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Home All issues Volume 658 (February 2022) A&A, 658 (2022) A43 Full HTML
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Table 2.

Source catalog: 100% pure.

ID α (J2000) δ (J2000) IDZF z log(M*/M⊙) S/Npeak S1.1 mm θ High-res Low-res Other ID
(deg) (deg) (mJy) (arcsec)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
A2GS1 53.118813 −27.782884 17856 2.309 (a) 11.06 18.78 2.15 ± 0.11 0.18 ± 0.02 Yes/100pur Yes/100pur AGS1,AS2,SG5,GS6
A2GS2 53.142840 −27.827895 12333 3.556 (b) 11.09 18.65 2.25 ± 0.12 0.20 ± 0.02 Yes/100pur Yes/100pur AGS4,SG12
A2GS3 53.148870 −27.821185 13086 2.582 (c) 11.44 18.11 2.11 ± 0.11 0.17 ± 0.02 Yes/100pur Yes/100pur AGS3,AS3,SG9,GS5
A2GS4 53.063887 −27.843804 10316 2.918 (d) 10.76 17.19 2.06 ± 0.10 0.17 ± 0.01 Yes/100pur Yes/100pur AGS2,SG3
A2GS5 53.020352 −27.779931 18282 1.797 (d) 11.09 15.80 2.75 ± 0.09 0.35 ± 0.03 Yes/100pur Yes/100pur AGS8,SG4,LESS18
A2GS6 53.158397 −27.733588 23898 3.46 11.14 14.55 2.15 ± 0.12 0.19 ± 0.02 Yes/100pur Yes/100pur AGS5,SG7
A2GS7 53.079416 −27.870820 6964 3.467 (b) 10.52 14.21 2.05 ± 0.12 0.48 ± 0.04 Yes/100pur Yes/100pur AGS17,SG11,LESS10
A2GS8 53.082752 −27.866560 7867 3.29 11.44 12.07 1.40 ± 0.12 0.13 ± 0.02 Yes/Prior Yes/100pur AGS7,SG16
A2GS9 53.181383 −27.777572 18645 2.696 (e) 10.90 11.12 1.41 ± 0.13 0.29 ± 0.05 Yes/Prior Yes/100pur AGS18,AS4,UDF2,C06,SG25
A2GS10 53.074868 −27.875889 6755 3.47 10.56 10.91 1.67 ± 0.10 0.11 ± 0.02 Yes/Prior Yes/100pur AGS15,SG13,LESS34
A2GS11 53.082069 −27.767279 19833 2.41 11.33 10.39 1.34 ± 0.11 0.21 ± 0.03 Yes/Prior Yes/100pur AGS10,SG10
A2GS12 53.092818 −27.801328 15639 3.847 (f) 10.87 9.66 1.39 ± 0.10 0.21 ± 0.03 Yes/Prior Yes/100pur AGS9,SG18
A2GS13 53.157199 −27.833492 11442 1.619 (g) 10.96 9.30 1.36 ± 0.12 0.44 ± 0.08 Yes/Prior Yes/100pur AGS26,SG23,GS7
A2GS14 53.071752 −27.843698 10241 1.956 (c) 11.19 8.30 0.83 ± 0.10 0.31 ± 0.06 Yes/Prior Yes/100pur AGS37,SG30,GS4
A2GS15 53.108810 −27.869037 7589 3.47 10.24 8.08 1.24 ± 0.10 < 0.13 Yes/Prior Yes/100pur AGS11,SG19
A2GS16 53.068881 −27.879724 6153 2.45 11.39 8.03 1.03 ± 0.11 0.16 ± 0.03 Yes/Prior Yes/100pur AGS31,SG43
A2GS17 53.183697 −27.836500 11353 4.64 10.39 7.96 1.23 ± 0.12 0.25 ± 0.05 Yes/Prior Yes/100pur AGS25,SG58
A2GS18 53.070260 −27.845595 10152 3.689 (h) 10.56 7.73 0.83 ± 0.09 0.14 ± 0.03 Yes/Prior Yes/100pur AGS21,SG26
A2GS19 53.131138 −27.773202 19033 2.225 (i) 11.43 7.56 0.72 ± 0.11 < 0.13 Yes/Prior Yes/100pur AGS13,AS8,SG40
A2GS20 53.049739 −27.770990 19463 2.68 10.72 7.49 0.93 ± 0.10 < 0.13 No Yes/100pur AGS33,SG32
A2GS21 53.183469 −27.776661 18658 2.698 (e) 10.30 7.27 1.49 ± 0.13 < 0.14 Yes/100pur Yes/100pur AGS6,AS1,UDF1,SG22
A2GS22 53.092372 −27.826850 12416 2.72 10.77 6.87 1.07 ± 0.09 0.17 ± 0.03 Yes/Prior Yes/100pur AGS20,SG14
A2GS23 53.121858 −27.752778 21730 2.00 10.76 6.68 0.73 ± 0.14 < 0.14 No Yes/100pur AS11
A2GS24 53.092391 −27.803269 15342 2.32 11.38 6.66 0.85 ± 0.11 0.28 ± 0.06 No Yes/100pur SG38
A2GS25 53.160620 −27.776287 18701 2.543 (j) 10.13 6.65 0.99 ± 0.12 0.17 ± 0.05 Yes/Prior Yes/100pur AGS12,AS5,UDF3,C01,SG48
A2GS26 53.090782 −27.782492 17976 1.927 (d) 10.64 6.55 0.76 ± 0.09 < 0.14 No Yes/100pur SG34
A2GS27 53.111595 −27.767864 19964 4.72 11.01 6.49 0.64 ± 0.12 0.22 ± 0.06 No Yes/Prior AGS32
A2GS28 53.137093 −27.761411 (…) 1.967 (d) 10.71 6.49 0.92 ± 0.10 0.17 ± 0.05 No Yes/100pur AS7,SG29
A2GS29 53.087184 −27.840242 (…) 3.47 11.32 6.41 0.85 ± 0.11 < 0.15 Yes/Prior Yes/100pur AGS24,SG44
A2GS30 53.048384 −27.770312 (…) 3.80 11.46 6.31 0.71 ± 0.11 1.66 ± 0.31 No Yes/100pur SG55
A2GS31 53.224499 −27.817250 13388 2.15 11.18 6.21 0.79 ± 0.11 0.28 ± 0.08 Yes/Prior Yes/Prior AGS28
A2GS32 53.077331 −27.859632 8449 2.251 (d) 11.55 6.02 0.51 ± 0.10 < 0.15 No Yes/Prior SG31
A2GS33 53.120402 −27.742111 (…) (…) (…) 5.91 0.95 ± 0.12 0.95 ± 0.30 No No AS20,SG68
A2GS34 53.131474 −27.841396 10345 1.613 (g) 11.43 5.86 0.74 ± 0.10 0.41 ± 0.11 No Yes/100pur SG65
A2GS35 53.069006 −27.807141 14926 4.73 10.94 5.72 0.72 ± 0.11 0.60 ± 0.16 Yes/Prior Yes/100pur AGS27
A2GS36 53.086635 −27.810257 14543 2.36 11.27 5.69 0.49 ± 0.10 0.17 ± 0.05 Yes/Prior Yes/Prior AGS23,SG36
A2GS37 53.119994 −27.743167 22905 3.85 11.16 5.66 0.71 ± 0.12 0.66 ± 0.20 No Yes/100pur SG72
A2GS38 53.206064 −27.819142 (…) (…) (…) 5.55 0.70 ± 0.13 (…) No Yes/100pur AS17
A2GS39 53.091617 −27.853421 9248 2.36 10.61 5.44 0.81 ± 0.10 0.33 ± 0.10 No Yes/Prior AGS39,SG42
A2GS40 53.196569 −27.757065 21234 2.46 10.21 5.44 0.62 ± 0.12 < 0.16 No Yes/Prior AS9
A2GS41 53.154105 −27.790947 16952 1.759 (d) 10.54 5.30 0.79 ± 0.12 0.30 ± 0.10 No Yes/100pur AS12,UDF5,C02
A2GS42 53.154440 −27.738686 23441 2.29 11.12 5.25 0.80 ± 0.11 0.42 ± 0.13 No Yes/100pur
A2GS43 53.076655 −27.873394 6921 3.54 10.54 5.12 0.70 ± 0.10 0.87 ± 0.21 No Yes/100pur
A2GS44 53.102654 −27.860660 8455 4.19 11.05 5.00 0.76 ± 0.10 0.42 ± 0.13 No Yes/100pur

