We present X-ray and optical properties of the optically confirmed galaxy cluster sample from the 3XMM/SDSS Stripe 82 cluster survey .
The sample includes 54 galaxy clusters in the redshift range of 0.05-1.2 , with a median redshift of 0.36 .
We first present the X-ray temperature and luminosity measurements that are used to investigate the X-ray luminosity-temperature relation .
The slope and intercept of the relation are consistent with those published in the literature .
Then , we investigate the optical properties of the cluster galaxies including their morphological analysis and the galaxy luminosity functions .
The morphological content of cluster galaxies is investigated as a function of cluster mass and distance from the cluster center .
No strong variation of the fraction of early and late type galaxies with cluster mass is observed .
The fraction of early type galaxies as a function of cluster radius varies as expected .
The individual galaxy luminosity functions ( GLFs ) of red sequence galaxies were studied in the five ugriz bands for 48 clusters .
The GLFs were then stacked in three mass bins and two redshift bins .
Twenty clusters of the present sample are studied for the first time in X-rays , and all are studied for the first time in the optical range .
Altogether , our sample appears to have X-ray and optical properties typical of ‘ ‘ average ’ ’ cluster properties .