New quasars with Z = 3.4 and 3.7 and the surface density of very high redshift quasars

Astronomy and Astrophysics – Astronomy

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Astronomical Spectroscopy, Quasars, Red Shift, Density Distribution, Emission Spectra, Photographic Plates, Schmidt Telescopes

Scientific paper

The discovery on a UK Schmidt telescope low-dispersion IIIaF objective prism plate of a QSO with z = 3.7 is reported. This QSO is now the one with the second highest redshift known and lies in the same region in which a QSO with z = 3.61 has already been reported. A QSO with z = 3.4 is also noted. Before these observations, only seven QSOs with z of 3.4 or greater were known throughout the whole sky. When compared with the results of a search for QSOs with redshift between 2.7 and 3.3 on the same plate, these observations do not support suggestions of a redshift cutoff of about 3.5 in the QSO distribution, but rather support the suggestion of a steady decline from redshift of about two. It is shown here that deep searches over small areas of sky are unlikely to be successful in discovering QSOs at redshift over four and that such searches must be carried out over very large areas.

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