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Studying the transformation of cluster galaxies contributes a lot to have aclear picture of evolution of the universe. Towards that we are studyingdifferent properties (morphology, star formation, AGN contribution andmetallicity) of galaxies in clusters up to $z\sim1.0$ taking three differentclusters: ZwCl0024+1652 at $z\sim0.4$, RXJ1257+4738 at $z\sim0.9$ and Virgo at$z\sim0.0038$. For ZwCl0024+1652 and RXJ1257+4738 clusters we used tunablefilters data from GLACE survey taken with GTC 10.4 m telescope and other publicdata, while for Virgo we used public data. We did the morphologicalclassification of 180 galaxies in ZwCl0024+1652 using galSVM, where 54\% and46\% of galaxies were classified as early-type (ET) and late-type (LT)respectively. We did a comparison between the three clusters within theclustercentric distance of 1Mpc and found that ET proportion (decreasing withredshift) dominates over the LT (increasing with redshift) throughout. Wefinalized the data reduction for ZwCl0024+1652 cluster and identified 46 [OIII]and 73 H$\beta$ emission lines. For this cluster we have classified 22 emissionline galaxies (ELGs) using BPT-NII diagnostic diagram resulting with 14composite, 1 AGN and 7 star forming (SF) galaxies. We are using these results,together with the public data, for further analysis of the variations ofproperties in relation to redshift within $z<1.0$.

Galaxy evolution studies in clusters: the case of Cl0024+1652 cluster galaxies at z$\sim$0.4