Table F.3
List of targets with one or more emission lines detected at S/N > 5 in the Prism/Clear data – truncated table, full version on https://arxiv.org/abs/2306.02467 and at the CDS.
| ID | zPRISM | List of detected emission lines and flux in units of 10−19 erg s−1 cm−2 |
|---|---|---|
| 6438 | 9.689 | Hγ (1.5 ± 0.2); Hβ (2.0 ± 0.2) |
| 10058975 | 9.438 | CIV λλ1549 (4.6 ± 0.8); HeII + OIII] (7.3 ± 1.0); CIII] λλ1909 (4.6 ± 0.3); [NeIII] λ3869 (2.6 ± 0.3); Hδ (2.1 ± 0.0); Hγ (3.7 ± 0.1); [OIII] λ4363 (1.5 ± 0.1); Hβ (6.7 ± 0.2); [OIII] λ4959 (10.7 ± 0.2); [OIII] λ5007 (29.4 ± 0.3) |
| 8013 | 8.479 | Hβ (1.8 ± 0.2); [OIII] λ4959 (3.2 ± 0.2); [OIII] λ5007 (9.1 ± 0.3) |
| 21842 | 7.981 | [OII] λλ3727 (1.9 ± 0.2); [NeIII] λ3869 (2.0 ± 0.2); Hδ (1.5 ± 0.2); Hγ (1.9 ± 0.1); [OIII] λ4363 (0.6 ± 0.1); Hβ (2.8 ± 0.2); [OIII] λ4959 (5.9 ± 0.2); [OIII] λ5007 (17.7 ± 0.2) |
| 10013682 | 7.277 | Hβ (1.0 ± 0.2); [OIII] λ4959 (2.4 ± 0.2); [OIII] λ5007 (6.0 ± 0.2) |
| 8079 | 7.260 | [OIII] λ5007 (1.7 ± 0.2) |
| 10013905 | 7.206 | [OII] λλ3727 (1.3 ± 0.2); Hγ + [OIII] λ4363 (2.7 ± 0.4); Hβ (4.0 ± 0.2); [OIII] λ4959 (6.6 ± 0.2); [OIII] λ5007 (19.5 ± 0.3) |
| 20961 | 7.051 | Hβ (2.5 ± 0.2); [OIII] λ4959 (3.1 ± 0.2); [OIII] λ5007 (9.6 ± 0.3) |
| 10013609 | 6.931 | [OII] λλ3727 (3.3 ± 0.4); [NeIII] λ3869 (4.4 ± 0.7); Hγ + [OIII] λ4363 (3.8 ± 0.4); Hβ (5.2 ± 0.4); [OIII] λ4959 (11.1 ± 0.4); [OIII] λ5007 (32.7 ± 0.5); Hα (16.7 ± 0.5) |
| 4297 | 6.718 | Hβ (3.9 ± 0.3); [OIII] λ4959 (8.7 ± 0.3); [OIII] λ5007 (24.0 ± 0.4); Hα (10.8 ± 0.4) |
| 3334 | 6.709 | Hβ (1.2 ± 0.2); [OIII] λ4959 (4.0 ± 0.2); [OIII] λ5007 (11.5 ± 0.2); Hα (5.0 ± 0.2) |
| 16625 | 6.631 | [NeIII] λ3869 (2.3 ± 0.3); Hδ (1.7 ± 0.2); Hγ + [OIII] λ4363 (3.4 ± 0.3); Hβ (5.1 ± 0.2); [OIII] λ4959 (6.5 ± 0.2); [OIII] λ5007 (19.1 ± 0.3); Hα (16.5 ± 0.2) |
| 10005447 | 6.627 | [OIII] λ4959 (2.0 ± 0.3); [OIII] λ5007 (4.4 ± 0.4); Hα (3.5 ± 0.3) |
| 18846 | 6.342 | CIV λλ1549 (8.8 ± 1.3); HeII + OIII] (10.3 ± 1.7); CIII] λλ1909 (7.1 ± 1.3); [NeIII] λ3869 (3.9 ± 0.3); Hδ (4.8 ± 0.5); Hγ + [OIII] λ4363 (5.4 ± 0.7); Hβ (11.0 ± 0.3); [OIII] λ4959 (16.5 ± 0.3); [OIII] λ5007 (51.6 ± 0.4); HeI λ5875 (1.3 ± 0.2); Hα (29.8 ± 0.4) |
| 18179 | 6.335 | [OII] λλ3727 (4.7 ± 0.6); Hβ (3.0 ± 0.3); [OIII] λ4959 (7.3 ± 0.4); [OIII] λ5007 (21.7 ± 0.5); Hα (11.8 ± 0.5) |
| 18976 | 6.329 | Hγ + [OIII] λ4363 (2.4 ± 0.7); Hβ (3.2 ± 0.2); [OIII] λ4959 (4.7 ± 0.2); [OIII] λ5007 (13.8 ± 0.3); Hα (9.3 ± 0.3) |
| 10009693 | 6.296 | [OIII] λ5007 (5.3 ± 0.3); Hα (3.0 ± 0.4) |
| 17566 | 6.105 | [OII] λλ3727 (9.5 ± 0.6); Hβ (3.7 ± 0.4); [OIII] λ4959 (7.7 ± 0.3); [OIII] λ5007 (25.0 ± 0.4); Hα (16.8 ± 0.3) |
| 19342 | 5.981 | Hγ + [OIII] λ4363 (2.0 ± 0.8); Hβ (4.4 ± 0.3); [OIII] λ4959 (6.9 ± 0.2); [OIII] λ5007 (18.9 ± 0.3); Hα (10.9 ± 0.3) |
