  This paper concludes a systematic search for evidence of the Monoceros Ring
and Canis Major dwarf galaxy around the Galactic Plane. Presented here are the
results for the Galactic longitude range of l = (280 - 025)deg. Testing the
claim that the Monoceros Ring encircles the entire Galaxy, this survey attempts
to document the position of the Monoceros Ring with increasing Galactic
longitude. Additionally, with the discovery of the purported Canis Major dwarf
galaxy, searching for more evidence of its interaction is imperative to tracing
its path through the Galaxy and understanding its role in the evolution of the
Milky Way. Two new detections of the Monoceros Ring have been found at (l, b) =
(280,+15)deg and (300,+10)deg. Interestingly, in general there seem to be more
detections above the Plane than below it; in this survey around 2/3 of the firm
Monoceros Ring detections are in the North. This coincides with the Northern
detections appearing to be qualitatively denser and broader than their Southern
counterparts. The maximum of the Galactic Warp in the South is also probed in
this survey. It is found that these fields do not resemble those in the Canis
Major region suggesting that the Warp does not change the shape of the CMD as
is witnessed around Canis Major. The origins and morphology of the Monoceros
Ring is still elusive primarily due to its enormous extent on the sky.
Continued probing of the Galactic Outer Disc is needed before a consensus can
be reached on its nature.
