A Free-Form mass model of the Hubble Frontier Fields Cluster AS1063 (RXC
  J2248.7-4431) with over one hundred constraints
  We derive a free-form mass distribution for the massive cluster AS1063
(z=0.348) using the completed optical imaging from the Hubble Frontier Fields
programme. Based on a subset of 11 multiply lensed systems with spectroscopic
redshift we produce a lens model that is accurate enough to unveil new multiply
lensed systems, totalling over a 100 arclets, and to estimate their redshifts
geometrically. Consistency is found between this precise model and that
obtained using only the subset of lensed sources with spectroscopically
measured redshifts. Although a relatively large elongation of the mass
distribution is apparent relative to the X-ray map, no significant offset is
found between the centroid of our mass distribution and that of the X-ray
emission map, suggesting a relatively relaxed state for this cluster. For the
well resolved lensed images we provide detailed model comparisons to illustrate
the precision of our model and hence the reliability of our de-lensed sources.
A clear linear structure is associated with one such source extending approx.
23 kpc in length, that could be an example of jet-induced star formation, at
redshift z=3.1.
