“…As noted elsewhere (e.g., Brahe 1602, p. 341;Thoren 1990;Green 2004), even when a straight-edged instrument is securely fixed (i.e., not handheld), such alignments are fraught with problems due to parallax inherent by the eye moving along the edge connecting the celestial objects and due to the constant diurnal motion of the sky. The only hope to get some reasonable convergence to the true location of the unknown object (V843 Oph, in this case) is to have as many different alignments as possible to look for a mean position.…”