Table 1.
Identified LBGs and LAEs.
ID | mag | MUV | log SFR | Redshift | Instrument | Lyα |
|
---|---|---|---|---|---|---|---|
z-band | Flux | EW | |||||
(1) | (2) | (3) | (4) | (5) | (6) | ||
22914 | 25.45 ± 0.22 | −21.61 | 1.70 | 6.319 ± 0.001 | DEIMOS | <3 (a) | <5 |
20654 | 25.27 ± 0.17 | −21.77 | 1.97 | 6.226 ± 0.002 | FORS2 | 8.5 ± 0.2 | 14 |
18262 | 25.70 ± 0.20 | −21.34 | 1.32 | 6.238 ± 0.004 | FORS2 | 5.3 ± 0.3 | 13 |
03909 | 25.55 ± 0.19 | −21.51 | 1.55 | 6.320 ± 0.003 | MODS | 5.0 ± 0.3 | 16 |
LAE1 | ≈27 (b) | −20.03 | 0.40 | 6.219 ± 0.002 | MUSE | 3.7 ± 0.2 | 27 |
LAE2 | >26.5 (c) | >−20.5 | <0.6 | 6.355 ± 0.001 | MUSE | 3.0 ± 0.2 | >11 |
Notes. (1) Source ID; (2) AB total magnitude. IDs and mags are from Balmaverde et al. (2017), except for the two MUSE-detected LAEs and ID22914 (see Appendix A); (3) monochromatic magnitude at 1350 Å; (4) logarithm of the star formation rate in units of M⊙ yr−1, computed from the UV luminosity adopting the Kennicutt (1998) calibration; (5) line fluxes in units of 10−18 erg s cm−2; (6) rest-frame equivalent widths in Å.
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