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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.

(a)

3-σ upper limit estimated from the continuum S/N;

(b)

synthetic magnitude estimated by convolving the spectrum with the LBC z-band filter response;

(c)

LAE2 is not detected in the continuum in the MUSE spectrum and is undetected both in the LBT/LBC and HST photometry, so we adopted the 5σ magnitude limit measured in the ACS F850LP image.

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