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

Independent Discovery of a Sub-Earth in the Habitable Zone Around a Very Close Solar-Mass Star