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[[preprinted]] 18 [[/preprinted]] [[underlined]] February 1, 1896 [[/underlined]] Measure of Comparison Stars to S Cassiopeiae repeated, taking account of density, as well as diameter of images. Plate I 144 taken Nov. 16, 1889 a| [[strikethrough]] 4 [[/strikethrough]]3.7| 4.0 b| 4.|4.7 c| 4.7| 5.0 e| 5.4| 5.7 f| 5.0| 5.3 g| 4.7| 5.0 image much blurred Unquestionably much lighter than f Dec. 9, 1903 h| 5.4| 5.7 k| 5.9| 6.2 l| 6.0| 6.3 m| 5.8| 6.1 n| | 7.7 o| | 6.8 p| | 7.6 q| | 7.8 r| | 7.9 [[margin]] Superseded {[[/margin]] [[bracket encapsulating s to v entries]] s| | 8.1 t| | 9.7 u| | 9.3 w| | 9.7 [[strikethrough]] y [[/strikethrough]] x| Hidden in trail of v v| | 6.5 y|| | 10.4? [[margin]] Meas. May 6, '96 [[/margin]] d| 5.4| 5.7 h| 6.2| 6.6 a| 4.3 Long trails - Images rather blurred [[end page]] [[start page]] [[preprinted]] 19 [[/preprinted]] Feb. 1, 1896 Plate I 3309 taken March 25, 1891 a| 4.9| 5.1 This plate Not used in Reduction of Magnitudes b| 5.3| 5.6 c| 5.2| 5.5 [[strikethrough]] d [[/strikethrough]] e| 6.1| 6.4 image much elongated f |5.9 |6.1 image much elongated g|5.8 |6.1 h| | 7.6 image much blurred and elongated k| | 7.9 l| | 8.3 m| | 8.0 n| | 9.1 o| | 8.7 p| | 9.2 q| | 9.4 r| | 9.6 s| | 9.8 t| |n.s. u| | n.s. w| |n.s. v| |n.s. [[strikethrough]] Meas. May 6, '96 d [[/strikethrough]] [[end page]]