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Theory of the astronomical transit instrument applied to the portable transit instrument Wuerdemann no.26: a compilation from various authorities, with original observations by Harry Edward Burton, 1903

Theory of the astronomical transit instrument applied to the portable transit instrument Wuerdemann no. 26: a compilation from various authorities, with original observations by Harry Edward Burton, 1903, Page 95

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[table of 6 columns] Interval | Star | Time . I[subscript]8[/subscript] | lg Time | lg I[subscript]8[/subscript] cos delta | I[subscript]0[/subscript][superscript][s?][/superscript] C[subscript]3[/subscript] - D[subscript]3[/subscript] | (1) | 35[superscript][s?][/superscript] | 1.54407 | 1.49213 | 31.055 D[subscript]3[/subscript] - E[subscript]3[/subscript] | | | | | 31.055 | (2) | 36.5 | 1.56229 | 1.49636 | 31.359 | | | | | 31.359 | (3) | 31 | 1.49136 | 1.49130 | 30.996 | | 31.5 | 1.49831 | 1.49825 | 31.496 | (4) | 32 | 1.50515 | 1.49640 | 31.362 | | | | | 31.362 | (5) | 45.5 | 1.65801 | 1.49567 | 31.309 | | | | | 31.309 | (6) | 35.5 | 1.55023 | 1.49828 | 31.498 | | 35 | 1.54407 | 1.49212 | [underlined]31.054[/underlined] | | | | | [underlined][121? or 12)?] 12 x 3[superscript]0[/superscript]+ 15.214[/underlined] | | | | | [underlined]Mean 31.268[/underlined]
 
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