XTE J1118+480 fading, visually confirmed The reported fading trend of the X-ray nova, XTE J1118+480, has been also confirmed visually. YYYYMMDD(UT) mag observer 20000513.906 126 (P. A. Dubovsky) 20000513.928 128 (R. J. Bouma) 20000513.998 127 (M. Reszelski) 20000514.891 127 (E. Muyllaert) 20000514.926 127 (R. J. Bouma) 20000514.928 128 (G. Poyner) 20000515.244 126 (M. Simonsen) 20000515.913 126 (P. A. Dubovsky) 20000517.931 126 (P. A. Dubovsky) 20000518.899 128 (E. Muyllaert) 20000519.938 127 (H. McGee) 20000519.940 129 (G. Poyner) 20000519.981 128 (E. Muyllaert) 20000519.992 126 (C. P. Jones) 20000519.994 130 (M. Reszelski) 20000520.949 128 (R. J. Bouma) 20000521.497 131 (T. Watanabe) 20000521.522 130 (T. Watanabe) 20000521.533 131 (T. Watanabe) 20000521.546 130 (T. Watanabe) 20000521.557 130 (T. Watanabe) 20000521.565 131 (T. Watanabe) 20000521.576 130 (T. Watanabe) 20000521.585 131 (T. Watanabe) 20000521.591 130 (T. Watanabe) 20000521.858 127 (P. A. Dubovsky)