Changing Look AGNs (CL AGNs) are objects which undergo dramatic variability of the emission line profiles and classification type which can move from one spectral class to another within very short time interval (from days to years). We started a project to use various telescopes worldwide to carry out spectral and photometric multiwavelength (from IR to X-ray) monitoring of a sample of CL AGNs. The telescopes we have been using include the 2.5-m, 1.25-m, 0.6-m, 0.5-m, 0.4-m (MASTER) telescopes of SAI MSU, SHAO 2-m and 0.6-m, SALT 11- m, SAAO 1.9-m, WIRO 2.3-m, the 1.0-m at Weihai Observatory of Shandong University, Swift XRT, and UVOT. In this talk, I will introduce the project and present some recent results for NGC2617 and NGC1566.