DY Per rising? The suspected R CrB-star DY Per may be recovering from a shallow minimum. YYMMDD(UT) mag observer 980915.619 127 (M. Hiraga) 980916.666 131 (T. Watanabe) 980916.742 132 (H. Maehara) 980919.667 130 (H. Maehara) 980919.896 128 (G. Poyner) 980920.565 <126 (M. Nakatani) 980920.597 127 (M. Hiraga) 980920.844 129 (R. J. Bouma) 980921.035 128 (G. Poyner) 980921.881 130 (E. Broens) 980921.898 131 (E. Muyllaert) 980922.826 128 (R. J. Bouma) 980922.860 129 (G. Comello) 980923.855 134 (A. Diepvens) 980924.817 129 (R. J. Bouma) 980925.705 130 (H. Maehara) 980929.812 128 (R. J. Bouma) 980930.853 130 (E. Muyllaert) 980930.860 127 (G. Poyner) 981002.751 127 (T. Watanabe) 981003.083 124 (G. Poyner) 981003.585 <126 (M. Nakatani) 981009.074 122 (G. Poyner) 981009.605 128: (M. Nakatani)