Losing a minute every two years: SRG X-ray view of the rapidly accelerating X-ray pulsar SXP 1323

SXP 1323 is a peculiar high-mass X-ray binary located in the Small Magellanic Cloud, renowned for its rapid spin-up. We investigate first time broadband properties of SXP1323, as observed by Mikhail Pavlinsky ART-XC and eRosita telescopes on board SRG observatory. Using eRosita, data we produced 1-20 keV spectrum estimated pulsed fraction above 8 keV. With addition archival XMM-Newton observations traced evolution spin period over last five years found that after 2016 source switched to linear spin-up with rate -29.9 s yr$^{-1}$. Broadband typical accreting pulsars, steep powerlaw index ($\Gamma$=-0.15) exponential cutoff energy 5.1 No significant difference between spectra obtained states without pulsations were found.