Table 2.
Main source catalog.
| ID | RA | Dec | S/Np | S/Nd | Speak | Sfit | Saper | Counterpart | eyes ID | Cat |
|---|---|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | (mJy) | (mJy) | (mJy) | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| ASW2DF.01 | 11:40:57.80 | −26:29:35.5 | 25.27 | 23.56 | 1.17 ± 0.05 | 1.51 ± 0.05 | 1.81 ± 0.13 | SMG,CO | Robust | A |
| ASW2DF.02 | 11:41:00.32 | −26:30:31.9 | 20.31 | 19.02 | 1.04 ± 0.05 | 2.02 ± 0.09 | 2.20 ± 0.11 | SMG,CO | Robust | A |
| ASW2DF.03 | 11:40:59.60 | −26:30:39.2 | 20.28 | 19.19 | 0.97 ± 0.05 | 1.78 ± 0.07 | 1.82 ± 0.14 | SMG,COext | Robust | A |
| ASW2DF.04 | 11:40:53.21 | −26:29:11.1 | 19.69 | 17.93 | 0.92 ± 0.05 | 1.18 ± 0.06 | 1.36 ± 0.12 | SMG | Robust | A |
| ASW2DF.05 | 11:40:46.06 | −26:29:11.3 | 18.87 | 17.60 | 0.76 ± 0.04 | 1.27 ± 0.08 | 1.40 ± 0.11 | HAE,COext | Robust | A |
| ASW2DF.06 | 11:40:35.36 | −26:28:35.1 | 15.28 | 14.27 | 0.68 ± 0.04 | 0.88 ± 0.07 | 0.93 ± 0.11 | − | Robust | A |
| ASW2DF.07 | 11:40:44.06 | −26:28:21.1 | 13.61 | 12.21 | 0.56 ± 0.04 | 0.84 ± 0.07 | 0.79 ± 0.10 | − | Robust | A |
| ASW2DF.08 | 11:40:57.42 | −26:30:48.0 | 11.78 | 10.93 | 0.66 ± 0.06 | 0.72 ± 0.08 | 1.16 ± 0.14 | − | Possible | B |
| ASW2DF.09 | 11:40:58.48 | −26:30:36.7 | 11.31 | 9.93 | 0.53 ± 0.05 | 0.56 ± 0.05 | 0.71 ± 0.10 | − | Possible | B |
| ASW2DF.10 | 11:40:53.64 | −26:27:57.0 | 10.32 | 9.52 | 0.54 ± 0.05 | 0.67 ± 0.06 | 0.82 ± 0.14 | SMG | Robust | A |
| ASW2DF.11 | 11:40:39.02 | −26:30:35.4 | 10.20 | 9.03 | 0.50 ± 0.05 | 0.59 ± 0.07 | 0.57 ± 0.12 | − | Robust | A |
| ASW2DF.12 | 11:40:46.66 | −26:29:10.2 | 10.03 | 8.96 | 0.42 ± 0.04 | 0.57 ± 0.06 | 0.63 ± 0.11 | HAE,COext | Robust | A |
| ASW2DF.13 | 11:40:59.38 | −26:30:43.5 | 9.99 | 9.51 | 0.51 ± 0.05 | 0.67 ± 0.07 | 0.81 ± 0.15 | − | Possible | B |
| ASW2DF.14 | 11:40:40.86 | −26:29:46.8 | 9.93 | 9.31 | 0.48 ± 0.05 | 0.81 ± 0.07 | 0.67 ± 0.10 | COext | Robust | A |
| ASW2DF.15 | 11:40:43.94 | −26:28:34.2 | 9.39 | 8.63 | 0.38 ± 0.04 | 0.57 ± 0.06 | 0.66 ± 0.11 | − | Robust | A |
| ASW2DF.16 | 11:40:37.32 | −26:30:17.3 | 8.36 | 7.76 | 0.38 ± 0.05 | 0.75 ± 0.08 | 0.76 ± 0.12 | HAE,CO | Robust | A |
