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Spectropolarimetric efforts in the last few years have provided an efficientmethod that is based on the profiles of the polarization plane position angleof broad emission lines in active galactic nuclei (AGNs). Here we present blackhole measurements of SBS 1419+538 using spectropolarimetric observations in theMg II spectral band. The observations are performed by 6m telescope of SAO RASusing SCORPIO-2. We found a good agreement for the estimated supermassive blackhole (SMBH) mass for this object using spectropolarimetry when compared withthe mass obtained using other methods.

The first supermassive black hole mass measurement in active galactic nuclei using the polarization of broad emission line Mg II