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[[preprinted]]30[[/preprinted]]

[[underline]]February[[/underline]] 4, [[underline]]1896[[/underline]]

Continuation of estimates of S Cephei from previous volume p. 153

Plate C8648 taken Dec. 20, 1895
V n.s.   v < 11.00
10.80[[/ink]] m ns = .2

Plate C 8669 taken Dec. 22, 1895
V n.s.   [[ink]] v < 11.94
11.64[[/ink]] V = .3
^[[margin]] April 2,1896 [[/margin]]

Plate C 8796 taken Jan. 30, 1896
V n.s.   [[ink]]v < 11.74
11.64[[/ink]] V=.1
[[margin note]]April 2, 1896 [[/margin note]]

Plate C8869 taken Feb. 20, 1896
v n.s.   [[ink]]v < 11.00
10.80[[/ink]] n=.2
[[margin note]]April 2, 1896 [[/margin note]]

Plate C8898 taken Feb. 24, 1896
V n.s.   [[ink]]v < 11.26
10.96[[/ink]] n=.3

Plate C8899 taken Feb. 24, 1896
V n.s.   [[ink]]v < 11.26
10.96[[/ink]] n=.3
Plate I 14409 taken Jan. 30, 1896
v op'? 

Any doubtful observation.  What I have taken for V may be a defect in the plate

Plate I 14738 taken March 27, 1896
V n.s.
V=.2     Continued III p 135

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[[preprinted]]31[[/preprinted]]

[[underline]]Feb.[[/underline]] 5 , 1896.

Annie J. Cannon  obs.
Estimates of the brightness of comparison stars
to S Cygni

Plate I 141, Taken Nov. 16. 1889.
a | 4.7
b | 5.5
c | 5.4
d | [[strikethrough]]4[[/strikethrough]]5.6
e | 5.4
f | 6.1
g | 5.4
h | 7.2
k | 6.6
l | 6.9
m | 7.2
n | 7.9
o | 7.3
p | 7.8
q | 8.2
r | 8.4
s | 8.5
t | 8.9 Image blurred.
Ft. star | 8.2 

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