Table 3
HST grism spectroscopic data for C III] emitters in the udf-10 .
MUSE ID | HUDF ID | z | [O III] EW | [O II] EW | HβEW | HαEW | 12+log(O/H) | 12+log(O/H) |
(Å) | (Å) | (Å) | (Å) | (R23, lower) | (R23, upper) | |||
|
||||||||
UDF10-22 | 2925 | 2.226 | 458 ± 9.52 | 88.4 ± 5.68 | 74.1 ± 4.10 | ... | 8.21 ± 0.052 | 8.44 ± 0.032 |
UDF10-41 | 2900 | 1.847 | 973 ± 38.2 | 86.0 ± 111 | 73.6 ± 10.3 | ... | 8.27 ± 0.223 | 8.42 ± 0.160 |
UDF10-42 | 2455 | 1.550 | 444 ± 20.9 | ... | 62.1 ± 10.8 | 264 ± 23.6 | ... | ... |
UDF10-51 | 2034 | 2.228 | 464 ± 44.4 | <279 | 145 ± 25.6 | ... | 7.42 ± 0.153 | 8.82 ± 0.051 |
UDF10-64 | 3058 | 1.847 | 299 ± 32.3 | 444 ± 413 | 24.9 ± 20.9 | ... | ... | ... |
UDF10-99 | 1622 | 2.543 | ... | 120 ± 48.6 | ... | ... | ... | ... |
UDF10-164 | 1698 | 1.906 | 1170 ± 292 | <3300 | 171 ± 74.3 | ... | 8.41 ± 0.398 | 8.31 ± 0.280 |
UDF10-231 | 2960 | 2.447 | ... | <641 | ... | ... | ... | ... |
UDF10-6664 | 1727 | 2.394 | 473 ± 119 | 88.8 ± 14.2 | 65.2 ± 20.4 | ... | 8.44 ± 0.325 | 8.28 ± 0.227 |
UDF10-6668 | 2090 | 1.850 | 937 ± 87.6 | <113 | 180 ± 30.9 | ... | ... | ... |
UDF10-6670 | 2018 | 2.069 | 535 ± 66.7 | 46.1 ± 34.1 | 39.9 ± 27.6 | ... | 8.87 ± 0.857 | 8.09 ± 0.544 |
UDF10-6674 | 2720 | 2.542 | ... | <209 | ... | ... | ... | ... |
Notes. Grism spectroscopic data for the C III] emitters in the UDF10. HUDF IDs come from the van Dokkum et al. (2013) catalog. “[O II]” refers to the combined [O II] λλ3727, 3729 doublet and “[O III]” refers to the combined [O III] λλ4959, 5007 doublet. The redshift coverage of C III] in MUSE and [O III] in the G141 grism is 1.4 ≲ z ≲ 2.4. All EWs are quoted in the rest frame. Upper limits for [O II] are based on the broadband JF125W continuum level and the brighter of the 3σ flux measurement from the spectrum or the flux limit of the stacked grism spectra (3σ ~ 3.9 × 10-18 erg s-1 cm-2; Brammer et al. 2013). Values of 12 + log (O / H) (gas-phase metallicity) are estimated using the R23 ratio [([O II] + [O III])/Hβ] and the calibration of Kobulnicky et al. (1999) for both the upper and lower branches of the R23 parameter.
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