Using Kepler Candidates to Examine the Properties of Habitable Zone Exoplanets
Arthur D. Adams, Stephen R. Kane

TL;DR
This study compares properties of habitable zone exoplanets with the overall Kepler exoplanet sample, analyzing distributions of planetary and stellar characteristics to understand their similarities and differences.
Contribution
It provides a comparative analysis of habitable zone exoplanets versus all Kepler planets, highlighting potential differences in size and host star properties.
Findings
Potential size distribution differences in HZ planets
No significant differences in stellar mass, temperature, or metallicity
Analysis accounts for detection biases and false positives
Abstract
An analysis of the currently known exoplanets in the habitable zones (HZs) of their host stars is of interest in both the wake of the NASA Kepler mission and with prospects for expanding the known planet population through future ground- and space-based projects. In this paper we compare the empirical distributions of the properties of stellar systems with transiting planets to those with transiting HZ planets. This comparison includes two categories: confirmed/validated transiting planet systems, and Kepler planet and candidate planet systems. These two categories allow us to present quantitative analyses on both a conservative dataset of known planets and a more optimistic and numerous sample of Kepler candidates. Both are subject to similar instrumental and detection biases, and vetted against false positive detections. We examine whether the HZ distributions vary from the overall…
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