Table F.2
List of targets with one or more emission lines detected with S /N > 5 in the R ≈ 1000 grating data, and derived redshifts – truncated table, full version on https://arxiv.org/abs/2306.02467 and at the CDS.
| ID | zR≈1000 | List of detected emission lines and flux in units of 10−19 erg s−1 cm−2 |
|---|---|---|
| 10058975 | 9.433 | [NeIII] λ3869 (3.1 ± 0.6); Hγ (3.0 ± 0.6); Hβ (8.0 ± 0.9); [OIII] λ4959 (11.5 ± 0.9); [OIII] λ5007 (35.8 ± 0.8) |
| 8013 | 8.473 | [OIII] λ5007 (12.9 ± 1.6) |
| 21842 | 7.980 | Hβ (3.1 ± 0.5); [OIII] λ4959 (8.7 ± 0.5); [OIII] λ5007 (17.9 ± 0.7) |
| 10013682 | 7.275 | Ly-α (23.8 ± 3.3); [OIII] λ5007 (7.2 ± 0.6) |
| 10013905 | 7.197 | Hβ (7.4 ± 0.9); [OIII] λ4959 (5.8 ± 0.9); [OIII] λ5007 (20.6 ± 0.8) |
| 20961 | 7.044 | Hβ (4.0 ± 0.8); [OIII] λ5007 (10.7 ± 0.8) |
| 10013609 | 6.929 | Hβ (6.7 ± 1.0); [OIII] λ4959 (11.8 ± 1.1); [OIII] λ5007 (35.4 ± 1.3); Hα (21.9 ± 1.5) |
| 4297 | 6.713 | Ly-α (30.9 ± 5.2); Hβ (5.2 ± 0.6); [OIII] λ4959 (9.4 ± 0.7); [OIII] λ5007 (29.0 ± 1.2); Hα (15.2 ± 1.3) |
| 3334 | 6.706 | [OIII] λ4959 (3.8 ± 0.5); [OIII] λ5007 (13.0 ± 0.6) |
| 16625 | 6.631 | Ly-α (21.1 ± 3.8); Hβ (7.1 ± 0.7); [OIII] λ4959 (6.1 ± 0.6); [OIII] λ5007 (20.9 ± 0.7); Hα (18.6 ± 1.0) |
| 10005447 | 6.623 | [OIII] λ5007 (5.4 ± 0.9) |
| 18846 | 6.335 | Ly-α (82.4 ± 4.6); Hγ (3.9 ± 0.8); Hβ (10.3 ± 0.6); [OIII] λ4959 (19.8 ± 0.7); [OIII] λ5007 (58.4 ± 1.1); Hα (36.0 ± 1.2) |
| 18976 | 6.327 | Hβ (4.0 ± 0.5); [OIII] λ4959 (5.4 ± 0.6); [OIII] λ5007 (14.3 ± 1.0); Hα (10.4 ± 1.1) |
| 10009693 | 6.286 | [OIII] λ5007 (5.9 ± 0.8) |
| 17566 | 6.102 | [OII] λλ3727 (10.0 ± 1.5); Hβ (5.7 ± 0.9); [OIII] λ4959 (9.9 ± 1.0); [OIII] λ5007 (32.2 ± 1.0); Hα (15.6 ± 1.3) |
| 19342 | 5.974 | Hβ (5.0 ± 0.7); [OIII] λ4959 (5.7 ± 0.6); [OIII] λ5007 (19.5 ± 0.8); Hα (13.8 ± 0.9) |
| 10013618 | 5.944 | [OII] λλ3727 (8.0 ± 0.9); Hβ (1.9 ± 0.4); [OIII] λ4959 (5.1 ± 0.6); [OIII] λ5007 (13.1 ± 0.5); Hα (7.5 ± 0.7) |
| 6002 | 5.937 | Ly-α (30.1 ± 4.2); Hβ (2.6 ± 0.4); [OIII] λ4959 (6.1 ± 0.6); [OIII] λ5007 (16.3 ± 0.5); Hα (10.2 ± 0.5) |
| 9422 | 5.936 | Ly-α (103.6 ± 6.0); CIV λλ1549 (34.0 ± 2.4); CIII] λλ1909 (7.4 ± 0.9); [NeIII] λ3869 (6.5 ± 0.3); Hγ (8.1 ± 0.7); Hβ (19.7 ± 0.5); [OIII] λ4959 (38.6 ± 0.9); [OIII] λ5007 (110.8 ± 1.2) |
