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Table 4

Emission line fluxes for all the sources.

Line z spec Flux rms fλ (continuum) E W obs−frame L
Å erg s-1 cm-2 erg s-1 cm-2 Å-1 Å erg s-1
AGN5
Hβ 15 679.3 ± 11.5 − (2.2 ± 3.0)E-17 32.1E-19 ≥7 (0.5 ± 1.1)E+42
[OIII]4959 15 988.5 ± 12.9 − (8.9 ± 1.6)E-17 32.1E-19 ≥30 (3.3 ± 0.6)E+42
[OIII]5007 16 143.6 ± 4.6 2.2234 ± 0.0009 (26.6 ± 4.7)E-17f 32.1E-19 ≥80 (9.9 ± 1.8)E+42
[NII]6548 21 100.8 ± 9.7 − (7.2 ± 1.2)E-17 22.3E-19 ≥30 (2.7 ± 0.5)E+42
Hα 21 153.1 ± 6.9 2.2223 ± 0.0011 (22.5 ± 5.9)E-17f 22.3E-19 ≥100 (8.6 ± 2.2)E+42
[NII]6583 21 217.2 ± 11.1 − (21.7 ± 3.2)E-17f 22.3E-19 ≥95 (8.3 ± 1.2)E+42
[SII]doublet 21 651.8 ± 2.7 − (8.7 ± 5.2)E-17 22.3E-19 ≥40 (3.3 ± 2.0)E+42
BzK25
Lyα(R) 3830.3 ± 0.5 − (24.3 ± 2.0)E-17 24.0E-19 100 (8.5 ± 0.7)E+42
Hβ 15 303.0 ± 6.0 − (7.2 ± 4.3)E-17 20.0E-19 ≥18 (2.5 ± 1.5)E+42
[OIII]4959 15 605.1 ± 5.2 − (12.7 ± 1.9)E-17 20.0E-19 ≥32 (4.4 ± 0.7)E+42
[OIII]5007 15 756.2 ± 1.8 2.1461 ± 0.0003 (37.7 ± 5.7)E-17 20.0E-19 ≥94 (13.2 ± 2.0)E+42
[NII]6548 20 603.5 ± ?? − (2.8 ± 1.3)E-17f 11.6E-19 ≥12 (1.0 ± 0.5)E+42
Hα 20 650.8 ± 4.2 2.1458 ± 0.0006 (25.1 ± 2.6)E-17 11.6E-19 ≥100 (8.8 ± 0.9)E+42
[NII]6583 20 713.6 ± 78.9 − (8.3 ± 4.0)E-17 11.6E-19 ≥36 (2.9 ± 1.4)E+42
AGN26
Hβ 14 669.3 ± 14.7 − (22.7 ± 8.5)E-17 27.1E-19 130 (6.8 ± 2.5)E+42
[OIII]4959 14 958.9 ± 12.6 − (18.0 ± 2.5)E-17 27.1E-19 100 (5.3 ± 0.7)E+42
[OIII]5007 15 103.7 ± 5.2 2.0158 ± 0.0010 (53.5 ± 7.5)E-17 27.1E-19 320 (16.0 ± 2.2)E+42
[NII]6548 19 739.8 ± 36.3 − (20.5 ± 3.6)E-17 24.0E-19 85 (6.1 ± 1.0)E+42
Hα 19 784.7 ± 24.1 2.0138 ± 0.0037 (44.7 ± 4.3)E-17 24.0E-19 180 (13.4 ± 1.3)E+42
[NII]6583 19 845.0 ± 46.4 − (48.6 ± 4.5)E-17 24.0E-19 200 (14.5 ± 1.3)E+42
[SII]6718 20 252.0 ± 11.6 − (5.3 ± 3.6)E-17f 24.0E-19 20 (1.6 ± 1.1)E+42
[SII]6730 20 288.1 ± 17.5 − (16.1 ± 7.3)E-17f 24.0E-19 65 (4.8 ± 2.2)E+42
z2LAE3
Hβ 14 967.6 ± 12.4 − (10.2 ± 6.7)E-17 72.0E-19 ≥7 (3.3 ± 2.2)E+42
[OIII]4959 15 263.1 ± 6.5 − (44.7 ± 2.7)E-17f 72.0E-19 ≥30 (14.4 ± 0.9)E+42
[OIII]5007 15 410.8 ± 1.9 2.0771 ± 0.0004 (133.1 ± 7.9)E-17 72.0E-19 ≥90 (43.0 ± 2.5)E+42
