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[[start page]] [[preprinted]] 94 [[/preprinted]] Reduced June 22, 1915 G.F.M. December 10, 1895 T Cass. Plate C 7974 July 11, 1895 f-v dist. too great to estimate ^[[9.27]] 8.55 v1g ^[[9.37]] 8.65 v = 8.55? ^[[9.27?]] Plate C 8019 taken July 23, 1895 f-v dist. too great to estimate ^[[8.97]] 8.25 v4g ^[[9.37]] 8.65 v = 8.25? ^[[v = 8.97?]] Plate C 8020 taken July 23, 1895 [[margin]] images elongated [[/margin]] f-v dist. too great ^[[8.97]] 8.25 v4g ^[[9.37]] 8.65 ^[[v = 8.97?]] v = 8.25? Plate C 8070 taken July 31, 1895 f-v dist. too great ^[[9.07]] 8.35 v3g ^[[9.37]] 8.65 ^[[v = 9.07?]] v = 8.35 Plate C 8084 taken Aug. 2, 1895 f-v dist. too great ^[[8.97]] 8.25 v4g ^[[9.37]] 8.65 ^[[v = 8.97?]] v = 8.25? Plate C 8192 taken Aug. 30, 1895 f-v dist. too great ^[[9.27]] 8.55 v1g ^[[9.37]] 8.65 ^[[v = 9.27?]] v = 8.55? Plate I 13380 taken Sept. 2, 1895 useless Plate C 8257 taken Sept. 5, 1895 v0g ^[[9.37]] 8.65 v = 9.37 Plate C 8225 taken Sept. 3, 1895 v0g ^[[9.37]] 8.65 v = 9.37 Plate C 8281 taken Sept. 15, 1895 ^[[9.37]] 8.65 g1v ^[[9.47]] 8.75 ^[[9.92]] 8.82 = 8. [[strikethrough]] 8 [[/strikethrough]] 78 .03 .04 ^[[9.82]] 8.82 v4g' ^[[10.22]] 9.22 v = 9.70 23 22 Continued page 156 [[end page]] [[start page]] [[preprinted]] 95 [[/preprinted]] [[underline]] December 10, 1895 [[/underline]] Measures of the photographic brightness of O.C. Wendell's comparison stars to R Cassiopeiae For n' and o' see chart p. 113 Plate B 1975 e|2.7|3.0 image much elongated f|4.6|4.9 g|4.3|4.6 Stars a,b,c,d,e appear on only a few plates. They vary in distance from the variable from 5 [[superscript]] o [[/superscript]] to 7 [[superscript]] o [[/superscript]] h|3.6|3.9 k|4.9|5.2 l|5.4|5.7 m|[[strikethrough]] 4 [[/strikethrough]] 5.1|[[strikethrough]] 4 [[/strikethrough]] 5.4 n|5.0|5.3 o|6.7|7.0 p| |8.1 q|6.7|7.0 r| |7.8? so near R that measurement is difficult s| |7.9? image very poor t| |8.8? image poor u| |8.8 image poor w| |9.2 image poor x| |10.0? image poor y| |just seen z| |just seen alpha| |n.s. v|6.4|6.7 n'|5.7|6.0 o'|6.1|6.4 Some images much nearer edge of plate than others. [[end page]]