File:Example of apparently detected PH3 spectrum on Venus after baseline-fitting with residual offset above and 5 ppb model of PH3 superimposed.png

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Captions

Captions

From the study "Re-analysis of Phosphine in Venus' Clouds" "As for (f4) but after baseline-fitting; residual offset above; 5 ppb model superimposed."

Summary

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Description
English: "Figure (f5) shows the same spectrum (in red) after removal of the 4th-order polynomial plotted in Figure (f4). The overlaid curve (in black) is a model profile for 5 ppb of PH 3, scaled from our radiative transfer model, and with a spectral baseline subtracted in the same way as for the data, and the upper (grey) histogram shows the residual after subtraction of this model line."


(A screenshot of the PDF made with Spectacle and Okular)
Date
Source https://arxiv.org/abs/2011.08176
Author Authors of the study: Jane S. Greaves, Anita M. S. Richards, William Bains, Paul B. Rimmer, David L. Clements, Sara Seager, Janusz J. Petkowski, Clara Sousa-Silva, Sukrit Ranjan, Helen J. Fraser

Licensing

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w:en:Creative Commons
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current22:50, 27 December 2020Thumbnail for version as of 22:50, 27 December 20207,351 × 5,046 (240 KB)Prototyperspective (talk | contribs)Uploaded a work by Authors of the study: Jane S. Greaves, Anita M. S. Richards, William Bains, Paul B. Rimmer, David L. Clements, Sara Seager, Janusz J. Petkowski, Clara Sousa-Silva, Sukrit Ranjan, Helen J. Fraser from https://arxiv.org/abs/2011.08176 with UploadWizard

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