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Table 2.
Different redshift ranges we consider in isolating strong emission lines to specific Spitzer/IRAC bands.
Spitzer/IRAC band | No. of sources | |||
---|---|---|---|---|
Redshift range | [3.6] | [4.5] | MUSE-Deep | MUSE-Wide |
2.900 < z1 < 3.309 | [S III] 9068.6 Å | 155 | 131 | |
3.416 < z2 < 3.829 | [S III] 9068.6 Å | 192 | 146 | |
3.856 < z3 < 4.514 | Hα | [S III] 9068.6 Å | 156 | 164 |
4.532 < z4 < 4.955 | Hα | 116 | 84 | |
5.103 < z5 < 5.329 | Hα | 36 | 32 |
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