No evidence of phosphine in the atmosphere of Venus from independent analyses

@article{Villanueva2021NoEO,
  title={No evidence of phosphine in the atmosphere of Venus from independent analyses},
  author={Geronimo L. Villanueva and Martin A. Cordiner and Patrick G. J. Irwin and Imke de Pater and B. Butler and Mark A. Gurwell and Stefanie N. Milam and Conor A. Nixon and Statia Luszcz-Cook and C. F. Wilson and Vincent Kofman and G. Liuzzi and Sara Faggi and Thomas J. Fauchez and Marco Lippi and Rosario Cosentino and Alexander E. Thelen and Arielle Moullet and Paul Hartogh and Edward M. Molter and Steven B. Charnley and Giada N. Arney and Avram M. Mandell and N. Biver and Ann Carine Vandaele and Katherine R. de Kleer and Ravi kumar Kopparapu},
  journal={Nature Astronomy},
  year={2021}
}
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, Fauchez T.J.1,10, Lippi M.1,9, Cosentino R.1,11, Thelen A. E.1,10, Moullet A.12, Hartogh P.13, Molter E.M.4, Charnley S.1, Arney G.N.1, Mandell A.M.1, Biver N.14, Vandaele A.C.15, de Kleer K. R.16, Kopparapu R.1 

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We first respond to two points raised by Villanueva et al. We show the JCMT discovery spectrum of PH3 can not be re-attributed to SO2, as the line width is larger than observed for SO2 features, and

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