| 10013704(a) | 5.920 | [NeIII] λ3869 (4.8 ± 0.7); Hγ (4.1 ± 0.6); Hβ (9.0 ± 0.7); [OIII] λ4959 (17.5 ± 0.6); [OIII] λ5007 (48.3 ± 0.9); Hα (63.5 ± 2.0) |
| 10013620 | 5.918 | Hβ (4.7 ± 0.8); [OIII] λ4959 (8.6 ± 0.8); [OIII] λ5007 (23.1 ± 0.9); Hα (13.8 ± 1.3) |
| 19606 | 5.889 | Hβ (6.1 ± 1.1); [OIII] λ4959 (8.9 ± 1.3); [OIII] λ5007 (28.0 ± 1.0); Hα (19.0 ± 1.6) |
| 10005113 | 5.821 | Hβ (2.1 ± 0.4); [OIII] λ4959 (4.4 ± 0.6); [OIII] λ5007 (14.2 ± 0.7) |
| 10056849 | 5.814 | Hβ (4.9 ± 0.9); [OIII] λ4959 (4.5 ± 0.9); [OIII] λ5007 (17.0 ± 1.0); Hα (14.1 ± 0.8) |
| 22251 | 5.798 | [OII] λλ3727 (9.0 ± 1.2); [NeIII] λ3869 (5.9 ± 1.0); Hβ (10.9 ± 0.8); [OIII] λ4959 (23.4 ± 0.7); [OIII] λ5007 (67.1 ± 1.2); Hα (33.8 ± 0.9) |
| 3968 | 5.768 | [OIII] λ5007 (7.9 ± 0.8) |
| 4404 | 5.764 | [OII] λλ3727 (5.5 ± 1.0); [NeIII] λ3869 (6.0 ± 1.0); Hβ (8.6 ± 1.2); [OIII] λ4959 (18.2 ± 1.2); [OIII] λ5007 (52.9 ± 1.3); Hα (30.1 ± 1.0) |
| 6384 | 5.615 | [OIII] λ5007 (7.8 ± 1.1) |
| 16745 | 5.567 | [OII] λλ3727 (14.3 ± 1.3); [NeIII] λ3869 (4.1 ± 0.8); Hβ (4.1 ± 0.6); Hα (20.8 ± 0.7) |
| 6246 | 5.562 | Hβ (3.4 ± 0.5); [OIII] λ4959 (3.5 ± 0.5); [OIII] λ5007 (11.6 ± 0.5); Hα (7.6 ± 0.5) |
| 10016374 | 5.504 | [OII] λλ3727 (5.4 ± 1.0); Hβ (7.2 ± 1.0); Hα (17.9 ± 0.8) |
| 9343 | 5.443 | Hβ (4.4 ± 0.7); [OIII] λ4959 (7.7 ± 1.0); [OIII] λ5007 (20.1 ± 1.2); Hα (10.6 ± 0.8) |
| 9743 | 5.440 | [OIII] λ4959 (11.3 ± 1.8); [OIII] λ5007 (24.6 ± 2.7); Hα (26.9 ± 2.0) |
| 9452 | 5.122 | [OIII] λ5007 (47.7 ± 3.8); Hα (18.8 ± 2.1) |
| 10015338 | 5.077 | Hγ (16.9 ± 3.1); [OIII] λ4959 (25.5 ± 2.7); [OIII] λ5007 (57.5 ± 2.6); Hα (31.7 ± 1.9) |
| 5759 | 5.052 | [OIII] λ4959 (9.9 ± 1.4); [OIII] λ5007 (19.9 ± 1.5); Hα (13.7 ± 1.2) |
Notes. Details of the emission line fitting can be found in Section 5.1. The last column gives a list of emission lines detected with S/N > 5, and the flux measured for that line. Targets marked (‡)were identified as likely having multiple objects in the shutter (see Section 5.3). Targets marked (a)showed a broad component under Hα and reported flux was obtained from direct integration rather than a single component fit (Section 5.1). These measurements are also available in a machine-readable format on The Mikulski Archive for Space Telescopes: https://archive.stsci.edu/hlsp/jades as GOODS-S-DeepHST v1.0.
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