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56 Friday, October 2 [strikethrough]7[\strikethrough]8, 1910 Sequence C1 Estimates of Orig. Nos. 3 and 9 selected as g and p by the Director and Mrs. F. AM6619 | AC11230 | B38215 Sept. 29, 1907 d^[[3]]4(3) | d^[[3]]2[[strikethrough]]9[[/strikethrough]](3) | d^[[1]]0d^[[2]] (3)1e | (3)1e | d^[[2]]7d^[[3]] e2f | e2f | d^[[3]]0(3) [[strikethrough]]K[[/strikethrough]] | | (3)3e | | e3f k6l | k5l | | l2([[strikethrough]]3[[/strikethrough]][[9]]) | l0(9) | k5l ([[strikethrough]]3[[/strikethrough]][[9]])2(m) | 94m | l2(9) | | (9)3m [[new columns]] MC599pc | A8196 Nov.14 1906 | I32017pc | d^[[2]]d^[[2]] |d^[[1]]6d^[[2]] | too ft | d^[[2]]7d^[[3]] | d^[[2]]0d^[[3]] |Reject prev. est d^[[3]]2(3) | d^[[3]]-(3) | for d^[[2]]+d^[[3] (3)3e | (3)-e | | e1f | | [[new column]]I32017 star | k-l | d^[[1]]2d^[[2]] [[new column]]MC599star [?] | l1(9) | d^[[2]]4d^[[3]] k4l | (9)0m | d^[[3]]1(3) l2(9) | | (3)le (9)2m | | | | | l3(9) | | 92m 57 Friday, October 28, 1910 Sequence C1 Examination of d^2 suspected of variability B38209 Sept. 28, 1907 | I34359 | AM5173 Sept. 27, 1907 d1d^[[1]] | d0d^[[1]] | AC 8823 Oct. 2, 1907 of nearly same date as the 3B plates show the star normal d^[[1]]0d^[[2]] | d^[[1]]1d^[[2]] | d^[[2]]8d^[[3]] | d^[[2]]5d^[[3]] | B 38214 Sept. 29, 1907 | | d1d^[[1]] | AW5258 | | d^[[1]]1d^[[2]] | d^[[1]]4d^[[2]] | AW4688 Nov. 13, 1906 d^[[2]]8d^[[3]] | d^[[2]]3d^[[3]] | Normal AC979^[[5]] |[[strikethrough]] AC3705 [[/strikethrough]] | AC8008 Nov. 13, 1906 d^[[1]]3d^[[2]] | AM3425 | Normal d^[[2]]5d^[[3]] | d^[[1]]4d^[[2]] | | | d^[[?]]3d^[[3]] | AC8031 Nov. 19, 1906 AM6697 | | Normal d^[[1]]3d^[[2]] | AM3015 | | d^[[2]]4d^[[3]] | AC4188 | | | AC2144 | | AC11264 | all the above show d62 normal d^[[1]]4d^[[2]] | d^[[2]]5d^[[3]] No evidence of variation. The extreme faintness on A 8196 is probably due to a peculiarity of the image, though of course it might indicate a variable of the Algol type. AM 6579 d^1 2 d^2 d^[[2]]5 d^[[3]] |