DY Per fading? The R CrB-type star DY Per is reported slightly fainter. Observations are encouraged to monitor whether this leads to a deep fading episode. YYYYMMDD(UT) mag observer 20011107.585 109 (Hitoshi Nakatani) 20011108.869 113 (Eddy Muyllaert) 20011108.931 111 (Hazel McGee) 20011108.981 113 (A. Sonka) 20011109.747 109 (Georg Comello) 20011109.769 109 (Reinder J. Bouma) 20011109.858 113 (Eddy Muyllaert) 20011109.876 108 (Gary Poyner) 20011110.812 113 (Eddy Muyllaert) 20011110.828 109 (Maciej Reszelski) 20011111.551 112 (Hitoshi Nakatani) 20011112.076 110 (Mike Simonsen) 20011113.742 108 (Maciej Reszelski) 20011113.933 107 (Gary Poyner) 20011114.783 108 (Maciej Reszelski) 20011114.899 112 (Eddy Muyllaert) 20011114.960 107 (Gary Poyner) 20011115.853 112 (Eddy Muyllaert) 20011117.076 108 (Maciej Reszelski) 20011117.092 110 (Mike Simonsen) 20011118.699 112 (Hitoshi Nakatani) 20011118.760 114 (A. Sonka) 20011119.599 111 (Hitoshi Nakatani) 20011119.812 108 (Maciej Reszelski) 20011121.551 109 (Hitoshi Nakatani) 20011121.933 110 (Mike Simonsen) 20011122.865 112 (Eddy Muyllaert) 20011122.873 107 (Gary Poyner) 20011123.632 113 (Hitoshi Itoh) 20011123.637 112 (Mamoru Ooishi) 20011124.547 109 (Hitoshi Nakatani) 20011126.874 108 (Gary Poyner) 20011126.910 112 (Georg Comello) 20011201.769 115 (Eddy Muyllaert) 20011201.919 108 (Gary Poyner) 20011201.990 112 (Georg Comello) 20011204.919 116 (Eddy Muyllaert)