et al.
Chapter I /  Figure 1.2
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Fig 1.2: Posterior distributions of the kinematic parameters of a high-redshift galaxy.
A. L. Danhaive
Danhaive et al.
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ChapterI
Figure1.2
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The science

A galaxy so distant that its light has been travelling for most of the age of the universe cannot simply be measured; its properties have to be inferred. This figure is that inference laid bare. Each panel shows how strongly the data constrain one parameter of the galaxy's motion, and how those constraints trade off against each other.

The diagonal shows what is known about each quantity on its own. Everything below it shows which combinations remain possible together.

Contributed by A. L. Danhaive.
et al.
O. Marx, Et Al. Apparel, Cambridge (2024)
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