Re-analysis of the 267 GHz ALMA observations of Venus

@article{Snellen2020ReanalysisOT,
  title={Re-analysis of the 267 GHz ALMA observations of Venus},
  author={Ignas A. G. Snellen and Lizette Guzm{\'a}n-Ram{\'i}rez and Michiel R. Hogerheijde and Alexander P. S. Hygate and Floris van der Tak},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2020}
}
Context: ALMA observations of Venus at 267 GHz have been presented in the literature that show the apparent presence of phosphine (PH3) in its atmosphere. Phosphine has currently no evident production routes on the planet's surface or in its atmosphere. Aims: The aim of this work is to assess the statistical reliability of the line detection by independent re-analysis of the ALMA data. Methods: The ALMA data were reduced as in the published study, following the provided scripts. First the… Expand

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A&A proofs: manuscript
  • JQSRT 130,
  • 2013