
1558.64 2.529 3–2 0.21± 0.04 721 ALMA 0.74± 0.14 0.53±0.16 26.03 34.67± 6.60 7
1558.73 2.526 3–2 0.19± 0.03 261 ALMA 0.67± 0.11 1.12±0.33 6.74 8.13± 1.28 7
1558.137 2.525 3–2 0.16± 0.02 264 ALMA 0.56± 0.07 1.03±0.31 5.71 5.75± 0.72 7
HXMM20 (z = 2.602)
HXMM20 S0b 2.60226 1–0 0.32± 0.05 688± 81 ALMA 10.00± 1.60 6.61±0.92 2.90 34.67± 5.61 8
HXMM20 S1b 2.59757 1–0 0.12± 0.04 278± 63 ALMA 3.70± 1.20 3.80±0.44 3.70 12.88± 4.23 8
HXMM20 S2 2.60201 1–0 0.16± 0.05 490±110 ALMA 5.00± 1.60 3.47±0.48 2.40 17.38± 5.70 8
HXMM20 S3b 2.60315 3–2 1.57± 0.21 484± 45 ALMA 5.40± 0.70 4.37±3.14 1.20 27.54± 4.46 8
HXMM20 S4 2.59682 1–0 0.15± 0.05 590±230 ALMA 4.70± 1.50 1.00±0.14 0.80 16.22± 5.32 8
B3 J2330 (z = 3.090)
JVLA J233024+392708b 3.0884 1–0 0.162±0.034 720±170 VLA 6.90± 1.50 8.97±0.47 0.80 5.52± 1.20 17
JVLA J233024+392708b 3.0901 4–3 1.12± 0.17 520±110 VLA 3.05± 0.46 8.97±0.47 0.80 5.52± 1.20 17
JVLA J233024+392708b 3.0934 4–3 3.29± 0.51 830±100 VLA 8.97± 1.39 17.61±0.49 0.80 17.50± 2.71 17
SSA22 (z = 3.090)
J221735.15+001537.3 3.09630 3–2 0.70± 0.20 560±110 PdBI 6.30± 1.60 6.17 1.00 6.30± 2.20 5
ALMA1+ALMA2+ALMA5 3.0982 4–3 0.44± 0.03 322± 29 ALMA 1.203±0.082 1.05±0.34 3.60 6.8± 1.5 18
ALMA3 3.0989 4–3 0.12± 0.02 316± 65 ALMA 0.328±0.055 0.97±0.31 3.60 1.7± 0.5 18
GOODSN (z = 3.140)
GN CL 2 3.148 5–4 1.59± 0.07 369± 23 NOEMA 2.93± 0.14 6.63±0.32 1.36 13.00± 2.00 19
GN CL 3 3.132 5–4 1.50± 0.10 500± 41 NOEMA 2.75± 0.18 4.11±1.47 1.36 12.00± 2.00 19
Clusters
7C 1756+6520 (z = 1.420)
AGN 1317 1.4161 2–1 0.52± 0.06 254± 33 PdBI 1.36±0.15 0.68 0.8 1.30±0.14 20
XCS J2215 (z = 1.460)
XCS J2215 03 1.453 2–1 0.50± 0.10 530± 90 ALMA 1.46±0.29 0.88 ±0.33 3.5 6.08 ±1.21 21
XCS J2215 06 1.454 2–1 0.25± 0.08 130± 30 ALMA 0.73±0.23 0.94 ±0.22 3.5 3.04 ±0.96 21
XCS J2215 07 1.450 2–1 0.19± 0.09 190±120 ALMA 0.55±0.26 0.36 ±0.20 3.5 2.29 ±1.08 21
XCS J2215 08 1.466 2–1 0.60± 0.10 460± 90 ALMA 1.79±0.30 0.33 ±0.10 3.5 7.46 ±1.25 21
XCS J2215 11 1.467 2–1 0.40± 0.10 390± 90 ALMA 1.19±0.30 0.55 ±0.22 3.5 4.96 ±1.25 21
XCS J2215 13 1.472 2–1 0.30± 0.10 370± 90 ALMA 0.90±0.30 0.24 ±0.12 3.5 3.75 ±1.25 21
ALMA.B3.01 1.466 2–1 ... 370± 20 ALMA 1.99±0.11 0.37 ±0.37 6.09 4.26 ±0.61 22
ALMA.B3.02 1.450 2–1 ... 310± 80 ALMA 0.45±0.09 0.33 ±0.16 5.03 2.52 ±0.50 22
ALMA.B3.03 1.453 2–1 ... 490± 30 ALMA 2.16±0.12 0.26 ±0.22 4.29 3.00 ±0.43 22
ALMA.B3.04 1.466 2–1 ... 480±110 ALMA 0.62±0.12 0.06 ±0.03 5.78 6.36 ±0.58 22
ALMA.B3.05 1.467 2–1 ... 250± 60 ALMA 0.47±0.09 0.50 ±0.27 4.35 5.65 ±0.44 22
ALMA.B3.06b 1.467 2–1 ... 490± 40 ALMA 2.12±0.12 1.52 ±0.72 4.18 10.87 ±0.84 22
ALMA.B3.07 1.452 2–1 ... 480± 70 ALMA 1.10±0.12 0.37 ±0.51 4.88 8.30 ±0.49 22
ALMA.B3.08b 1.457 2–1 ... 360± 40 ALMA 1.22±0.10 1.10 ±0.31 4.58 6.87 ±0.46 22
ALMA.B3.09 1.468 2–1 ... 350± 70 ALMA 0.68±0.10 0.49 ±0.28 5.41 5.95 ±0.54 22
ALMA.B3.10 1.454 2–1 ... 270± 20 ALMA 1.40±0.09 0.76 ±0.29 4.98 6.47 ±0.50 22
