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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