On the Feasibility of Intense Radial Velocity Surveys for Earth-twin Discoveries
Richard D. Hall, Samantha J. Thompson, Will Handley, Didier Queloz

TL;DR
This paper evaluates the potential of next-generation high-precision Radial Velocity instruments, specifically the Terra Hunting Experiment with HARPS3, to detect Earth-twin exoplanets amidst stellar noise and observational challenges.
Contribution
It presents an end-to-end simulation framework demonstrating the feasibility and advantages of intense RV surveys for Earth-twin detection, comparing ground-based and space-based observation schedules.
Findings
Terra Hunting can detect Earth-twins in habitable zones.
It outperforms typical surveys in parameter accuracy.
It performs comparably to space-based schedules.
Abstract
This work assesses the potential capability of the next generation of high-precision Radial Velocity (RV) instruments for Earth-twin exoplanet detection. From the perspective of the importance of data sampling, the Terra Hunting Experiment aims to do this through an intense series of nightly RV observations over a long baseline on a carefully selected target list, via the brand-new instrument HARPS3. This paper describes an end-to-end simulation of generating and processing such data to help us better understand the impact of uncharacterised stellar noise in the recovery of Earth-mass planets with orbital periods of the order of many months. We consider full Keplerian systems, realistic simulated stellar noise, instrument white noise, and location-specific weather patterns for our observation schedules. We use Bayesian statistics to assess various planetary models fitted to the…
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