An Orphan No Longer? Detection of the Southern Orphan Stream and a
  Candidate Progenitor
  Using a shallow, two-color survey carried out with the Dark Energy Camera, we
detect the southern, possibly trailing arm of the Orphan Stream. The stream is
reliably detected to a declination of $-38^\circ$, bringing the total known
length of the Orphan stream to $108^\circ$. We find a slight offset or "S"
shape in the stream at $\delta \simeq -14^\circ$ that would be consistent with
the transition from leading to trailing arms. This coincides with a moderate
concentration of $137 \pm 25$ stars (to $g = 21.6$) that we consider a possible
remnant of the Orphan progenitor. The position of this feature is in agreement
with previous predictions.
