  We here report a spectroscopic identification of two new changing-look AGNs
(CL-AGNs): SDSS\,J104705.16+544405.8 and SDSS\,J120447.91+170256.8 both with a
"turn-off" type transition from type 1 to type 1.8/1.9. The identification is
arrived by a follow-up spectroscopic observation of the five changing-look AGN
(CL-AGN) candidates that are extracted from the sample recently released in
Macleod et al. The candidates are extract by the authors from the Sloan Digit
Sky Survey Data Release 7 spectroscopically confirmed quasars with large
amplitude variability. By compiling a sample of 26 previously identified
CL-AGNs, we confirm the claim in Macleod et al. that CL-AGNs tend to be biased
against low Eddington ratio, and identify an overlap between the CL-AGNs at
their dim state and the so-called intermediate-type AGNs. The overlap implies
that there two populations of the intermediate-type AGNs with different
origins. One is due to the torus orientation effect, and the another the
intrinsic change of the accretion rate of the central supermassive blackholes.
