We present results from a search for gravitationally lensed galaxies
present in the Hubble Space Telescope (HST)/Wide Field Camera-3 (WFC3)
images of the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey
(CANDELS). We present one bona fide lens system in UDS and two compact
lens candidates in the GOODS-S field. The lensing system in UDS involves
two background galaxies, one at z=1.847 lensed to an arc and a
counterimage, and the second at a photometric redshift of
z=2.32^{+0.10}_{-0.06} lensed to a double image. We reconstruct the
lensed sources in the source plane and find in each of the two cases the
sources can be separated to a pair of galaxies. The sources responsible
for the arc are compact with effective radii of 0.3 to 0.4 kpc in WFC3
J_{125}-band and a total stellar mass and a star-formation rate of
2.1_{-0.4}^{+2.4} times 10^7 M_sun and 2.3_{-1.7}^{+ 0.6} M_sun yr^{-1},
respectively.The abnormally high H_{160}-band flux of this source is
likely due to OIII emission lines with a rest-frame equivalent width
about 700 Angstroms for OIII 5007 Angstroms. The sources responsible for
the double image have corresponding values of about 0.4 to 0.5 kpc,
1.4_{-0.8}^{+1.9} times 10^9 M_sun, and 8.7_{-7.0}^{+11.1} M_sun
yr^{-1}. Once completed CANDELS is expected to contain about 15 lensing
systems and will allow statistical studies on both lensing mass profiles
and z ~ 2 lensed galaxies.