ALMA.B3.11 1.451 2–1 ... 530±100 ALMA 0.96±0.12 0.18 ±0.30 5.15 8.76 ±0.52 22
ALMA.B3.12 1.445 2–1 ... 210± 30 ALMA 0.56±0.08 0.57 ±0.16 4.92 3.94 ±0.49 22
ALMA.B3.13 1.471 2–1 ... 520± 70 ALMA 1.06±0.12 0.22 ±0.58 4.36 10.46 ±0.44 22
ALMA.B3.14 1.451 2–1 ... 480±100 ALMA 0.62±0.11 0.03 4.16 10.40 ±0.83 22
ALMA.B3.15 1.465 2–1 ... 520± 90 ALMA 1.09±0.12 0.29 ±0.10 5.50 3.30 ±0.55 22
ALMA.B3.16 1.465 2–1 ... 590± 80 ALMA 1.36±0.13 0.39 ±0.30 4.21 3.37 ±0.42 22
ALMA.B3.17b 1.460 2–1 ... 440± 80 ALMA 0.89±0.11 1.29 ±0.54 4.56 5.93 ±0.91 22
COSMOS1002+0134 (z = 1.550)
51613 1.517 1–0 0.20± 0.05 200± 80 JVLA 2.42±0.58 0.57 3.60 8.64 ±2.16 23
51858 1.556 1–0 0.10± 0.03 360±220 JVLA 1.26±0.38 0.95 3.60 4.32 ±1.44 23
51207 1.530 1–0 0.085±0.021 300 JVLA 1.03±0.25 0.49 ±0.28 3.60 3.70 ±0.90 23
51380 1.551 1–0 0.090±0.021 300 JVLA 1.12±0.26 0.33 ±0.17 3.60 4.00 ±0.94 23
SpARCS J022546−035517 (z = 1.590)
J0225−371b 1.599 2–1 1.26± 0.10 442± 39 ALMA 5.30±0.40 1.82 ±0.80 4.36 10.03 ±2.62 24
J0225−460b 1.600 2–1 0.50± 0.05 388± 44 ALMA 2.10±0.20 1.22 ±0.63 4.36 23.11 ±1.74 24
J0225−281b 1.611 2–1 0.80± 0.08 292± 34 ALMA 3.40±0.30 1.26 ±0.53 4.36 4.80 ±0.87 24
J0225−541 1.611 2–1 1.12± 0.26 341± 89 ALMA 4.80±1.10 0.86 ±0.32 4.36 9.16 ±0.87 24
J0225−429b 1.602 2–1 0.25± 0.05 283± 65 ALMA 1.10±0.20 1.87 ±0.87 4.36 1.74 ±0.44 24
J0225−407 1.599 2–1 0.26± 0.04 290± 57 ALMA 1.10±0.20 0.88 ±0.29 4.36 4.80 ±0.87 24
J0225−324 1.600 2–1 0.09± 0.02 193± 61 ALMA 0.40±0.10 0.51 ±0.28 4.36 14.82 ±1.31 24
J0225−303 1.596 2–1 0.55± 0.15 687±222 ALMA 2.30±0.60 0.03 ±0.03 4.36 20.93 ±4.80 24
SpARCS J033057−284300 (z = 1.613)
J0330−57 1.613 2–1 0.31± 0.13 155± 40 ALMA 1.40±0.60 0.38 ±0.22 4.36 6.10 ±2.62 25
SpARCS J022426−032330 (z = 1.630)
J0224−3656 1.626 2–1 0.30± 0.06 539±113 ALMA 1.30±0.30 0.45 ±0.21 4.36 5.67 ±1.31 25
J0224−159b 1.635 2–1 0.46± 0.11 245± 68 ALMA 2.00±0.50 2.28 ±0.86 4.36 8.72 ±2.18 25
J0224−3680/3624 1.626 2–1 1.07± 0.19 776±192 ALMA 4.70±0.80 0.72 ±0.25 4.36 20.49 ±3.49 25
J0224−396/424b 1.634 2–1 1.32± 0.12 493± 53 ALMA 5.80±0.60 1.75 ±0.63 4.36 25.29 ±2.62 25
CLG J0218−0510 (z = 1.630)
30169 1.629 1–0 0.06± 0.01 836 VLA 0.76±0.18 0.29 ±0.12 4.36 3.49 ±0.44 26
30545b 1.624 1–0 0.19± 0.01 351± 12 VLA 2.55±0.18 1.70 ±0.70 4.36 11.34 ±0.44 26
SpARCS 1049+56 (z = 1.710)
SpARCS 1049+56 BCGb 1.7091 2–1 3.60± 0.30 569± 63 LMT 11.60±1.00 9.03 ±1.37 0.80 11.04 ±0.96 27
Cl J1449+0856 (z = 1.990)
A1b 1.9902 4–3 474.00±67.00 619±111 ALMA 0.62±0.09 2.38 ±0.23 3.6 6.12 ±0.36 28
A2 1.9951 4–3 307.00±54.00 387± 89 ALMA 0.40±0.07 0.89 ±0.23 3.5 3.42 ±0.60 29
H13 1.9944 4–3 148.00±38.00 343± 93 ALMA 0.19±0.05 0.40 ±0.12 4.5 1.78 ±1.78 29
H6 1.9832 4–3 178.00±50.00 541±162 ALMA 0.23±0.06 1.24 ±0.13 4.2 2.75 ±0.90 29
N7 1.9965 4–3 116.00±31.00 302±115 ALMA 0.15±0.04 0.27 4.2 1.26 ±1.26 29
B1 1.9883 4–3 62.00±28.00 533±213 ALMA 0.08±0.04 0.60 ±0.13 3.9 1.51 ±0.76 29
H3 1.9903 4–3 70.00±24.00 252± 83 ALMA 0.09±0.03 0.24 ±0.09 4.7 1.35 ±1.35 29

