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

The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2016 follow-up campaign. II. New quasar lenses from double component fitting