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Here, we present the search algorithm and criteria for distinguishing candidates from spurious Ly{alpha} forest lines. In addition, we compare our findings with simulations of the Ly{alpha} forest in order to estimate the detectability of OVI doublets over various redshift intervals. We have obtained a sample of 1756 OVI doublet candidates with rest-frame equivalent width (EW)&gt;=0.05{AA} in 855 active galactic nuclei spectra (out of 3702 objects with redshifts in the accessible range for OVI detection).</description><source format="bibcode">2010AJ....140..817F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/140/817</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/354/L25">J/MNRAS/354/L25 : MgII absorbers in SDSS QSOs (Bouche+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/639/766">J/ApJ/639/766 : 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