Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender

TL;DR
This paper reports the discovery and characterization of a super-Earth candidate in the habitable zone of the nearby star GJ 251, highlighting its potential for future direct imaging with next-generation telescopes.
Contribution
It provides improved parameters for the known planet GJ 251 b and constrains the minimum mass of the new candidate GJ 251 c using multiple high-precision RV datasets and activity mitigation techniques.
Findings
GJ 251 c is a plausible terrestrial super-Earth in the habitable zone.
GJ 251 b's parameters are refined with high-precision RV data.
GJ 251 c is a prime target for future direct imaging efforts.
Abstract
We present the discovery of GJ 251 c, a candidate super-Earth orbiting in the Habitable Zone (HZ) of its M dwarf host star. Using high-precision Habitable-zone Planet Finder (HPF) and NEID RVs, in conjunction with archival RVs from the Keck I High Resolution Echelle Spectrometer (HIRES), the Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle Spectrograph (CARMENES), and the SPectropolarim\`etre InfraROUge (SPIRou), we improve the measured parameters of the known planet, GJ 251 b ( = 14.2370 days; = 3.85 M), and we significantly constrain the minimum mass of GJ 251 c, placing it in a plausibly terrestrial regime (P = 53.647 0.044 days; = 3.84 0.75 M). Using activity mitigation techniques that leverage chromatic information content, we perform a…
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