Table 1.
Line and continuum detections of LH-SBC3 members.
| ID | RA | Dec | zspec | δv( † ) | CO(4–3) |
[CI](1–0) |
3 mm |
|||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| I | S/N | P( ‡ ) |
 |
FWZI( * *) | I | S/N | S | |||||
| (deg) | (deg) | (km s−1) | (mJy km s−1) | (km s−1) | (mJy km s−1) | (μJy) | ||||||
| a | 160.4684 | 58.7558 | 3.949 | −54 | 1567 ± 57 | 27.5 | 0.000 | 0.000 | 825 | 205 ± 68 | 3.0 | 73 ± 11 |
| b | 160.4764 | 58.7584 | 3.954 | −348 | 528 ± 45 | 11.6 | 0.000 | 0.000 | 671 | 136 ± 54 | 2.5 | 114 ± 10 |
| c | 160.4648 | 58.7554 | 3.940 | 543 | 180 ± 38 | 4.8 | 0.024 | 0.001 | 566 | < 108 | < 2 | 23 ± 10 |
| d | 160.4702 | 58.7561 | 3.951 | −141 | 226 ± 52 | 4.6 | 0.034 | 0.002 | 824 | 190 ± 65 | 2.9 | 43 ± 10 |
Notes. ( † ): velocity relative to the cluster center by assuming the average redshift zav = 3.949; ( ‡ ): chance of spurious probability calculated over the entire spectrum based on Jin et al. (2019); ( * ): chance of spurious probability calculated over ±2000 km s−1 of the CO(4–3) line at zav = 3.949; ( * *): full width at zero intensity of the lines.
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