In this paper, we use large scale structure observations to test the redshift dependence of cosmic distance duality relation (CDDR), $$D_\mathrm{L}(1+z)^{-2}/D_\mathrm{A}=\eta (z)$$
D
L
(
1
+
z
)
-
2
/
D
A
=
η
(
z
)
, with $$D_\mathrm{L}$$
D
L
and $$D_\mathrm{A}$$
D
A
, being the luminosity and angular diameter distances, respectively. In order to perform the test, the following data set are considered: strong lensing systems and galaxy cluster measurements (gas mass fractions). No specific cosmological model is adopted, only a flat universe is assumed. By considering two $$\eta (z)$$
η
(
z
)
parametrizations, It is observed that the CDDR remain redshift independent within $$1.5\sigma $$
1.5
σ
which is in full agreement with other recent tests involving cosmological data. It is worth to comment that our results are independent of the baryon budget of galaxy clusters.