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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.

MYS0CQY1PJR4XT7 · mystery · click to copyMPhosphine in the clouds of VenusArticledoi: 10.1093/mnrasl/slaa187Checked against the original0

What it's used for here

The critique of the JCMT detection.

Cited by on this site 4 records

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
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