  We report the discovery, spectroscopic confirmation and first lens models of
the first two, strongly lensed quasars from a combined search in WISE and Gaia
over the DES footprint.
  The four-image lensWGD2038-4008 (r.a.=20:38:02.65, dec.=-40:08:14.64) has
source- and lens-redshifts $z_{s}=0.777 \pm 0.001$ and $z_l = 0.230 \pm 0.002$
respectively. Its deflector has effective radius $R_{\rm eff} \approx
3.4^{\prime\prime}$, stellar mass $\log(M_{\star}/M_{\odot}) =
11.64^{+0.20}_{-0.43}$, and shows extended isophotal shape variation. Simple
lens models yield Einstein radii $R_{\rm E}=(1.30\pm0.04)^{\prime\prime},$ axis
ratio $q=0.75\pm0.1$ (compatible with that of the starlight) and considerable
shear-ellipticity degeneracies. The two-image lensWGD2021-4115
(r.a.=20:21:39.45, dec.=--41:15:57.11) has $z_{s}=1.390\pm0.001$ and $z_l =
0.335 \pm 0.002$, and Einstein radius $R_{\rm E} = (1.1\pm0.1)^{\prime\prime},$
but higher-resolution imaging is needed to accurately separate the deflector
and faint quasar image. We also show high-rank candidate doubles selected this
way, some of which have been independently identified with different
techniques, and discuss a DES+WISE quasar multiplet selection.
