Mis V0120 Mis V0120 is 54 arcsec from V1465 Cyg, a rapidly changing irregular Mis V0120 variable, at R.A. 20h01m49.98s, Decl. +33{deg}14'24.3" (2000.0) in the Mis V0120 GCVS0 But MisV0120 is identified with IRAS 20000+3305, so it is Mis V0120 probably Mira type or semi-regular type. Considering the large Mis V0120 distance and the type difference, we concluded that MisV0120 is Mis V0120 another new variable star. However, no star brighter than 14.6 mag was Mis V0120 detected on our unfiltered CCD images taken on JD 2451299.20, Mis V0120 2451367.18, 2451392.11 and 2451394.16 at the position of V1465 Cyg. Mis V0120 Therefore, it cannot be completely ruled out that the position of Mis V0120 V1465 Cyg is inaccurate and MisV0120 is identical with V1465 Cyg. Mis V0130 MisV0130 is identified with HS 1332, one of the variable stars Mis V0130 discovered by FASTT, Flagstaff Astrometric Scanning Transit Telescope Mis V0130 (cf. Henden and Stone, 1998AJ....115..296H). Mis V0134 NSV 11661 is 1.7 arcmin from MisV0134. No star brighter than 15.2 mag Mis V0134 was detected at the position of NSV 11661 on our unfiltered CCD images Mis V0134 taken on JD 2451298.21, 2451330.22 and 2451367.17. However, Mis V0134 considering the large angular distance, MisV0134 is probably another Mis V0134 variable object. Mis V0163 MisV0163 is identified with a carbon star CS 4613. Mis V0173 V2000 Cyg is 4.3 arcmin from MisV0173. V2000 Cyg was detected on our Mis V0173 unfiltered CCD images at around 14 mag. No variability was found on Mis V0173 our images. However, considering the large distance, MisV0173 is Mis V0173 probably another new variable star. Mis V0205 V393 Cyg is 3.4 arcmin from MisV0205, that was detected on our Mis V0205 unfiltered CCD image as a 10 mag star. MisV0205 is thus another new Mis V0205 variable star. Mis V0212 BL Sct is 4.1 arcmin from MisV0212. No star brighter than 14.7 mag was Mis V0212 detected at the position of BL Sct on our unfiltered CCD images on Mis V0212 Apr. 14 and May 20. However, considering the large angular distance, Mis V0212 MisV0212 is probably another variable object. Mis V0217 NSV 12624 is 1.0 arcmin from MisV0217. No star brighter than 14.8 mag Mis V0217 was detected at the position of NSV 12624 on Apr. 30 and July 24. Mis V0217 Therefore, MisV0217 may be identified with NSV 12624. Mis V0231 NSV 12646 is 2.9 arcmin from MisV0231, that was detected on our Mis V0231 unfiltered CCD image as a 8.5 mag star. Therefore, MisV0231 is another Mis V0231 new variable star. Mis V0244 NSV 11612 is 4.6 arcmin from MisV0244, that was detected on our Mis V0244 unfiltered CCD image. It was fainter than 14.7 mag on Apr. 14, but Mis V0244 11.5 mag on July 24. Therefore, MisV0244 is another new variable star. Mis V0251 NSV 12738 is 4.4 arcmin from MisV0251. However, it was detected on Mis V0251 our unfiltered CCD image as around 16 mag. Therefore, MisV0251 is Mis V0251 another new variable star. Mis V0261 EM Oph is 4.5 arcmin from MisV0261. QY Oph is 4.0 arcmin from Mis V0261 MisV0263. IN Sco is 4.7 arcmin from MisV0265. No star brighter than Mis V0261 14 mag was detected at these positions on our unfiltered CCD images. Mis V0261 However, considering the large distance, MisV0261, MisV0263 and Mis V0261 MisV0265 are probably new variable objects. Mis V0297 MisV0297 is located at a distance of 129 arcsec from the cataloged Mis V0297 position of the obscure nova DZ Ser. A slight uncertainly of the Mis V0297 coordinates reported among existing references (Duerbeck, 1987, Space Mis V0297 Sci. Rev., 45, 58 ) may have led to a possible identification. More Mis V0297 extensive study of the new variable and the comparison with the Mis V0297 discovery material of DZ Ser are needed to clarify the situation. Mis V0314 V1191 Oph is 1.2 arcmin from MisV0314, that was detected on Kadota's Mis V0314 unfiltered CCD images as a 13 mag star. MisV0314 is thus a new Mis V0314 variable star. Mis V0348 V1002 Sgr is 1.7 arcmin from MisV0348, that was detected as a Mis V0348 12.5mag star. Mis V0348 is thus another new variable star. Mis V0360 is identified with a carbon star CS4603. Mis V0372 is within the positional error range of an X-ray source Mis V0372 1RXPJ180245-2942.3 at RA=18h02m45.6s, DE=-29{deg}42'20" (2000.0). Mis V0391 V2084 Sgr is 3.7 arcmin from MisV0391, that was detected on Kadota's Mis V0391 unfiltered CCD images as another variable star between 9.8 and Mis V0391 10.8mag. Therefore, Mis V0391 is another new variable star. Mis V0393 NSV 12730 is 2.8 arcmin from MisV0393, that was detected as another Mis V0393 variable star between 11.2 and 12.0 mag. Therefore, Mis V0393 is Mis V0393 another new variable star. Mis V0395 The photometry of MisV0395 was obtained as NGC 6194 No. 1130, which Mis V0395 shows it is a red star (Mermilliod et al., 1994, Catalogue of Mean Mis V0395 UBV Data on Stars, Sringer-Verlag) Mis V0438 NSV 11613 is 3.1 arcmin from MisV0438. No star brighter than 15.0mag Mis V0438 was detected at the position of NSV 11613 on Kadota's unfiltered CCD Mis V0438 images. However, considering the large angular distance, MisV0438 is Mis V0438 probably another new variable object Mis V0471 TY Oph is 2.1 arcmin from MisV0471, that was detected as a 7.5mag Mis V0471 star. Mis V0481 MisV0481 is identified with a star at RA=17h58m7, DE=-28{deg}12' Mis V0481 (2000.0) whose spectral type is M8III (Buscombe, 1995, Twelfth Mis V0481 General Catalogue of MK Spectral Classification, Northwestern Univ., Mis V0481 Evanston, Illinois, See Cat. ) Mis V0498 MisV0498 is identified with an S-type star GCSS1018 (Stephenson, Mis V0498 1984, General Catalogue of Galactic S Stars, Cat. .