  The recently postulated existence of a giant ninth planet in our solar system
has sparked search efforts for distant solar system objects (SSOs) both via new
observations and archival data analysis. Due to the likely faintness of the
object in the optical and infrared regime, it has so far eluded detection. We
set out to re-analyze data acquired by the Wide-Field Infrared Survey Explorer
(WISE), an all-sky survey well suited for the detection of SSOs. We present a
new approach to SSO detection via parallactic fitting. Using the heliocentric
distance as a fit parameter, our code transforms groups of three or more single
observation point sources to heliocentric coordinates under the assumption that
all data stem from an object. The fact that the orbit of a distant SSO is
approximately linear in heliocentric coordinates over long time-scales can be
utilized to produce candidates, which can then be confirmed with follow-up
observations. We demonstrate the feasibility of the approach by a posteriori
detecting the outer SSO Makemake within WISE data. An all-sky search for Planet
Nine yielded no detection. While the postulated Planet Nine eluded detection by
our algorithm, we tentatively predict that this new approach to moving-object
analysis will enable the discovery of new distant SSOs that cannot be
discovered by other algorithms. Especially in cases of sparse data observed
over long time spans, our approach is unique and robust due to the use of only
one fit parameter.
