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20 Friday, May 14, 1909 Plot 7 Sept. 30, 1919 Standard Sequences at +86° ^[[Copied Bk 53:46]] [[left margin]]3.50 Scale M[[/left margin]] Scale Measure on Plate I35319 Several Exp. at Diff. Declinations [[table]] |No | Polar Sequence | Diff.| 8 b^[[1]] | 3.7[[v.f.?]]^[[3.92]] 3.9 | 4.33 9 b^[[2]] | [[strikethrough]]3.9[[/strikethrough]]^[[5.0]][[v.f.?]]^[[5.2]] 5.4 5.30 11 | 3.53 10 c^[[1]] | 4.8 5.0 5.5 5.25 23 | 3.77 11 c^[[2]] | [[strikethrough]]4[[/strikethrough]]^[[5]].9 6.1 6.0 6.05 10 | 3.50 12 c^[[3]] | 6.7 6.9 6.7 6.80 11 | 3.06 13 d | 6.9 7.1 7.2 7.15 12 | 3.15 7r e | 7.7 | . | 8r f^[[1]] | 8.0 | . | 17 f^[[2]] | 8.5 | 3.13 18 f^[[3]] | 8.8 | 3.26 19 g | 8.9 | 3.52 20 h | 9.4 | 3.33 11r i | 9.8 [[equation]] | . | 23 k^[[1]] | 10.1 | 3.24 12r k^[[2]] | . | | 25 k^[[3]] | . | | 8s k^[[4]] | . | | 26 k^[[5]] | . | | 9s l | . | | [[4 column table]] | | Sequence 33 | curve | magn. d | 4.9 [[f.?]]^[[1]][[strikethrough]]4.7[[/strikethrough]]^[[5.1]] 5.2^[[2]] [[strikethrough]]4.8[[/strikethrough]] 3 5.15 10 | 3.75 | 8.90 e | 5.8 [[f.?]]^[[6.0]] 5.7 5.85 21 | 3.45 | 9.30 f | 6.5 6.7 6.5 6.60 11 | 3.20 | 9.80 g | 6.8 7.0 6.9 6.95 01 | 3.12 | 10.07 h | 7.0 7.2 7.7 7.45 23 | 3.10 | 10.55 k | 7.9 | 3.13 | 11.03 k^[[1]] | 8.5 | 3.18 | 11.68 l | 8.0 | 3.14 | 11.14 l^[[1]] | [[strikethrough]]7[[/strikethrough]]^[[8]].8 assume error | [[strikethrough]]3.12[[/strikethrough]]^[[3.22]] | [[strikethrough]]10.92[[/strikethrough]]^12.02 m | 9.0 | 3.25 | 12.25 n | 9.1 | 3.27 | 12.37 o | 9.3 | 3.30 | 12.60 p | 9.8 | [[equation]]3.37 | [[underlined]]13.17[[/underlined]] q | 9.9 | 3.38 | [[underlined]]13.28[[/underlined]] r | | | s | | | c | 3.9^[[4.1]] 4.4 ^12 | 4.17 | 8.42 Measures difficult 4.0 H. I. S. [[/page]] [[page]] 21 Friday, May 14, 1909 Standard Sequence at +86° Seq. 24 AC 9480 Est. [[table]] g|9.5|9.8|9.65 12| h|10.0?|10.0|10.00 00| k|9.7|10.0|9.85? 12| l|10.0? too ft.| | | Remeasured because these faint stars were not included in first set of estimates. Im. of K is probably defection. Very different from thus. Certainly bright than h on AC9480. All these stars have such faint images that there is much uncertainty in estimating. AC9503 too diff. I35634 I35514 k 10.2 10.1 s 13.4 13.5 o 12.0 11.8 marked up to p. reversed On both the above plates, the two sequences (polar and seq. 24) are about a design apart, and the strange thing is not that the above stars gave very large [[resistant?]], but that most of the estimates were as accordant as they were.
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