| ASW2DF.17 | 11:40:48.34 | −26:29:08.5 | 8.22 | 7.84 | 0.47 ± 0.06 | 1.00 ± 0.10 | 1.46 ± 0.19 | SMG,COext | Robust | A |
| ASW2DF.18 | 11:40:35.14 | −26:29:35.2 | 7.07 | 6.67 | 0.32 ± 0.04 | 0.34 ± 0.06 | 0.36 ± 0.12 | − | Possible | B |
| ASW2DF.19 | 11:40:53.70 | −26:29:11.8 | 6.90 | 6.56 | 0.32 ± 0.05 | 0.60 ± 0.07 | 0.79 ± 0.11 | − | Possible | B |
| ASW2DF.20 | 11:40:51.27 | −26:29:38.6 | 6.57 | 6.05 | 0.40 ± 0.06 | 0.75 ± 0.11 | 0.91 ± 0.18 | HAE,CO | Robust | A |
| ASW2DF.21 | 11:40:56.52 | −26:29:44.8 | 6.56 | 5.92 | 0.33 ± 0.05 | 0.29 ± 0.06 | 0.38 ± 0.13 | − | Possible | B |
| ASW2DF.22 | 11:40:43.54 | −26:29:02.5 | 6.17 | 5.59 | 0.26 ± 0.04 | 0.29 ± 0.05 | 0.49 ± 0.11 | − | Possible | B |
| ASW2DF.23 | 11:40:54.56 | −26:28:23.8 | 5.67 | 5.03 | 0.26 ± 0.05 | 0.47 ± 0.09 | 0.52 ± 0.11 | HAE, CO | Possible | B |
| ASW2DF.24 | 11:40:53.10 | −26:28:47.2 | 5.59 | 5.28 | 0.26 ± 0.05 | 0.36 ± 0.06 | 0.28 ± 0.14 | − | Possible | B |
| ASW2DF.25 | 11:40:52.45 | −26:29:39.8 | 5.35 | 4.78 | 0.25 ± 0.05 | 0.19 ± 0.05 | 0.18 ± 0.12 | − | Possible | B |
| ASW2DF.26 | 11:40:39.73 | −26:30:27.8 | 5.25 | 4.57 | 0.25 ± 0.05 | 0.32 ± 0.07 | 0.32 ± 0.14 | − | Possible | B |
| ASW2DF.27 | 11:40:46.31 | −26:29:32.8 | 5.19 | 4.22 | 0.21 ± 0.04 | 0.15 ± 0.04 | 0.17 ± 0.11 | − | Possible | B |
| ASW2DF.28 | 11:40:54.74 | −26:28:03.1 | 5.06 | 4.82 | 0.24 ± 0.05 | 0.40 ± 0.08 | 0.56 ± 0.12 | HAE | Possible | B |
| ASW2DF.29 | 11:40:38.58 | −26:30:25.5 | 5.05 | 4.55 | 0.38 ± 0.08 | 0.30 ± 0.08 | 0.43 ± 0.19 | CO | Marginal | B |
| ASW2DF.30 | 11:40:49.14 | −26:30:37.8 | 4.91 | 4.47 | 0.29 ± 0.06 | 0.23 ± 0.06 | 0.16 ± 0.17 | − | Possible | B |
| ASW2DF.31 | 11:40:48.76 | −26:27:52.8 | 4.90 | 4.44 | 0.36 ± 0.07 | 0.65 ± 0.15 | 0.60 ± 0.19 | SMG | Possible | B |
| ASW2DF.32 | 11:40:57.52 | −26:27:59.1 | 4.88 | 4.32 | 0.24 ± 0.05 | 0.18 ± 0.05 | 0.13 ± 0.14 | − | − | B |
| ASW2DF.33 | 11:40:57.81 | −26:30:47.8 | 4.83 | 4.66 | 0.28 ± 0.06 | 0.67 ± 0.11 | 1.14 ± 0.15 | SMG, COext | Cloud-like | B |
| ASW2DF.34 | 11:40:50.82 | −26:30:07.2 | 4.82 | 4.08 | 0.28 ± 0.06 | 0.23 ± 0.05 | 0.26 ± 0.17 | − | − | B |
| ASW2DF.35 | 11:40:42.43 | −26:28:04.3 | 4.81 | 4.14 | 0.26 ± 0.05 | 0.32 ± 0.08 | 0.50 ± 0.13 | − | Cloud-like | B |
