Table A.1.
Spectroscopic fluxes for the sample of EELG candidates with NIRSpec spectra ordered by increasing CEERS ID number.
| ID | MPT ID | zspec | F([OII])prism | F([OII])MR | F(Hβ)prism | F(Hβ)MR | F([OIII]λ5007)prism | F([OIII]λ5007)MR | F(Hα)prism | F(Hα)MR |
|---|---|---|---|---|---|---|---|---|---|---|
| 10−18cgs | 10−18cgs | 10−18cgs | 10−18cgs | 10−18cgs | 10−18cgs | 10−18cgs | 10−18cgs | |||
| 1253 | 44 | 7.10 | – | – | < 0.4 | – | 3.2(0.2) | – | – | – |
| 2149 | 3584 | 4.64 | 1.9(0.4) | – | 3.2(0.2) | – | 23.4(0.4) | – | 11.8(0.3) | – |
| 2166 | 1912 | 5.10 | 2.9(0.5) | – | 0.8(0.2) | – | 5.6(0.2) | – | 3.8(0.3) | – |
| 4176 | 1953 | 4.61 | – | – | 0.9(0.2) | – | 5.0(0.2) | – | 2.6(0.1) | – |
| 5040 | 3585 | 3.87 | – | 2.5(0.4) | < 1.7 | 2.0(0.2) | 1.1(0.3) | 20.9(0.5) | 0.6(0.2) | 10.5(0.3) |
| 8674 | 2355 | 6.12 | 0.8(0.2) | – | < 0.4 | – | 1.2(0.1) | – | 1.2(0.2) | – |
| 9290 | 3587 | 3.92 | – | – | 0.6(0.2) | – | 6.6(0.1) | – | 2.8(0.1) | – |
| 16056 | 2000 | 4.81 | 3.6(0.4) | – | 3.0(0.2) | – | 21.0(0.3) | – | 10.7(0.3) | – |
| 19984 | 323 | 5.67 | – | – | 1.6(0.2) | 2.2(0.3) | 8.2(0.2) | 7.5(2.3) | 5.4(0.2) | 6.1(0.2) |
| 21394 | 355 | 6.10 | 1.1(0.2) | < 4.3 | 1.3(0.1) | 1.1(0.3) | 7.9(0.2) | 7.7(0.2) | – | 3.5(0.2) |
| 25074 | 397 | 6.00 | 3.9(0.3) | 3.6(0.3) | 5.3(0.2) | 5.9(1.6) | 38.4(0.3) | 40.0(1.3) | 18.5(0.4) | 18.9(0.5) |
| 26436 | 428 | 6.10 | – | 0.7(0.2) | – | – | – | – | – | 2.9(0.3) |
| 27280 | 439 | 7.18 | – | – | 0.8(0.1) | – | 4.5(0.2) | – | – | – |
| 31338 | 498 | 7.18 | < 0.6 | – | 0.7(0.2) | – | 4.2(0.2) | – | – | – |
| 31339 | 499 | 7.17 | – | – | – | < 0.2 | – | 1.4(0.1) | – | – |
| 35306 | 82043 | 4.32 | – | – | 1.6(0.3) | – | 9.2(0.3) | – | 4.9(0.2) | – |
| 35645 | 82052 | 5.15 | – | – | 0.4(0.1) | – | 2.7(0.1) | – | 1.6(0.1) | – |
| 45809 | 80239 | 7.49 | – | – | 0.4(0.1) | – | 1.7(0.1) | – | – | – |
| 46186 | 82300 | 4.72 | – | – | < 0.5 | – | 1.6(0.2) | – | 0.8(0.1) | – |
| 46552 | 80244 | 7.01 | – | – | 0.3(0.1) | – | 1.1(0.1) | – | < 29506.8 | – |
| 48859 | 80671 | 5.74 | – | – | – | – | – | – | – | – |
| 53583 | 535 | 7.12 | – | – | 0.8(0.1) | – | 4.1(0.2) | – | – | – |
| 59817 | 792 | 6.26 | – | 2.5(0.3) | – | 0.8(0.2) | – | 6.5(0.3) | – | 2.3(0.3) |
| 59920 | 1027 | 7.82 | < 0.8 | < 0.7 | 1.6(0.2) | 1.2(0.2) | 9.8(0.3) | 9.5(0.5) | – | – |
| 61253 | 80710 | 6.55 | – | – | < 0.2 | – | 0.9(0.1) | – | 0.8(0.1) | – |
| 61419 | 24 | 9.00 | – | – | – | – | – | 2.2(0.3) | – | – |
| 70867 | 1236 | 4.48 | 1.2(0.4) | < 0.7 | – | < 5.9 | – | 2.3(0.2) | – | 1.3(0.2) |
| 78973 | 1305 | 4.28 | – | – | – | 0.5(0.1) | – | 2.5(0.2) | – | 1.3(0.1) |
| 79680 | 1038 | 7.19 | – | < 1.2 | – | 0.6(0.1) | – | 2.6(0.2) | – | – |
| 81061 | 1019 | 8.68 | – | 1.6(0.1) | – | 1.4(0.5) | – | 19.0(0.8) | – | – |
| 86030 | 80374 | 7.18 | – | – | 0.6(0.1) | – | 1.6(0.2) | – | – | – |
| 86830 | 80916 | 5.68 | < 0.8 | – | 1.1(0.1) | – | 7.5(0.2) | – | 4.4(0.2) | – |
| 87370 | 1374 | 5.00 | 4.4(0.4) | 11.6(0.5) | 2.7(0.2) | 9.8(0.5) | 20.9(0.3) | 65.8(0.9) | 9.9(0.2) | 31.4(3.5) |
| 90671 | 80083 | 8.64 | – | – | < 0.6 | – | 2.3(0.1) | – | – | – |
| 97883 | 83779 | 4.31 | < 0.9 | – | 0.9(0.2) | – | 8.9(0.2) | – | 4.8(0.2) | – |
| 98160 | 80432 | 7.48 | < 0.5 | – | 1.1(0.1) | – | 6.2(0.2) | – | – | – |
| 100152 | 81063 | 6.09 | – | – | 0.7(0.1) | – | 7.4(0.2) | – | 3.2(0.2) | – |
| 100312 | 83856 | 4.56 | – | – | 1.5(0.1) | – | 4.3(0.1) | – | 4.8(0.2) | – |
| 100621 | 81068 | 6.27 | – | – | 0.7(0.1) | – | 4.4(0.2) | – | 2.1(0.1) | – |
Notes. We include the MPT ID which is the identification code of the galaxies in the spectroscopic catalog in CEERS. We report fluxes from prism and medium-resolution grating. Fluxes are in cgs units of erg cm−2 s−1. In parenthesis, the uncertainties are reported.
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