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essarily occupied in cutting a roadway through the forest from a convenient point on the Calais road to the monument at the source of the river St. Croix, a series of astronomical observations was made, both by day and by night, by which the latitude and longitude of Houlton were satisfactorily determined and the rates of the chronometers further tested. By the 24th of September the roadway was sufficiently opened to permit a camp to be established upon the experimental line traced by the United States and British surveyors in the year 1817, when an attempt was made to mark this portion of the boundary between the two countries agreeably to the provisions of the treaty of Ghent of 1815. The provisions and camp equipage were transported upon a strong but roughly constructed sled, drawn by horses, whilst the instruments were carried by hand, the surface of the country over which this roadway was opened being too rough for any wheeled vehicle to pass. The point decided upon as the true source of the river St. Croix by the United States and British commissioners appointed for that purpose under the fifth article of the treaty of 1794 was found and identified, both by the inscriptions upon the monument erected there to mark the spot and also by the testimony of a living witness of high respectability, who has known the locality since it was first designated by the commissioners under the treaty of 1794. The avenue which had been cleared through a dense forest from the monument to a distance of 12 miles north of it by the surveyors in 1817 was easily recognized by the new and thick growth of young timber, which, having a width of from 40 to 50 feet, now occupied it. Axmen were at once set at work to reopen this avenue, under the supposition that the due north line would at least fall within its borders for a distance of 12 miles. In the meantime the first astronomical station and camp were established, and the transit instrument set up at a distance of 4,578 feet north of the monument, upon an eminence 45-1/2 feet above the level of its base. This position commanded a distinct view of the monument to the south, and of the whole line to the north for a distance of 11 miles, reaching to Parks Hill. Whilst the work of clearing the line of its young growth of timber was progressing a series of astronomical observations was commenced at this first camp, and continued both day and night without intermission (except when int
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