  We present the results of our identification of 14 X-ray sources detected in
the eastern Galactic sky ($0<l<180 \circ$ ) in the 4-12 keV energy band on the
combined map of the first five all-sky surveys (from December 2019 to March
2022) with the Mikhail Pavlinsky ART-XC telescope onboard the SRG observatory.
All 14 sources are reliably detected by the SRG/eROSITA telescope in the 0.2-8
keV energy band. Six of them have been detected in X-rays for the first time,
while the remaining ones have already been known previously as X-ray sources,
but their nature has remained unknown. We have taken optical spectra for 12
sources with the 1.6-m AZT-33IK telescope at the Sayan Observatory (the
Institute of Solar-Terrestrial Physics, the Siberian Branch of the Russian
Academy of Sciences). For two more objects we have analyzed the archival
spectra taken during the 6dF survey. All objects have turned out to be Seyfert
galaxies (one NLSy1, three Sy1, four Sy1.9, and six Sy2) at redshifts
$z=0.015-0.238$. Based on data from the eROSITA and ART-XC telescopes onboard
the SRG observatory, we have obtained X-ray spectra for all objects in the
energy range 0.2-12 keV. In four of them the intrinsic absorption exceeds
$N_{\rm H}>10^{22}$ cm$^{-2}$ at a 90% confidence level, with one of them being
probably heavily obscured ($N_{\rm H}>5\times 10^{22}$ cm$^{-2}$ with 90%
confidence). This paper continues our series of publications on the
identification of hard X-ray sources detected during the all-sky survey with
the SRG orbital X-ray observatory.