[NII]6548 20 157.2 ± ?? − (5.0 ± 1.0)E-17 34.9E-19 ≥7 (1.6 ± 0.3)E+42
Hα 20 203.1 ± 4.9 2.0776 ± 0.0007 (58.6 ± 4.1)E-17 34.9E-19 ≥80 (18.9 ± 1.3)E+42
[NII]6583 20 265.9 ± 7.8 − (14.9 ± 3.1)E-17f 34.9E-19 ≥20 (4.8 ± 1.0)E+42
BX1
Lyα(R) 3921.8 ± 0.6 2.2260 ± 0.0005 (10.1 ± 0.8)E-17 4.9E-19 150 (3.9 ± 0.3)E+42
Hβ 15 691.5 ± 28.8 − (1.6 ± 1.5)E-17 10.3E-19 ≥8 (0.6 ± 0.6)E+42
[OIII]4959 15 986.7 ± 5.7 − (4.3 ± 0.4)E-17 10.3E-19 ≥20 (1.6 ± 0.2)E+42
[OIII]5007 16 149.8 ± 1.9 2.2246 ± 0.0004 (12.7 ± 1.2)E-17 10.3E-19 ≥60 (4.8 ± 0.5)E+42
[NII]6548 21 110.3 ± 47.8 − (0.5 ± 1.0)E-17 7.0E-19 ≥3 (0.2 ± 0.3)E+42
Hα 21 158.3 ± 5.4 2.2231 ± 0.0008 (4.1 ± 0.9)E-17 7.0E-19 ≥28 (1.6 ± 0.3)E+42
[NII]6583 21 224.1 ± ?? − (1.6 ± 2.8)E-17f 7.0E-19 ≥11 (0.6 ± 2.8)E+42
BX10
Lyα(R) 4403.4 ± 0.3 2.622 ± 0.0002 (9.7 ± 0.5)E-17 7.3E-19 103 (5.5 ± 0.3)E+42
Hβ 17 575.0 ± 19.9 − (7.0 ± 6.3)E-17 44.6E-19 ≥8 (4.0 ± 0.4)E+42
[OIII]4959 17 922.0 ± 20.6 − (6.5 ± 2.4)E-17 44.6E-19 ≥7 (3.7 ± 1.4)E+42
[OIII]5007 18 095.5 ± 11.6 2.6132 ± 0.0026 (19.3 ± 7.0)E-17f 44.6E-19 ≥22 (11.0 ± 4.0)E+42
Hα 6562.82 × 3.614 − ≤17.5E-17 35.3E-19 − ≤9.9E+42
BX4
[OIII]5007 5007.0 × 3.505 − (≤10.0)E-17f 18.9E-19 − ≤5.0E+42
[NII]6548 22 948.4 ± ?? − (1.9 ± 1.0)E-17 20.1E-19 ≥5 (0.9 ± 0.5)E+42
Hα 23 000.9 ± 8.7 2.5038 ± 0.0013 (16.6 ± 3.3)E-17 20.1E-19 ≥40 (8.2 ± 1.6)E+42
[NII]6583 23 071.0 ± 10.6 − (5.8 ± 3.0)E-17 20.1E-19 ≥14 (2.9 ± 1.5)E+42
BX7
Hβ 4863.0 × 3.418 − ≤7.5E-17 15.4E-19 − ≤3.4E+42
[OIII]4959 16 949.7 ± 10.0 − (4.4 ± 0.7)E-17 15.4E-19 ≥13 (2.0 ± 0.3)E+42
[OIII]5007 17 113.8 ± 3.6 2.4171 ± 0.0007 (13.0 ± 2.4)E-17f 15.4E-19 ≥40 (6.0 ± 1.0)E+42
[NII]6548 22 362.9 ± 82.1 − (0.5 ± 0.5)E-17 10.7E-19 ≥1 (0.2 ± 0.2)E+42
Hα 22 413.8 ± 4.0 2.4143 ± 0.0006 (10.5 ± 1.6)E-17 10.7E-19 ≥50 (4.8 ± 0.7)E+42
[NII]6583 22 483.4 ± 32.7 − (1.6 ± 1.6)E-17f 10.7E-19 ≥7 (0.7 ± 0.7)E+42
BX14
Hβ 16 373.0 ± 9.6 − (3.3 ± 2.6)E-17f 20.8E-19 ≥15 (1.4 ± 1.1)E+42
[OIII]4959 16 696.2 ± 11.7 − (5.2 ± 1.0)E-17f 20.8E-19 ≥24 (2.2 ± 0.4)E+42
[OIII]5007 16 857.8 ± 3.9 2.3660 ± 0.0008 (15.6 ± 3.0)E-17 20.8E-19 ≥70 (6.7 ± 1.3)E+42
