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121

May 8, 1906

[[4 columned table]]
|AM 3695|July 7, 1905|Ex. 512^[[m]]|Est.|
|---|---|---|---|
|Image No 5|7034.583|13^[[h^[[W.M.T.]]]] 59^[[m]]|10.0 10.0|
|6|7034.603|14 29|10.0 10.0|
|7|7034.624|14 59|9.8 9.9|
|8|7034.645|15 29|[[strikethrough]]8.9[[/strikethrough]] 9.[[go to notes]] 9.5|
|9|7034.666|15 59|[[strikethrough]]8.9[[/strikethrough]] 9.[[go to notes]] 9.0|
|10|7034.687|16 29|8.7 [[strikethrough]]9.1[[/strikethrough]]|
|11|7034.708|16 59|8.7|
|12|7034.728|17 29|8.7|
|13|7034.749|17 59|8.7|
|14|7034.770|18 29|8.7|
|15|7034.791|18 59|8.7|
|16|7034.812|19 29|8.7|
|17|7034.833|19 59|8.9|

On AM 1406 & 3695 the images of comparison p\m̄ g" cannot- be separatēd from the images of the van. Assuming the brightest images lō be al- max (8.7) and the faintest- 10.0 have estimated as nearly as possible_ those between.

John G. Wolbach Library, Harvard-Smithsonian Center for Astrophysics · Provided by the NASA Astrophysics Data System

Transcription Notes:
go to notes: The number is written in such a way that it can be read as either '9.3' or '9.5'