| 10013618 | 5.948 | [OII] λλ3727 (4.6 ± 0.5); Hβ (1.7 ± 0.2); [OIII] λ4959 (4.0 ± 0.2); [OIII] λ5007 (11.5 ± 0.3); HeI λ5875 (0.5 ± 0.1); Hα (6.9 ± 0.2) |
| 9422 | 5.943 | CIV λλ1549 (38.7 ± 3.0); HeII + OIII] (11.6 ± 0.8); [OII] λλ3727 (3.6 ± 0.4); [NeIII] λ3869 (8.2 ± 1.0); [NeIII] λ3967 (3.4 ± 0.5); Hδ (3.3 ± 0.5); Hγ + [OIII] λ4363 (11.7 ± 0.5); Hβ (18.5 ± 0.4); [OIII] λ4959 (35.2 ± 0.5); [OIII] λ5007 (104.4 ± 0.8); HeI λ5875 (2.6 ± 0.1); Hα (50.8 ± 0.6); HeI λ7065 (2.0 ± 0.2) |
| 6002 | 5.941 | [NeIII] λ3869 (2.8 ± 0.4); Hγ + [OIII] λ4363 (1.8 ± 0.6); Hβ (2.6 ± 0.1); [OIII] λ4959 (5.2 ± 0.1); [OIII] λ5007 (15.4 ± 0.2); Hα (8.2 ± 0.2) |
| 10013704 | 5.931 | [OII] λλ3727 (1.7 ± 0.3); [NeIII] λ3869 (3.6 ± 0.4); Hγ + [OIII] λ4363 (5.8 ± 0.4); Hβ (8.3 ± 0.4); [OIII] λ4959 (15.3 ± 0.4); [OIII] λ5007 (45.0 ± 0.5); HeI λ5875 (1.3 ± 0.1); Hα (49.2 ± 0.6) |
| 10013620 | 5.920 | [OII] λλ3727 (6.4 ± 0.6); [NeIII] λ3869 (2.4 ± 0.4); Hγ + [OIII] λ4363 (2.6 ± 0.3); Hβ (4.4 ± 0.3); [OIII] λ4959 (8.2 ± 0.3); [OIII] λ5007 (23.8 ± 0.4); Hα (11.9 ± 0.3) |
| 19606 | 5.891 | [NeIII] λ3869 (2.7 ± 0.5); Hγ + [OIII] λ4363 (2.6 ± 0.4); (4.3 ± 0.4); [OIII] λ4959 (9.2 ± 0.4); [OIII] λ5007 (24.6 ± 0.5); Hα (13.2 ± 0.4) |
| 10056849 | 5.822 | Hγ + [OIII] λ4363 (1.9 ± 0.2); Hβ (4.7 ± 0.2); [OIII] λ4959 (5.0 ± 0.2); [OIII] λ5007 (14.5 ± 0.2); Hα (10.8 ± 0.2) |
| 10005113 | 5.820 | Hγ + [OIII] λ4363 (2.1 ± 0.3); Hβ (3.6 ± 0.2); [OIII] λ4959 (4.1 ± 0.2); [OIII] λ5007 (12.2 ± 0.3); Hα (9.1 ± 0.3) |
| 22251 | 5.804 | [OII] λλ3727 (5.4 ± 0.3); [NeIII] λ3869 (5.8 ± 0.3); [NeIII] λ3967 (3.0 ± 0.4); Hγ + [OIII] λ4363 (5.6 ± 0.4); Hβ (8.8 ± 0.3); [OIII] λ4959 (21.5 ± 0.4); [OIII] λ5007 (61.0 ± 0.5); HeI λ5875 (1.3 ± 0.2); Hα (30.3 ± 0.4) |
| 4404 | 5.775 | [OII] λλ3727 (4.9 ± 0.6); [NeIII] λ3869 (3.9 ± 0.6); Hγ + [OIII] λ4363 (5.5 ± 0.3); Hβ (9.8 ± 0.4); [OIII] λ4959 (16.3 ± 0.4); [OIII] λ5007 (43.4 ± 0.5); Hα (23.7 ± 0.3) |
| 3968 | 5.769 | [OIII] λ4959 (2.9 ± 0.3); [OIII] λ5007 (6.6 ± 0.4); Hα (3.3 ± 0.2) |
Notes. Details of the emission line fitting can be found in Section 5.1. Note that some lines (notably, Hβ, [O III] λ4959 and [O III] λ5007) are reported independently at high-redshift, but are reported as blends at lower redshift due to the reduced spectral resolution of the prism at shorter wavelengths. We also caution that some fluxes reported here as being for individual lines may feature non-negligible contributions from fainter lines (e.g. Hα from [N II] λ6583, or [Ne III] λ3869 from He I λ3889). In these cases, the reported flux will represent the total flux of the observed emission feature. Targets marked (‡) were identified as likely having multiple objects in the shutter (see Section 5.3). These measurements are available in a machine-readable format on The Mikulski Archive for Space Telescopes: https://archive.stsci.edu/hlsp/jades as GOODS-S-DeepHSTv1.0.
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