  We report upon the follow up of 34 candidate lensed quasars found in the Dark
Energy Survey using NTT-EFOSC, Magellan-IMACS, KECK-ESI and SOAR-SAMI. These
candidates were selected by a combination of double component fitting,
morphological assessment and color analysis. Most systems followed up are
indeed composed of at least one quasar image and 13 with two or more quasar
images: two lenses, four projected binaries and seven Nearly Identical Quasar
Pairs (NIQs). The two systems confirmed as genuine gravitationally lensed
quasars are one quadruple at $z_s=1.713$ and one double at $z_s=1.515$. Lens
modeling of these two systems reveals that both systems require very little
contribution from the environment to reproduce the image configuration.
Nevertheless, small flux anomalies can be observed in one of the images of the
quad. Further observations of 9 inconclusive systems (including 7 NIQs) will
allow to confirm (or not) their gravitational lens nature.
