Three of the brightest maser spots from Cloud 5 of G24.33+00.12. They are indicated by red dots in the spectrum presented in the middle panel. Their LSR velocities are given above each image. The images in the middle panel present the subtraction of the emission as indicated above each image. The synthesized beam is presented in the left bottom corners of each image and the noise level is also given. The bottom panel presents the deconvolved size of a maser spot vs. natural logarithm of its peak flux density. The dot diameters in the spectrum and in the last dependence are proportional to the deconvolved size of the maser spot.