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NEID is a high-resolution optical spectrograph on the WIYN 3.5-m telescope atKitt Peak National Observatory and will soon join the new generation of extremeprecision radial velocity instruments in operation around the world. We plan touse the instrument to conduct the NEID Earth Twin Survey (NETS) over the courseof the next 5 years, collecting hundreds of observations of some of the nearestand brightest stars in an effort to probe the regime of Earth-mass exoplanets.Even if we take advantage of the extreme instrumental precision conferred byNEID, it will remain difficult to disentangle the weak (~10 cm s$^{-1}$)signals induced by such low-mass, long-period exoplanets from stellar noise forall but the quietest host stars. In this work, we present a set of quantitativeselection metrics which we use to identify an initial NETS target listconsisting of stars conducive to the detection of exoplanets in the regime ofinterest. We also outline a set of observing strategies with which we aim tomitigate uncertainty contributions from intrinsic stellar variability and othersources of noise.

Target Prioritization and Observing Strategies for the NEID Earth Twin Survey