| ASW2DF.36 | 11:40:57.57 | −26:30:24.3 | 4.74 | 4.21 | 0.22 ± 0.05 | 0.15 ± 0.04 | 0.05 ± 0.09 | − | − | B |
| ASW2DF.37 | 11:40:52.84 | −26:29:11.0 | 4.72 | 4.36 | 0.22 ± 0.05 | 0.35 ± 0.08 | 0.46 ± 0.11 | − | Possible | B |
| ASW2DF.38 | 11:40:58.88 | −26:29:58.7 | 4.72 | 4.33 | 0.22 ± 0.05 | 0.16 ± 0.05 | 0.25 ± 0.09 | − | − | B |
| ASW2DF.39 | 11:40:56.21 | −26:29:32.9 | 4.67 | 4.01 | 0.26 ± 0.06 | 0.24 ± 0.06 | 0.12 ± 0.16 | − | Possible | B |
| ASW2DF.40 | 11:41:00.77 | −26:30:42.9 | 4.60 | 4.21 | 0.31 ± 0.07 | 0.35 ± 0.08 | 0.56 ± 0.15 | − | Possible | B |
| ASW2DF.41 | 11:40:35.98 | −26:29:02.3 | 4.58 | 4.18 | 0.21 ± 0.04 | 0.53 ± 0.10 | 0.65 ± 0.12 | − | Cloud-like | B |
| ASW2DF.42 | 11:40:40.18 | −26:28:39.5 | 4.57 | 4.24 | 0.22 ± 0.05 | 0.21 ± 0.06 | 0.06 ± 0.14 | − | Robust | A |
| ASW2DF.43 | 11:40:55.81 | −26:30:24.7 | 4.54 | 4.12 | 0.34 ± 0.07 | 0.26 ± 0.08 | 0.17 ± 0.18 | − | Marginal | B |
| ASW2DF.44 | 11:40:48.99 | −26:30:17.1 | 4.51 | 4.14 | 0.26 ± 0.06 | 0.56 ± 0.12 | 0.90 ± 0.15 | − | Cloud-like | B |
| ASW2DF.45 | 11:40:53.96 | −26:29:00.9 | 4.43 | 4.15 | 0.21 ± 0.05 | 0.27 ± 0.06 | 0.35 ± 0.13 | − | − | B |
| ASW2DF.46 | 11:40:50.71 | −26:28:31.4 | 4.35 | 4.08 | 0.25 ± 0.06 | 0.26 ± 0.08 | 0.32 ± 0.20 | − | − | B |
| ASW2DF.47 | 11:40:51.11 | −26:29:05.1 | 4.24 | 4.05 | 0.25 ± 0.06 | 0.48 ± 0.10 | 0.61 ± 0.15 | COext | Possible | B |
Notes. (1) ALMA sources with IDs sorted by the peak S/N; (2) Right ascension (J2000); (3) Declination (J2000); (4) S/N at the peak pixel; (5) S/N at the fifth brightest pixel of a source, which can be detected by the “fixed” method at 4σ; (6) Peak flux at 1.2 mm; (7) Gaussian fitting flux; (8) Twice the value of the synthesized beam aperture flux; (9) Counterparts of ALMA sources matched from different galaxy populations, including SMGs (Dannerbauer et al. 2014), HAEs (Koyama et al. 2013; Shimakawa et al. 2018b), and CO emitters (Jin et al. 2021; Chen et al. 2024) – the CO emitters identified as extended gas reservoirs by Chen et al. (2024) are marked with a subscript “ext”; (10) The classifications of the sources identified by visual inspection, including “robust”, “possible”, “could-like” and “edge”; (11) Source category.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.