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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[[margin]] Superseded {[[/margin]] [[bracket encapsulating s to v entries]]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

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[[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]]

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