Diffuse extragalactic background radiation: Difference between revisions

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Revision as of 13:05, 30 November 2023 edit Dabed (talk \| contribs) Extended confirmed users 4,308 edits →See also: +Photon underproduction crisis Tag: Visual edit ← Previous edit		Latest revision as of 19:52, 17 June 2025 edit undo The Space Enthusiast (talk \| contribs) Extended confirmed users 17,035 edits Adding short description: "Photon field that fills our universe" Tag: Shortdesc helper
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Line 1: {{Short description\|Photon field that fills our universe}} {{one source \|date=March 2024}} [[Image:Extragalactic-background-power-density.jpg\|thumb\|321px\|right\|Schematic representation of the spectral energy distribution of the DEBRA. The dependent quantity is the [[spectral radiometric quantity\|spectral]] [[spectral radiance\|radiance]] multiplied by [[wavelength]], i.e. ''λL''<sub>e''λ''</sub>.