Abstract
We have analyzed images from the VST ATLAS survey to identify candidate
gravitationally lensed quasar systems in a sample of WISE sources with W1 - W2
> 0.7. Results from followup spectroscopy with the Baade 6.5 m telescope are
presented for seven systems. One of these is a quadruply lensed quasar. Two are
projected superpositions of two quasars at different redshifts. In one system
two quasars, though at the same redshift, have very different emission line
profiles, and constitute a physical binary. In three systems the component
spectra are consistent with the lensing hypothesis, after allowing for
micro-lensing. But as no lensing galaxy is detected in these three, we classify
them as nearly identical quasar pairs. More extensive observations are needed
to establish whether they are lensed quasars or physical binaries.
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