The construction of the cosmic distance-duality relation ( CDDR ) has been widely studied .
However , its consistency with various new observables remains a topic of interest .
We present a new way to constrain the CDDR \eta ( z ) using different dynamic and geometric properties of strong gravitational lenses ( SGL ) along with SNe Ia observations .
We use a sample of 102 SGL with the measurement of corresponding velocity dispersion \sigma _ { 0 } and Einstein radius \theta _ { E } .
In addition , we also use a dataset of 12 two image lensing systems containing the measure of time delay \Delta t between source images .
Jointly these two datasets give us the angular diameter distance D _ { A _ { ol } } of the lens .
Further , for luminosity distance , we use the 740 observations from JLA compilation of SNe Ia .
To study the combined behavior of these datasets we use a model independent method , Gaussian Process ( GP ) .
We also check the efficiency of GP by applying it on simulated datasets , which are generated in a phenomenological way by using realistic cosmological error bars .
Finally , we conclude that the combined bounds from the SGL and SNe Ia observation do not favor any deviation of CDDR and are in concordance with the standard value ( \eta = 1 ) within 2 \sigma confidence region , which further strengthens the theoretical acceptance of CDDR . Keywords : Cosmic distance duality relation , Strong gravitational lensing , JLA SNe Ia , Gaussian process .