  We present Low-Frequency Array (LOFAR) telescope observations of the
radio-loud gravitational lens systems MG 0751+2716 and CLASS B1600+434. These
observations produce images at 300 milliarcseconds (mas) resolution at 150 MHz.
In the case of MG 0751+2716, lens modelling is used to derive a size estimate
of around 2 kpc for the low-frequency source, which is consistent with a
previous 27.4 GHz study in the radio continuum with Karl G. Jansky Very Large
Array (VLA). This consistency implies that the low-frequency radio source is
cospatial with the core-jet structure that forms the radio structure at higher
frequencies, and no significant lobe emission or further components associated
with star formation are detected within the magnified region of the lens. CLASS
B1600+434 is a two-image lens where one of the images passes through the
edge-on spiral lensing galaxy, and the low radio frequency allows us to derive
limits on propagation effects, namely scattering, in the lensing galaxy. The
observed flux density ratio of the two lensed images is 1.19 +/- 0.04 at an
observed frequency of 150 MHz. The widths of the two images give an upper limit
of 0.035 kpc m^-20/3 on the integrated scattering column through the galaxy at
a distance approximately 1 kpc above its plane, under the assumption that image
A is not affected by scattering. This is relatively small compared to limits
derived through very long baseline interferometry (VLBI) studies of
differential scattering in lens systems. These observations demonstrate that
LOFAR is an excellent instrument for studying gravitational lenses. We also
report on the inability to calibrate three further lens observations: two from
early observations that have less well determined station calibration, and a
third observation impacted by phase transfer problems.