Notes.

(a)

The CO luminosity refers to the listed transition. Gas masses are obtained by multiplying by the reported αCO value. is obtained from the measured and the brightness temperature ratios from Bothwell et al. (2013).

(b)

Source selected for the comparison with the PHz-IRAM sample because CO detected and with log(LIR) > 11.44+0.5×z.

(c)

The ALMA data of the galaxy members in CL J1001 have been analyzed by both Gómez-Guijarro et al. (2019), and Champagne et al. (2021). In the case of objects in common, the measurements from the latter work were reported, but the identifier from Gómez-Guijarro et al. (2019) is added in parenthesis (e.g., S#). In the case of an object that was also observed with the JVLA by Wang et al. (2018), we report the JVLA data and add the identifier from Gómez-Guijarro et al. (2019) in parenthesis.

References. (1) D’Amato et al. (2020); (2) Bothwell et al. (2010); (3) Casey (2016); (4) Casey et al. (2011); (5) Bothwell et al. (2013); (6) Dannerbauer et al. (2017); (7) Tadaki et al. (2019); (8) Gómez-Guijarro et al. (2019); (9) Chapman et al. (2015); (10) Li et al. (2021); (11) Emonts et al. (2019); (12) Ivison et al. (2013); (13) Lee et al. (2017); (14) Wang et al. (2018); (15) Champagne et al. (2021); (16) Tadaki et al. (2014); (17) Ivison et al. (2012); (18) Umehata et al. (2021); (19) Jones et al. (2021); (20) Casasola et al. (2013); (21) Stach et al. (2017); (22) Hayashi et al. (2017); (23) Aravena et al. (2012); (24) Noble et al. (2019); (25) Noble et al. (2017); (26) Rudnick et al. (2017); (27) Webb et al. (2017); (28) Gobat et al. (2011); (29) Coogan et al. (2018).

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