Optical Identification of Four Hard X-ray Sources from the INTEGRAL Sky
  Surveys
  We continue the study begun in Karasev et al. (2018) and present the results
of our optical identifications of four hard X-ray sources from the INTEGRAL sky
surveys. Having first improved the positions of these objects in the sky with
the X-ray telescope (XRT) of the Swift observatory, we have identified their
counterparts using optical and infrared sky survey data. Then, we have obtained
optical spectra for the supposed counterparts with the RTT-150 Russian-Turkish
telescope and the AZT-33IK telescope. This has allowed the nature of the
objects under study to be established. The sources IGR J11079+7106 and IGR
J12171+7047 have turned out to be extragalactic in nature and be Seyfert 1 and
2 galaxies, respectively, with the second object being characterized by a large
absorption column density. The source IGR J18165-3912 is most likely an
intermediate polar with a very high luminosity. The fourth source, IGR
J20596+4303, is a chance superposition of two objects - a Seyfert 2 galaxy and
a cataclysmic variable.
