IP Peg observations (update) Since Sep. 24.75 UT: YYMMDD(UT) mag observer 970924.751 123 (T. Kinnunen) 970924.780 124 (T. Kinnunen) 970924.784 127 (T. Kinnunen) 970924.786 127 (T. Kinnunen) 970924.787 130 (T. Kinnunen) 970924.788 129 (T. Kinnunen) 970924.790 132 (T. Kinnunen) 970924.790 132 (T. Kinnunen) 970924.791 137 (T. Kinnunen) 970924.792 137 (T. Kinnunen) 970924.792 139 (T. Kinnunen) 970924.793 136 (T. Kinnunen) 970924.794 136 (T. Kinnunen) 970924.794 137 (T. Kinnunen) 970924.795 134 (T. Kinnunen) 970924.796 131 (T. Kinnunen) 970924.797 133 (T. Kinnunen) 970924.799 127 (T. Kinnunen) 970924.799 128 (T. Kinnunen) 970924.800 127 (T. Kinnunen) 970924.801 125 (T. Kinnunen) 970924.84 121 (E. Schweitzer) 970924.856 123 (T. Kinnunen) 970924.86 127 (E. Schweitzer) 970924.873 124 (T. Kinnunen) 970924.876 122 (B. H. Granslo) 970924.906 12.01C (Haagaar Observatory team) 970924.909 11.97C (Haagaar Observatory team) 970924.912 12.04C (Haagaar Observatory team) 970924.916 12.03C (Haagaar Observatory team) 970924.919 12.01C (Haagaar Observatory team) 970924.923 12.00C (Haagaar Observatory team) 970924.927 12.06C (Haagaar Observatory team) 970924.930 12.08C (Haagaar Observatory team) 970924.931 12.08C (Haagaar Observatory team) 970924.933 12.16C (Haagaar Observatory team) 970924.934 12.22C (Haagaar Observatory team) 970924.935 12.29C (Haagaar Observatory team) 970924.937 12.36C (Haagaar Observatory team) 970924.938 12.41C (Haagaar Observatory team) 970924.940 12.51C (Haagaar Observatory team) 970924.940 127 (B. H. Granslo) 970924.941 12.56C (Haagaar Observatory team) 970924.942 130 (B. H. Granslo) 970924.942 12.63C (Haagaar Observatory team) 970924.944 12.75C (Haagaar Observatory team) 970924.944 133 (B. H. Granslo) 970924.945 12.92C (Haagaar Observatory team) 970924.947 13.14C (Haagaar Observatory team) 970924.948 13.30C (Haagaar Observatory team) 970924.948 139 (B. H. Granslo) 970924.949 141 (B. H. Granslo) 970924.949 13.36C (Haagaar Observatory team) 970924.951 13.41C (Haagaar Observatory team) 970924.951 139 (J. Pietz) 970924.951 141 (B. H. Granslo) 970924.952 13.31C (Haagaar Observatory team) 970924.953 13.16C (Haagaar Observatory team) 970924.953 139 (B. H. Granslo) 970924.955 13.03C (Haagaar Observatory team) 970924.956 12.90C (Haagaar Observatory team) 970924.957 137 (B. H. Granslo) 970924.958 12.72C (Haagaar Observatory team) 970924.958 132 (B. H. Granslo) 970924.959 12.55C (Haagaar Observatory team) 970924.960 12.42C (Haagaar Observatory team) 970924.962 12.26C (Haagaar Observatory team) 970924.962 129 (B. H. Granslo) 970924.963 12.11C (Haagaar Observatory team) 970924.965 12.07C (Haagaar Observatory team) 970924.966 12.08C (Haagaar Observatory team) 970924.967 12.10C (Haagaar Observatory team) 970924.967 125 (B. H. Granslo) 970924.969 12.09C (Haagaar Observatory team) 970924.970 12.03C (Haagaar Observatory team) 970924.973 123 (B. H. Granslo) 970924.982 123 (A. Diepvens) 970925.107 135 (A. Diepvens) 970925.112 138 (B. H. Granslo) 970925.116 132 (B. H. Granslo) 970925.119 128 (B. H. Granslo) 970925.125 126 (B. H. Granslo) 970925.434 125 (R. Stubbings) 970925.442 123 (R. Stubbings) 970925.792 123 (A. Diepvens) 970925.819 123 (T. Kinnunen) 970925.873 124 (E. Broens) 970925.887 125 (E. Broens) 970925.892 127 (E. Broens) 970925.894 127 (E. Broens) 970925.894 129 (E. Broens) 970925.897 130 (E. Broens) 970925.899 131 (E. Broens) 970925.900 139 (J. Pietz) 970925.901 133 (E. Broens) 970925.901 133 (E. Broens) 970925.905 132 (E. Broens) 970925.907 129 (E. Broens) 970925.908 128 (E. Broens) 970925.910 123 (A. Diepvens) 970925.910 126 (E. Broens) 970925.912 125 (E. Broens) 970925.914 124 (E. Broens) 970925.915 124 (E. Broens) 970926.842 130 (E. Broens) 970926.844 130 (E. Broens) 970926.846 133 (E. Broens) 970926.847 134 (E. Broens) 970926.848 136 (E. Broens) 970926.850 139 (E. Broens) 970926.851 138 (E. Broens) 970926.853 136 (E. Broens) 970926.853 134 (E. Broens) 970926.856 133 (E. Broens) 970926.857 131 (E. Broens) 970926.858 128 (E. Broens) 970926.860 126 (E. Broens) 970926.863 126 (E. Broens) The brightness outside eclipses seems to be fading linearly. Will anyone try to detect superhumps? Although this star is nominally classified as an SS Cyg-type dwarf nova, it is still to be tested whether long outbursts of some short orbital-period SS Cyg stars bear characteristics of superoutbursts. Some claims have been made regarding possible hump-like structure and disk asymmetry during long outbursts of IP Peg. Regards, Taichi Kato