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Table 1.

Properties of the CO or continuum-detected galaxies in the massive protoclusters of NICE-COSMOS.

Structure ID r/Rvir zspec log10M SFR αCO log 10 M gas RJ $ _{10}M_{\mathrm{gas}}^{\mathrm{RJ}} $ log 10 M gas CO $ _{10}M_{\mathrm{gas}}^{\mathrm{CO}} $ SFRradio SFR24 μm
[M] [M yr−1] [M (K km s−1 pc2)−1] [M] [M] [M yr−1] [M yr−1]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
HPC1001 ...* 0.07 3.613 11.2 0.2 + 0.2 $ ^{+0.2}_{-0.2} $ 662 66 + 65 $ ^{+65 }_{-66 } $ 3.59 11.48±0.07 11.30±0.04 125±41 978±883
HPC1001 1272853 1.12 3.604 11.3 0.2 + 0.1 $ ^{+0.1}_{-0.2} $ 496 241 + 290 $ ^{+290}_{-241} $ 3.62 ... 10.87±0.10 ... ...
HPC1001 1274387 0.78 3.61 10.3 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 68 20 + 69 $ ^{+69 }_{-20 } $ 4.59 11.26±0.18 10.84±0.10 < 159 ...

COS-SBC3 1340799 0.30 2.365 11.5 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 190 61 + 90 $ ^{+90 }_{-61 } $ 3.52 11.41±0.12 10.84±0.07 < 138 231±13

COS-SBC4 840072 0.04 1.65 11.4 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 100 18 + 18 $ ^{+18}_{-18} $ 3.54 11.21±0.12 ... 165±12 252±20

COS-SBC6 835289 0.07 2.323 11.1 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 73 19 + 15 $ ^{+15 }_{-19 } $ 3.62 10.95±0.16 10.99±0.05 101±20 289±17
COS-SBC6 839791** 0.10 2.324 11.0 0.1 + 0.0 $ ^{+0.0}_{-0.1} $ 93 6 + 6 $ ^{+6 }_{-6 } $ 4.01 11.51±0.04 11.03±0.05 1143±60 195±25

COS-SBCX1 1408110 0.29 2.422 11.4 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 156 31 + 30 $ ^{+30 }_{-31 } $ 3.54 11.07±0.15 11.03±0.05 134±16 183±33

COS-SBCX3 1088927 0.04 3.032 10.5 0.2 + 0.1 $ ^{+0.1}_{-0.2} $ 100 90 + 45 $ ^{+45 }_{-90 } $ 4.78 11.28±0.15 11.09±0.05 495±56 472±76
COS-SBCX3 1088787 0.11 3.03 10.7 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 53 12 + 40 $ ^{+40 }_{-12 } $ 4.31 11.17±0.19 11.25±0.04 490±57 284±114

COS-SBCX4 1049510 0.07 2.642 11.1 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 257 186 + 83 $ ^{+83 }_{-186} $ 3.62 10.94±0.22 10.78±0.07 < 123 137±31
COS-SBCX4 1050531 0.05 2.647 11.2 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 416 265 + 135 $ ^{+135}_{-265} $ 3.69 11.66±0.04 11.43±0.02 533±37 496±51
COS-SBCX4 1049929 0.14 2.648 10.9 0.2 + 0.2 $ ^{+0.2}_{-0.2} $ 195 101 + 120 $ ^{+120}_{-101} $ 3.78 10.80±0.31 10.67±0.07 < 141 ...

COS-SBCX7 392639 0.75 2.413 10.3 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 114 112 + 25 $ ^{+25 }_{-112} $ 4.66 ... 11.00±0.12 < 84 36±17
COS-SBCX7 394944 0.14 2.416 11.1 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 92 25 + 70 $ ^{+70 }_{-25 } $ 3.60 11.22±0.12 10.89±0.06 < 87 184±16
COS-SBCX7 394609 0.01 2.416 10.8 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 14 4 + 11 $ ^{+11 }_{-4 } $ 3.93 11.24±0.11 11.03±0.05 186±24 239±17
COS-SBCX7 392257 0.15 2.415 10.7 0.1 + 0.1 $ ^{+0.1}_{-0.1} $ 91 49 + 61 $ ^{+61 }_{-49 } $ 4.10 10.81±0.34 10.86±0.07 212±25 122±17

Notes. Columns: (1)–(6) protocluster ID, galaxy ID in COSMOS2020 (Weaver et al. 2022), distance to protocluster center, redshift, stellar mass, and SFR as given in Sillassen et al. (2024). (7) CO-to-H2 conversion factor. (8) & (9) Molecular gas masses from dust continuum and from CO. (10) SFR from 3GHz observations, with 3σ upper limits for nondetections. (11) SFR from 24 μm fluxes adopting conversion factors from Wuyts et al. (2008). For details, see Section 2. *: This source could be a blend of several galaxies (Sillassen et al. 2022). **: Radio-loud galaxy.

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