University of Hertfordshire

By the same authors

An improved quantification of HD 147379 b

Research output: Contribution to journalArticlepeer-review


  • 1801.10541v1

    Accepted author manuscript, 501 KB, PDF document


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Original languageEnglish
Article number23
JournalResearch Notes of the American Astronomical Society
Publication statusPublished - 5 Feb 2018


We reanalyze the CARMENES and HIRES/KECK radial velocity data for HD 147379, and also analyze the SOPHIE data using the Agatha software in combination with MCMC posterior sampling. The analysis confirms the existence of HD 147379 b and improves the parameter estimation through modeling of red noise. The multiple radial velocity data sets for HD147379 provide a benchmark case for RV data analyses. Based on our analysis of the HD 147379 data, CARMENES radial velocity data is dominated by red noise and thus need to incorporate a red noise model.


© 2018 The American Astronomical Society. This is an author-created, un-copyedited version of an article accepted for publication in Research Notes of the American Astronomical Society. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The definitive publisher authenticated version is available online at

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