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Table 4.

Approximate redshift ranges where various emission lines are affected by the detector gap for the different NIRSpec dispersers.

Line λ [μm] G140H G235H G395H
Lyα 0.12152 10.59–11.23 18.42–19.50 31.78–33.60
NV 0.12408 10.35–10.98 18.02–19.08 31.10–32.89
CIV 0.15495 8.09–8.59 14.23–15.08 24.71–26.14
HeII 0.16404 7.58–8.06 13.39–14.19 23.28–24.63
CIII] 0.19087 6.38–6.79 11.36–12.05 19.87–21.03
MgII 0.27991 4.03–4.31 7.43–7.90 13.23–14.02
[OII] 0.37271 2.78–2.99 5.33–5.68 9.69–10.28
[OII] 0.37299 2.77–2.98 5.33–5.68 9.68–10.27
Hβ 0.48627 1.90–2.06 3.85–4.12 7.19–7.65
[OIII] 0.49603 1.84–2.00 3.76–4.02 7.03–7.48
[OIII] 0.50082 1.81–1.97 3.71–3.97 6.95–7.40
[NII] 0.65499 1.15–1.27 2.60–2.80 5.08–5.42
Hα 0.65646 1.14–1.26 2.60–2.79 5.07–5.41
[NII] 0.65853 1.14–1.26 2.58–2.78 5.05–5.39
[SII] 0.67183 1.10–1.21 2.51–2.71 4.93–5.26
[SII] 0.67327 1.09–1.21 2.51–2.70 4.92–5.25
CaII 0.85004 0.66–0.75 1.78–1.93 3.69–3.95
CaII 0.85444 0.65–0.74 1.76–1.92 3.66–3.92
CaII 0.86645 0.63–0.72 1.72–1.87 3.60–3.85
[SIII] 0.90711 0.55–0.64 1.60–1.75 3.39–3.64
[SIII] 0.95332 0.48–0.56 1.48–1.61 3.18–3.41
Paγ 1.09411 0.29–0.36 1.16–1.28 2.64–2.84
Paβ 1.28216 0.10–0.16 0.84–0.94 2.11–2.28
[FeII] 1.64445 ... 0.44–0.51 1.42–1.56
Paα 1.87561 ... 0.26–0.33 1.12–1.24
Brγ 2.16612 ... 0.09–0.15 0.84–0.94

Notes. Wavelengths are from http://classic.sdss.org/dr6/algorithms/speclinefits.html and NIST (Kramida et al. 2018). All are listed for vacuum; those marked with an asterisk were converted from air to vacuum using the transformation in Ciddor (1996).

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