  With the wealth of planets that have been discovered over the past $\sim$ 20
years, the field can broadly be divided into two regimes. For understanding
broad occurrence and formation rates, large numbers of planets allow for
population statistics to be calculated, and this work preferentially tends
towards fainter planets (and fainter host stars) to allow for a large number of
detections. The second regime is the detailed understanding of a single planet,
with particular consideration to planetary structure and atmosphere, and in
this case benefits from finding individual planets (and host stars) that are
very close, and subsequently, very bright. The closest of these also provide
very novel possibilities for exploration if they are close enough that travel
time to them is relatively low, something that would be extremely unlikely for
more distant planets. Here, we announce the independent discovery of a
sub-earth planet orbiting in the habitable zone of a very close solar-mass star
using a novel processing technique and observations from the Kilodegree
Extremely Little Telescope (KELT).