[NII]6548 22 049.7 ± ?? − (0.2 ± 0.6)E-17f 14.0E-19 ≥0.7 (0.08 ± 0.3)E+42
Hα 22 099.9 ± 4.1 2.3665 ± 0.0006 (13.3 ± 2.3)E-17 14.0E-19 ≥47 (5.7 ± 1.0)E+42
[NII]6583 22 168.6 ± 51.6 − (0.6 ± 1.9)E-17f 14.0E-19 ≥2 (0.3 ± 0.8)E+42
BX16
Lyα(R) 4019.0 ± 1.2 2.3060 ± 0.0010 -(6.3 ± 1.1)E-17 12.3E-19 -45 −
Hβ 16 129.1 ± ?? − (2.9 ± 1.3)E-17 13.0E-19 ≥20 (2.4 ± 0.7)E+42
[OIII]4959 16 447.5 ± 15.0 − (1.9 ± 0.6)E-17f 13.0E-19 ≥6 (0.8 ± 0.2)E+42
[OIII]5007 16 606.7 ± 5.7 2.3159 ± 0.0011 (5.6 ± 1.7)E-17 13.0E-19 ≥40 (1.2 ± 0.5)E+42
[NII]6548 21 718.1 ± ?? − (0.6 ± 0.4)E-17f 11.5E-19 ≥3 (0.3 ± 0.2)E+42
Hα 21 767.5 ± 4.3 2.3159 ± 0.0007 (10.4 ± 1.6)E-17 11.5E-19 ≥45 (4.3 ± 0.7)E+42
[NII]6583 21 835.2 ± 13.4 − (1.7 ± 1.4)E-17f 11.5E-19 ≥7 (0.7 ± 0.6)E+42
LBG11
Lyα(R) 51 12.4 ± 0.6 3.2054 ± 0.0005 (3.0 ± 0.7)E-17 11.6E-19 34 (2.8 ± 0.7)E+42
Hβ 20 432.6 ± 14.4 − (2.9 ± 2.4)E-17 8.2E-19 ≥18 (2.7 ± 2.2)E+42
[OIII]4959 20 836.0 ± 16.0 − (2.6 ± 0.8)E-17f 8.2E-19 ≥16 (2.4 ± 0.7)E+42
[OIII]5007 21 037.7 ± 5.0 3.2006 ± 0.0010 (8.0 ± 2.3)E-17 8.2E-19 ≥50 (7.5 ± 2.1)E+42
LAE27
Lyα(R) 4966.7 ± 0.3 3.0856 ± 0.0002 (2.2 ± 0.2)E-17 4.4E-19 105 (1.9 ± 0.2)E+42
Hβ 19 860.8 ± 48.8 − (12.0 ± 13.3)E-17 32.5E-19 ≥19 (10.1 ± 11.3)E+42
[OIII]4959 20 252.8 ± 16.4 − (8.2 ± 2.6)E-17f 32.5E-19 ≥14 (7.0 ± 2.2)E+42
[OIII]5007 20 448.9 ± 5.0 3.0830 ± 0.0001 (25.8 ± 7.7)E-17 32.5E-19 ≥41 (21.9 ± 6.5)E+42
z3LAE2
Lyα(R) 5002.4 ± 0.5 3.1149 ± 0.0004 (2.3 ± 0.5)E-17 9.9E-19 74 (2.0 ± 0.4)E+42
Hβ 20 000.5 ± 11.4 − (12.3 ± 5.0)E-17f 29.6E-19 ≥20 (10.7 ± 6.8)E+42
[OIII]4959 20 395.3 ± 11.1 − (7.0 ± 1.5)E-17f 29.6E-19 ≥12 (6.1 ± 1.3)E+42
[OIII]5007 20 592.7 ± 3.1 3.1118 ± 0.0006 (20.9 ± 4.4)E-17 29.6E-19 ≥35 (18.2 ± 3.8)E+42
z2LAE2
Hβ 14 849.6 ± 5.7 − (11.7 ± 4.9)E-17f 20.0E-19 ≥30 (3.7 ± 1.6)E+42
[OIII]4959 15 142.8 ± 10.3 − (11.4 ± 1.5)E-17 20.0E-19 ≥30 (3.6 ± 0.5)E+42
[OIII]5007 15 289.3 ± 4.4 2.0528 ± 0.0009 (34.1 ± 4.6)E-17 20.0E-19 ≥90 (10.8 ± 1.5)E+42
Hα 6562.82 × 3.054 − ≤15.0E-17f 28.0E-19 − ≤4.8E+42
DB8
Lyα ≤2.8E+41phot
Hβ 15 952.8 ± 30.9 − (4.3 ± 3.4)E-17 15.0E-19 ≥14 (1.8 ± 1.4)E+42
[OIII]4959 16 288.1 ± 28.2 − (4.1 ± 0.9)E-17f 15.0E-19 ≥15 (1.7 ± 0.4)E+42
