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Table 2.

Derived properties of the OFGs.

ID RA Dec H [4.5] S1.13 mm z log(M) log(LIR) SFR Other ID
(deg) (deg) (mag) (mag) (mJy) log(M) log(L) (M yr−1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
OFG1 53.087184 ( † ) −27.840242 ( † ) (...) 22.10 0.85 ± 0.11 3.47o 10.79 12.41 ± 0.05 384 ± 48 AGS24, A2GS29
OFG2 53.108810 ( † ) −27.869037 ( † ) (...) 23.72 1.24 ± 0.10 3.47o 10.76 12.39 ± 0.03 365 ± 30 AGS11, A2GS15
OFG3 53.102536 −27.806531 (...) 23.75 (...) 7.04 10.91 (...) (...) (...)
OFG4 53.206064 ( † ) −27.819142 ( † ) (...) 25.16 0.70 ± 0.13 6.13 10.60 12.56 ± 0.07 537 ± 100 A2GS38
OFG5 53.119150 ( † ) −27.814066 ( † ) (...) 23.34 0.43 ± 0.13 3.81 10.17 12.26 ± 0.09 268 ± 61 A2GS87, GDS44539
OFG6 53.197493 −27.813789 (...) 23.23 (...) 4.10 10.93 (...) (...) (...)
OFG7 53.183697 ( † ) −27.836500 ( † ) (...) 24.55 1.23 ± 0.12 4.58 10.34 12.86 ± 0.04 1070 ± 101 AGS25, A2GS17
OFG8 53.210736 −27.813706 27.64 24.93 (...) 4.14 9.92 (...) (...) (...)
OFG9 53.191204 −27.835791 27.61 24.82 (...) 3.99 9.59 (...) (...) (...)
OFG10 53.191348 −27.737554 27.54 24.25 (...) 5.04 10.37 (...) (...) (...)
OFG11 53.196569 ( † ) −27.757065 ( † ) 27.44 23.59 0.62 ± 0.12 3.60 10.41 12.41 ± 0.09 384 ± 90 A2GS40, GDS48885
OFG12 53.154787 −27.806529 27.36 24.43 (...) 5.55 10.31 (...) (...) (...)
OFG13 53.047834 −27.829186 27.34 25.07 (...) 3.56 9.50 (...) (...) (...)
OFG14 53.105489 −27.830711 27.34 24.38 (...) 3.39 9.86 (...) (...) (...)
OFG15 53.132675 −27.765496 27.08 24.23 (...) 3.192sp 9.96 (...) (...) (...)
OFG16 53.080379 −27.869420 26.93 23.58 (...) 3.69 10.38 (...) (...) (...)
OFG17 53.062276 −27.875036 26.84 23.93 (...) 4.23 10.29 (...) (...) (...)
OFG18 53.188278 ( † ) −27.801928 ( † ) 26.82 24.88 0.37 ± 0.11 3.81 9.44 12.28 ± 0.11 286 ± 86 A2GS47
OFG19 53.162978 ( † ) −27.841940 ( † ) 26.76 24.14 0.40 ± 0.12 4.09 10.30 12.26 ± 0.09 271 ± 59 A2GS82
OFG20 53.064807 ( † ) −27.862613 ( † ) 26.64 22.85 0.54 ± 0.10 4.74 10.88 12.79 ± 0.04 913 ± 86 A2GS57
OFG21 53.060144 −27.793838 26.59 24.68 (...) 5.89 9.75 (...) (...) (...)
OFG22 53.043745 −27.804347 26.51 24.56 (...) 4.56 9.97 (...) (...) (...)
OFG23 53.081890 −27.828815 26.45 23.83 (...) 3.88 10.25 (...) (...) (...)
OFG24 53.109771 −27.807466 26.40 25.07 (...) 6.27 9.87 (...) (...) (...)
OFG25 53.074868 ( † ) −27.875889 ( † ) 26.31 23.10 1.67 ± 0.10 3.47o 9.99 12.92 ± 0.03 1227 ± 74 AGS15, A2GS10
OFG26 53.207252 −27.791408 26.29 23.63 (...) 4.16 10.33 (...) (...) (...)
OFG27 ( * ) 53.079416 ( † ) −27.870820 ( † ) (...) 21.53 2.05 ± 0.12 3.467sp 11.11 13.08 ± 0.02 1795 ± 90 AGS17, A2GS7

OFG28 ( * *) 53.120402 ( † ) −27.742111 ( † ) (...) (...) 0.95 ± 0.12 (...) (...) (...) (...) A2GS33

Notes. (1) Source ID; (2)(3) Right ascension and declination (J2000) of sources. Coordinates detected in the ALMA 1.13 mm image are marked with a “( † )” exponent; (4)(5) H-band and IRAC 4.5 μm AB magnitudes. These magnitudes are given for the best-fitting Sérsic profile during de-blending procedure (see Sect. 3.3); (6) ALMA 1.13 mm flux density: obtained from the GOODS-ALMA 2.0 catalog (Gómez-Guijarro et al. 2022a); (7) Photometric redshifts: determined with the EAzY code (see Sect. 4.1; spectroscopic redshifts expressed in three decimal places and flagged with a “sp” exponent). The spectroscopic redshifts of OFG15 and OFG27 are from Herenz et al. (2017) and Zhou et al. (2020), respectively. OFG1, 2, 25, 27 were discovered in an overdensity region with the redshift peak to be 3.47 (flagged with a “o” exponent; Zhou et al. 2020); (8) Stellar masses: determined with the FAST++ (see Sect. 4.1); (9) Infrared luminosities: derived from CIGALE for three sources (OFG2, OFG20, and OFG27) with a Herschel counterpart or from the IR template library (Schreiber et al. 2018c) for the galaxies without a Herschel counterpart (see Sect. 4.2); (10) SFR = SFRIR + SFRUV (see Sect. 4.3); (11) Source IDs in other work: AGS (GOODS-ALMA 1.0 catalog; Franco et al. 2018, 2020a); A2GS (GOODS-ALMA 2.0 catalog; Gómez-Guijarro et al. 2022a); GDS (H-dropouts catalog; Wang et al. 2019). ( * )The missing galaxy in our selection approach is due to incompleteness of the search radius of 0.6″. We add it to our catalog to correct this incompleteness. ( * *)OFG28 is a candidate IRAC 4.5 μm dropout, which is only detected in longer wavelength images, e.g., 850 μm from the JCMT/SCUBA-2 and 870 μm from the ALMA (ID68 in Cowie et al. 2018), 1.13 mm from the GOODS-ALMA 2.0 100% pure source catalog (A2GS33 in Gómez-Guijarro et al. 2022a), and 1.2 mm from the ALMA (ID20 in Yamaguchi et al. 2019). We add it here to refine our OFG catalog in the GOODS-ALMA field. We note that OFG28 is not used in our analysis. We also note that OFG9, OFG13, OFG18, OFG22, and OFG24 are identified as LBGs (see Sect. 3.5.1). In this catalog, eight sources (OFG1-OFG7, and OFG27) are H-dropouts, which are not detected in the H-band (< 3σ).

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