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[[preprinted]] 70 [[/preprinted]]

October 4, 1904

15° 4905 continued

Plate B 11363  continued

After the exposure which formed the image described above as toward the preceding side of the plate, the spectrum trailed again, the trail being much fainter and for this region, being interrupted by the edge of the plate.  For the brighter stars more favorably placed the trail appears to have no well defined end, and is much fainter than between the earlier exposures.  The images measured at the preceding side of the plate were, therefore, probably formed some time after the middle time of the complete exposure of 175 minutes. The last exposure, that toward the preceding edge, appears to be the longest, as the images are brighter.

The exposure was from S.J. 18h 40 to 21h 35m
Assumed twice of the middle of the separate exposures:-

Following edge | 19h | 10 | S.M.J | 19 |10
Middle | 20 | 0 |   | 20 | 0
Preceding edge | 20 | 50 |   | 20 | 50

Omit from table, but make remark to follow the ledger

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[[preprinted]] 71 [[/preprinted]]

October 4, 1904  

15° 4905
Re-examination of certain Plates

[[check mark]] B9277 see p. 51
9.[[strikethrough]] 94 [[/strikethrough]]89 d4 gamma 10.[[strikethrough]] 34 [[/strikethrough]]29 10.[[/strikethrough]] 34 [[/strikethrough]]29 10.[[/strikethrough]] 34 [[/strikethrough]]29 00 00
10.[[striketrhrough]] 34 [[strikethrough]]29 v2e 10.[[strikethrough]] 54 [[strikethrough]]49
Edge of plate

B9278 see p.51
9.[[strikethrough]]94[[strikethrough]]89 d6 gamma ? 10.[[strikethrough]] 54 [[strikethrough]]49 ? 00 00
gamma 0e 10.[[strikethrough]] 54 [[strikethrough]]49
Image of f too poor
Edge of plate. Images poor
Comparison of the above two plates makes
evident the uncertainty of these estimates, as the stars of the region are much affected
by their distances to the edge of the plate

AC [[strikethrough]] 856 [[strikethtough]] 4955 [[strikethrough]] May 11, 1900 [[strikethtough]] June 11, 1904
10[[strikethrough]] 54 [[strikethrough]]49 e 2 v 10.[[strikethrough]] 74 [[strikethrough]]69 10.[[strikethrough]] 72 [[strikethrough]]67 10.[[strikethrough]] 73 [[strikethrough]]68 01 [[underlined]] 01 [[/underlined]]
10.[[strikethrough]] 72 [[strikethrough]]67 v 1 f 10.[[strikethrough]] 82 [[strikethrough]]77
Images very faint and poor. Observation uncertain
AC 858
Variable certainly faint. Images too poor
for accurate measurement

9.[[strikethrough]]94 d0e 10 [[strikethrough]]54[[strikethrough]]49[[strikethrough]]
9.[[strikethrough]]94[[strikethrough]]89 d2v 10.[[strikethrough]]14[[strikethrough]]09 [[Bracket with line below]]
10.[[strikethrough]]54[[strikethrough]]49 e2v 10.[[strikethrough]]74[[strikethrough]]69 [[Bracket with line above]] 10.[[strikethrough]]8[[strikethrough]]72 [[strikethrough]] 10.5[[strikethrough]]7[[strikethrough]]0 43[1[[strikethrough]]4[[strikethrough]]7 2.5[strikethrough]]^[[strikethrough]] [[underlined]]41[[/underlined]] 19 22[[strikethrough]] 10.48  [[underlined]] 39 [[/underlined]]21, 19
Image of [[v]] [[especially]] from 
May 3, 1907 Where did obs. d2v come from? [[?]], and take mean of other 2 obs. [[symbol - equals]] 10.73 Res.  [[underlined]]04[[/underlined]], 04

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