Table 3: Emission lines in MRC0406-244.
Line $\lambda_0$ $\lambda_{\rm obs}$ z FWHM Flux
(1) (2) (3) (4) (5) (6)
H$\beta $ 4861 1.66532 $\pm$ 0.00034 2.42587 $\pm$ 0.00071 1250 $\pm$ 83 1.9 $\pm$ 0.1
[OIII] 4959 1.69860 $\pm$ 0.00034 2.42528 $\pm$ 0.00069 1524 $\pm$ 93 2.2 $\pm$ 0.1
[OIII] 5007 1.71495 $\pm$ 0.00034 2.42510 $\pm$ 0.00068 1349 $\pm$ 81 6.6 $\pm$ 0.4
[OI] 6300 2.15777 $\pm$ 0.00045 2.42503 $\pm$ 0.00072 826 $\pm$ 65 0.74 $\pm$ 0.07
H$\alpha +[$NII] 6563, 6583 2.24879 $\pm$ 0.00045 2.42647 $\pm$ 0.00060 1756 $\pm$ 106 9.75 $\pm$ 0.59
[SII] 6716, 6731 2.30292 $\pm$ 0.00048 2.42492 $\pm$ 0.00071 1590 $\pm$ 102 2.40 $\pm$ 0.16
Column (1) - line. Column (2) - rest-frame wavelength in Å. Column (3) - observed wavelength in Å. Column (4) - redshift. Column (5) - rest-frame FWHM, corrected for instrumental resolution in km s-1. Column (6) - line flux in units of 10-15 erg s-1 cm-2. For H$\alpha $, [NII] $\lambda \lambda $6548, 6583 and [NII $]\lambda\lambda$6716, 6731 we give the values for the blended lines, respectively.

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