[OIII]5007 16 445.8 ± 8.0 2.2837 ± 0.0015 (12.5 ± 2.8)E-17 15.0E-19 ≥45 (5.1 ± 1.1)E+42
Hα 6562.82 × 3.285 − ≤5.0E-17 9.5E-19 − 2.3E+41phot
DB12
Lyα 1.6E+42phot
Hβ 15 518.0 ± 10.1 − (4.1 ± 3.0)E-17 16.0E-19 ≥12 (1.5 ± 1.1)E+42
[OIII]4959 15 824.3 ± 29.3 − (4.0 ± 1.4)E-17f 16.0E-19 ≥12 (1.5 ± 0.5)E+42
[OIII]5007 15 977.5 ± 7.0 2.1902 ± 0.0014 (12.0 ± 4.0)E-17 16.0E-19 ≥27 (4.4 ± 1.5)E+42
[NII]6548 20 907.8 ± 10.4 − (1.3 ± 0.9)E-17 18.3E-19 ≥3 (0.5 ± 0.3)E+42
Hα 20 955.4 ± 8.0 2.1922 ± 0.0012 (18.1 ± 3.2)E-17 18.3E-19 ≥50 (6.7 ± 1.2)E+42
[NII]6583 21 020.5 ± 33.0 − (3.9 ± 2.6)E-17 18.3E-19 ≥10 (1.4 ± 0.9)E+42
DB22
Lyα ≤2.8E+41phot
Hβ 4863.0 × 3.212 − ≤12.5E-17 22.8E-19 − ≤4.9E+42
[OIII]4959 15 930.3 ± 34.4 − (6.9 ± 1.7)E-17 22.8E-19 ≥14 (2.7 ± 0.7)E+42
[OIII]5007 16 084.5 ± 11.8 2.2116 ± 0.0024 (20.7 ± 5.7)E-17 22.8E-19 ≥40 (8.0 ± 2.2)E+42
Hα 6562.82 × 3.212 − ≤6.0E-17f 13.1E-19 − 3.9E+41phot

Notes.

(f)

means sky line residuals can affect the flux estimation. (R) refers to the fact that the rest-frame UV spectrum was normalized to the galaxy R band magnitude. Lyα emission line fluxes of “BX” galaxies are estimated from GOODS public spectra (5.7 Å/pixel, VIMOS-LR); of LAE27 are calculated from spectra obtained with VIMOS (2.57 Å/pixel, VIMOS-MR), of z3LAE2 and LBG11 with IMACS (1.3 Å/pixel) by MUSYC. Optical emission lines are obtained from our 7 Å/pixel spectra. To determine redshifts we assumed vacuum λLyα = 1215.67 Å, λ[OIII] 5007 = 5008.239 Å, λHα = 6564.614 Å. Column 1−3: emission line names, their central wavelengths, and implied redshift. An “??” indicates a formally infinite error. Column 4: emission line integrated fluxes. Column 5: continuum flux densities. Column 6: obs-frame equivalent widths of the emission lines listed in the 1st column. In the case of lower limits, the equivalent width is estimated from the 2σ upper limit of the continuum. The continuum σ is defined as its root-mean-square. Column 7: emission line luminosities. For a few of the DB sources we report photometric Hα luminosity as phot.

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