Galaxy evolution studies in clusters: the case of Cl0024+1652 cluster
  galaxies at z$\sim$0.4
  Studying the transformation of cluster galaxies contributes a lot to have a
clear picture of evolution of the universe. Towards that we are studying
different properties (morphology, star formation, AGN contribution and
metallicity) of galaxies in clusters up to $z\sim1.0$ taking three different
clusters: 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 tunable
filters data from GLACE survey taken with GTC 10.4 m telescope and other public
data, while for Virgo we used public data. We did the morphological
classification of 180 galaxies in ZwCl0024+1652 using galSVM, where 54\% and
46\% of galaxies were classified as early-type (ET) and late-type (LT)
respectively. We did a comparison between the three clusters within the
clustercentric distance of 1Mpc and found that ET proportion (decreasing with
redshift) dominates over the LT (increasing with redshift) throughout. We
finalized the data reduction for ZwCl0024+1652 cluster and identified 46 [OIII]
and 73 H$\beta$ emission lines. For this cluster we have classified 22 emission
line galaxies (ELGs) using BPT-NII diagnostic diagram resulting with 14
composite, 1 AGN and 7 star forming (SF) galaxies. We are using these results,
together with the public data, for further analysis of the variations of
properties in relation to redshift within $z<1.0$.
