Dependence of the extinction on distance for the investigated area up to d = 200 pc. Stars with photometric distances are plotted as dots and stars with Gaia distances as circles. The stars with Gaia distances and four numbered stars withphotometric distances on the rising part of the extinction are shown with the error crosses. The black broken curve designates the extinction rise with distance in the diffuse Galactic dust layer for b = +36.75° according to the exponential Parenago (1945) law.