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K. Sugiyama∗a, K. Fujisawaba, K. Hachisukac, Y. Yonekurad , K. Motogib, Z. -Q. Shenc, M. Honmae, T. Hirotae, S. Sawada-Satoh f , Y. Muratag, A. Doig, R. Dodsonh, M. J. Riojah, S. P. Ellingseni, K.-T. Kim j, and H. Ogawak aGraduate school of Science and Engineering, Yamaguchi University, Japan bResearch Institute for Time Studies, Yamaguchi University, Japan cShanghai Astronomical Observatory, Chinese Academy of Sciences, China dCenter for Astronomy, Ibaraki University, Japan eVERA Project, National Astronomical Observatory of Japan (NAOJ), Japan f Mizusawa VLBI Observatory, NAOJ, Japan gThe Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan hInternational Center for Radio Astronomy Research, University of Western Australia, Australia iSchool of Mathematics and Physics, University of Tasmania, Australia jKorea Astronomy and Space Science Institute, 776 Daedeokdae-ro, South Korea kDepartment of Physical Science, Osaka Prefecture University, Japan

The VLBI imaging survey of the 6.7 GHz methanol masers using the JVN/EAVN