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The statistical reliability of 267-GHz JCMT observations of Venus: no significant evidence for phosphine absorption
M. A. Thompson, 2020. Monthly Notices of the Royal Astronomical Society: Letters 501(1), L18–L22.
Re-analyses the JCMT spectrum with low-order and multiple higher-order polynomial baselines and a non-parametric bootstrap; neither method recovers a significant line, and polynomial fitting produces false positives.
What it's used for here
The critique of the JCMT detection.
Cited by on this site 4 records
EVD
Phosphine in the clouds of Venus
MYSThe mystery article
Cite it
Thompson, M. A. (2020). The statistical reliability of 267-GHz JCMT observations of Venus: no significant evidence for phosphine absorption. Monthly Notices of the Royal Astronomical Society: Letters 501(1), L18–L22. https://doi.org/10.1093/mnrasl/slaa187
@article{thompson2020statistical,
author = {Thompson, M. A.},
title = {The statistical reliability of 267-GHz JCMT observations of Venus: no significant evidence for phosphine absorption},
journal = {Monthly Notices of the Royal Astronomical Society: Letters 501(1), L18–L22},
year = {2020},
doi = {10.1093/mnrasl/slaa187},
url = {https://doi.org/10.1093/mnrasl/slaa187}
}TY - JOUR TI - The statistical reliability of 267-GHz JCMT observations of Venus: no significant evidence for phosphine absorption AU - Thompson, M. A. PY - 2020 JO - Monthly Notices of the Royal Astronomical Society: Letters 501(1), L18–L22 DO - 10.1093/mnrasl/slaa187 UR - https://doi.org/10.1093/mnrasl/slaa187 ER -
Thompson, M. A.. “The statistical reliability of 267-GHz JCMT observations of Venus: no significant evidence for phosphine absorption.” Monthly Notices of the Royal Astronomical Society: Letters 501(1), L18–L22 (2020). https://doi.org/10.1093/mnrasl/slaa187.