  The paper presents the first results of the ongoing spectropolarimetric
monitoring of magnetic fields of stars, whose chemically peculiar nature has
been previously revealed with the 1-m SAO RAS telescope. We selected the sample
candidates using the photometric data of the Kepler and TESS space missions.
The efficiency of the method of searching for new CP stars based on photometric
light curves has been confirmed. We present the magnetic field measurements and
estimate the atmospheric parameters of the objects under study.
