Lens Models of Herschel-Selected Galaxies From High-Resolution Near-IR
  Observations
  We present Keck-Adaptive Optics and Hubble Space Telescope high resolution
near-infrared (IR) imaging for 500 um-bright candidate lensing systems
identified by the Herschel Multi-tiered Extra-galactic Survey (HerMES) and
Herschel Astrophysical Terahertz Survey (H-ATLAS). Out of 87 candidates with
near-IR imaging, 15 (~17%) display clear near-IR lensing morphologies. We
present near-IR lens models to reconstruct and recover basic rest-frame optical
morphological properties of the background galaxies from 12 new systems.
Sources with the largest near-IR magnification factors also tend to be the most
compact, consistent with the size bias predicted from simulations and pre-
vious lensing models for sub-millimeter galaxies. For four new sources that
also have high-resolution sub-mm maps, we test for differential lensing between
the stellar and dust components and find that the 880 um magnification factor
(u_880) is ~1.5 times higher than the near-IR magnification factor (u_NIR), on
average. We also find that the stellar emission is ~2 times more extended in
size than dust. The rest-frame optical properties of our sample of
Herschel-selected lensed SMGs are consistent with those of unlensed SMGs, which
suggests that the two populations are similar.
