The Exoplanet Orbit Database II: Updates to exoplanets.org

Abstract

The Exoplanet Orbit Database (EOD) compiles orbital, transit, host star, and other parameters of robustly detected exoplanets reported in the peer-reviewed literature. The EOD can be navigated through the Exoplanet Data Explorer (EDE) Plotter and Table, available on the World Wide Web at exoplanets.org. The EOD contains data for 1492 confirmed exoplanets as of July 2014. The EOD descends from a table in Butler et al. (2002) and the Catalog of Nearby Exoplanets (Butler et al. 2006), and the first complete documentation for the EOD and the EDE was presented in Wright et al. (2011). In this work, we describe our work since then. We have expanded the scope of the EOD to include secondary eclipse parameters, asymmetric uncertainties, and expanded the EDE to include the sample of over 3000 Kepler Objects of Interest (KOIs), and other real planets without good orbital parameters (such as many of those detected by microlensing and imaging). Users can download the latest version of the entire EOD as a single comma separated value file from the front page of exoplanets.org.

PASP in press, Issue No. 943, September 2014, ahead-of-print published version available at http://www.jstor.org/stable/10.1086/678447; 20 pages, 3 figures

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Cited by in corpus (191)

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• The K2-HERMES Survey. I. Planet Candidate Properties from K2 Campaigns 1-3
• Long-Period Giant Companions to Three Compact, Multiplanet Systems
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• Moderately Eccentric Warm Jupiters from Secular Interactions with Exterior Companions
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• Possible Internal Structures and Compositions of Proxima Centauri b
• The Pan-Pacific Planet Search VII: The most eccentric planet orbiting a giant star
• Simulating the M-R Relation from APF follow up of TESS targets: Survey design and strategies for overcoming mass biases
• Determining the true mass of radial-velocity exoplanets with Gaia: 9 planet candidates in the brown-dwarf/stellar regime and 27 confirmed planets
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• The SOPHIE search for northern extrasolar planets. X. Detection and characterization of giant planets by the dozen
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• MOPSS I: Flat Optical Spectra for the Hot Jupiters WASP-4 b and WASP-52b
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