The survey data of Wide-field Infrared Survey Explorer ( WISE ) provide an opportunity for the identification of galaxy clusters .
We present an efficient method for detecting galaxy clusters by combining the WISE data with SuperCOSMOS and 2MASS data .
After performing star-galaxy separation , we calculate the number of companion galaxies around the galaxies with photometric redshifts previously estimated by the SuperCOSMOS , 2MASS and WISE data .
A scaled richness is then defined to identify clusters .
From a sky area of 275 { \deg } ^ { 2 } coincident with Sloan Digital Sky Survey Stripe 82 region , we identify 302 clusters in the redshift range of 0.1 < z < 0.35 , 247 ( 82 \% ) of which are previously known SDSS clusters .
The results indicate that our method is efficient for identifying galaxy clusters by using the all sky data of the SuperCOSMOS , 2MASS and WISE .