Notes. (1) ALMA source ID; (2) right ascension (J2000) in degrees of the ALMA source as detected by PyBDSF; (3) declination (J2000) in degrees of the ALMA source as detected by PyBDSF; (4) ID associated to the stellar counterpart in the ZFOURGE catalog (5) redshift with spectroscopic redshifts shown with three decimal digits; (6) stellar mass; (7) detection signal to noise ratio from PyBDSF, measured as the peak flux density over the local rms noise; (8) 1.1 mm flux density measured using a diameter aperture corrected from aperture losses and flux boosting; (9) source size given by the FWHM of a circular Gaussian model fit in the uv plane; (10) and (11) source presence in the high/low resolution datasets (Yes or No) and whether it was detected as a 100% pure source or using priors (100pur or Prior) in those datasets; (12) source ID in other surveys: AGS (GOODS-ALMA; Franco et al. 2018, 2020b); AS (ASAGAO; Hatsukade et al. 2018), UDF (Dunlop et al. 2017); C (ASPECS; Aravena et al. 2020); SG (SUPER GOODS; Cowie et al. 2018); LESS (Hodge et al. 2013); GS (Elbaz et al. 2018). Spectroscopic redshift references: (a) Kurk et al. (2013); (b) Zhou et al. (2020); (c) Wuyts et al. (2009); (d) Momcheva et al. (2016); (e) Decarli et al. (2019); (f)B. Mobasher, priv. comm.; (g) Vanzella et al. (2008); (h) Garilli et al. (2021); (i) Kriek et al. (2008); (j) Inami et al. (2017).

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