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

[[underline]] Superseded [[/underline]] see p. 79

[[underline]]November 4, 1895[[/underline]]

Estimate of brightness of T Cassiopeiae
a^5 b^5 c^0 e^6 d^0 f^7 h^3 g^5 k^2 m^0 n^3 l (double on C plates)
Comparison stars of O.C. Wendell arranged in order of photographic magnitude -

Plate B65 taken Oct. 16, 1885
[[margin]] Edge of plate [[/margin]]
V0g [[strikethrough]] 8.65 [[/strikethrough]]8.86

Plate 75 taken Oct. 24, 1885
[[margin]] Edge of plate [[/margin]]
[[strikethrough]] 8.65 [[/strikethrough]] 8.86 g4v [[strikethrough]] 9.05 [[/strikethrough]] 9.26 [[strikethrough]] 9.44 [[/strikethrough]] 9.65 = [[strikethrough]] 9.24 .19 .20 [[/strikethrough]] 9.46  .20
[[strikethrough]] 9.50 [[/strikethrough]] 9.65 v1k [[strikethrough]] 9.64 [[/strikethrough]] 9.75

Plate B 1975 taken Dec. 1, 1887
[[margin]] Edge of plate [[/margin]]
[[strikethrough]] 8.65 [[/strikethrough]] 8.86 g4v [[strikethrough]] 9.05 [[/strikethrough]] 9.26 [[strikethrough]] 9.26 [[/strikethrough]] 9.36 = [[strikethrough]] 9.16 [[/strikethrough]] 9.31 [[strikethrough]] .11 [[/strikethrough]] .05 [[strikethrough]] .10 [[/strikethrough]] .05

Plate B 2690 taken June 8, 1888
[[margin]] Edge of plate  magnitude not in order found in others [[/margin]]
[[strikethrough]] 8.66 [[/strikethrough]] 8.85 h4v [[strikethrough]] 9.06 [[/strikethrough]] 9.23 [[strikethrough]] 9.46 [[/strikethrough]] 9.56 = [[strikethrough]] 9.26 [[/strikethrough]] 9.40 [[strikethrough]] .20 [[/strikethrough]] .17 [[strikethrough]] .20 [[/strikethrough]] .16

Plate B 2707 taken June 12, 1888
[[strikethrough]] 8.66 [[/strikethrough]] 8.83 h1v [[strikethrough]] 8.76 [[/strikethrough]] 8.93 [[strikethrough]] 8.55 [[/strikethrough]] 8.76 = [[strikethrough]] 8.66 [[/strikethrough]] 8.85 [[strikethrough]] .10 [[/strikethrough]] .08 [[strikethrough]] .09 .11 [[/strikethrough]] .09 [[strikethrough]] 8.55 [[/strikethrough]] 8.76 v1g [[strikethrough]] 8.65 [[/strikethrough]] 8.86

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

November 5, 1895

[[strikethrough]]
a b e f h g g' n l' o
Here I have substituted l' for l, because l is double on the C plates. g' has been substituted for k and m, because it divides the interval more evenly. o & p added because there are no companion stars given faint enough.
Plat I 81 taken Nov. 5, 18 [[strikethrough]] 9 [[/strikethrough]] 89
o2v
v3p
Plate I 423 taken Jan. 3, 1890.
Edge of plate region not distinct enough for measurement.
Plate I 424 taken Jan. 3, 1890
[[/strikethrough]]

Obtained a chart from Professor Wendell for faint comparison stars. see next page.

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