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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 13

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II. Focus the objective by directing the telescope to some distant well defined terrestrial object (not less than a mile away) and placing the [wires?] in the principal focus of the objective by sliding the [tick?] carrying the [wires?] and eye piece, in the main tube until an image of the object seen on one of the [wires?] will remain on the [wire?] when the position of the eye is changed . The object of the adjustment viz, to bring the image formed by the objective into coincidence with the [wires?], is then accomplished. If the eye piece has been properly focused, this position of the objective will also be the position of most distinct [vision?] for both the [wires?] and image The adjustments I and II are to be made by daylight, but at night the focus of the objective will need to be corrected [?] a star as the object (Unless the focus is made [nearly?] night by daylight none but the brightest star will be seen at all at night.
 
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