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LATENT REFERENCES / TAG2

Cosmic Microwave Background Estimation

Archive curator and editor: Keigo Yoshida

This reference note belongs to Tag2 in Latent References, an archive curated by Keigo Yoshida. Its archive region is Visual. The note preserves its source text and links so that readers can trace the material behind the 3D map.

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Tag2
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Visual

Archived reference note

English translation of the archived note. JP shows the original text. Source links and literal code are retained; the translation does not update or independently verify the source claims.

https://scrapbox.io/files/648b1e54392237001be7bda2.png https://dus.jpl.nasa.gov/projects/cmb/ The Cosmic Microwave Background (CMB) is the main source of information we have about the early Universe. The importance of estimating the spatial power spectrum of the cosmic microwave background is the due to the wealth of information it yields about the physical properties of the Universe. These fundamental properties leave different statistical patterns of hot and cold spots on the sky at microwave frequencies.

Source updated 2023-06-15 · Snapshot 2026-10-08

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