The statistical reliability of 267-GHz JCMT observations of Venus: no significant evidence for phosphine absorption

@article{Thompson2020TheSR,
  title={The statistical reliability of 267-GHz JCMT observations of Venus: no significant evidence for phosphine absorption},
  author={M A Thompson},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2020}
}
  • M. Thompson
  • Published 28 October 2020
  • Physics
  • arXiv: Earth and Planetary Astrophysics
In the light of the recent announcement of the discovery of the potential biosignature phosphine in the atmosphere of Venus I present an independent reanalysis of the original JCMT data to assess the statistical reliability of the detection. Two line detection methods are explored, low order polynomial fits and higher order multiple polynomial fits. A non-parametric bootstrap analysis reveals that neither line detection method is able to recover a statistically significant detection. Similar to… 

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Villanueva G.L.1, Cordiner, M.1,2, Irwin P.G.J.3, de Pater I.4, Butler B.5, Gurwell M.6, Milam S.N.1, Nixon C. A.1, Luszcz-Cook S. H.7,8, Wilson C.F.3, Kofman V.1,9, Liuzzi G.1,9, Faggi S.1,9,
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