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[[preprinted]] 94 [[/preprinted]]

Reduced June 22, 1915 G.F.M.
December 10, 1895  T Cass.

Plate C 7974 July 11, 1895
f-v dist. too great to estimate
^[[9.27]] 8.55 v1g ^[[9.37]] 8.65  v = 8.55? ^[[9.27?]]

Plate C 8019 taken July 23, 1895
f-v dist. too great to estimate
^[[8.97]] 8.25 v4g ^[[9.37]] 8.65 v = 8.25? ^[[v = 8.97?]]

Plate C 8020 taken July 23, 1895
[[margin]] images elongated [[/margin]]
f-v dist. too great
^[[8.97]] 8.25 v4g ^[[9.37]] 8.65 ^[[v = 8.97?]] v = 8.25?

Plate C 8070 taken July 31, 1895
f-v dist. too great
^[[9.07]] 8.35 v3g ^[[9.37]] 8.65 ^[[v = 9.07?]] v = 8.35

Plate C 8084 taken Aug. 2, 1895
f-v dist. too great
^[[8.97]] 8.25 v4g ^[[9.37]] 8.65 ^[[v = 8.97?]] v = 8.25?

Plate C 8192 taken Aug. 30, 1895
f-v dist. too great
^[[9.27]] 8.55 v1g ^[[9.37]] 8.65 ^[[v = 9.27?]] v = 8.55?

Plate I 13380 taken Sept. 2, 1895
useless

Plate C 8257 taken Sept. 5, 1895
v0g ^[[9.37]] 8.65  v = 9.37

Plate C 8225 taken Sept. 3, 1895
v0g ^[[9.37]] 8.65  v = 9.37

Plate C 8281 taken Sept. 15, 1895
^[[9.37]] 8.65 g1v ^[[9.47]] 8.75 ^[[9.92]] 8.82 = 8. [[strikethrough]] 8 [[/strikethrough]] 78  .03  .04
^[[9.82]] 8.82 v4g' ^[[10.22]] 9.22  v = 9.70  23 22
Continued page 156

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[[preprinted]] 95 [[/preprinted]]

[[underline]] December 10, 1895 [[/underline]]

Measures of the photographic brightness of O.C. Wendell's comparison stars to R Cassiopeiae

For n' and o' see chart p. 113
Plate B 1975

e|2.7|3.0 image much elongated
f|4.6|4.9
g|4.3|4.6  Stars a,b,c,d,e appear on only a few plates. They vary in distance from the variable from 5 [[superscript]] o [[/superscript]] to 7 [[superscript]] o [[/superscript]]
h|3.6|3.9
k|4.9|5.2
l|5.4|5.7
m|[[strikethrough]] 4 [[/strikethrough]] 5.1|[[strikethrough]] 4 [[/strikethrough]] 5.4
n|5.0|5.3
o|6.7|7.0
p|   |8.1
q|6.7|7.0
r|   |7.8? so near R that measurement is difficult
s|   |7.9? image very poor
t|   |8.8? image poor
u|   |8.8   image poor
w|   |9.2   image poor
x|   |10.0? image poor
y|   |just seen
z|   |just seen
alpha|   |n.s.
v|6.4|6.7
n'|5.7|6.0
o'|6.1|6.4
Some images much nearer edge of plate than others.

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