Quasar variability (Wold+, 2007)

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Scientific paper

The sample was formed by matching objects categorized as having broad emission lines at redshifts z<0.75 in the SDSS DR2 (Abazajian et al., 2004AJ....128..502A, http://www.sdss.org/dr2/ ) with sources in the 200k Light Curve Catalogue of the QUEST1 variability survey (Rengstorf et al., 2004, Cat. ).
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