Near-IR spectra (zoomed around Hα) of the three X-ray selected obscured AGNs with evidence for a broad component of Hα. The red line shows the fit resulting from a combination of a broad Hα Gaussian component (blue line), narrow Gaussian components of Hα, [NII] and, in the case of Abell2690#29, [SII] (green lines) and a linear continuum. The bottom panels show the sky spectrum in arbitrary units.