Linked from

The 16 pages that link to Sunyaev–Zel'dovich effect, each with the reason it gives.

• Cosmic microwave backgroundCompared with: It modifies the primordial glow along galaxy-cluster sightlines rather than originating at recombination.

• Galaxy clusterRelated: It detects clusters through their hot plasma, including at great distances.

• Cosmic webRelated: It helps detect hot gas in clusters and dense cosmic structures.

• Intracluster mediumRelated: Intracluster electrons imprint this signal, enabling cluster studies independent of distance dimming.

• Intergalactic mediumRelated: Hot electrons in galaxy clusters imprint this signal on the background radiation.

• Thomson scatteringBroader topic: It uses the related scattering process to detect hot cluster gas.

• Inverse Compton scatteringBroader topic: It is a large-scale, measurable signature of photons gaining energy from energetic electrons.

• Circumgalactic mediumRelated: It can measure the pressure of hot gas in massive galaxy halos.

• Shapley SuperclusterRelated: This effect helps detect and measure clusters independently of their optical galaxy light.

• Warm–hot intergalactic mediumRelated: Electrons in hot intergalactic gas can imprint a microwave signal even when the gas is faint in X-rays.

• Missing baryon problemRelated: Its signal can reveal hot gas in galaxy groups and filaments without relying on visible light.

• Perseus ClusterRelated: Its signal can probe the Perseus Cluster’s thermal pressure independently of X-ray emission.

• South Pole TelescopeRelated: This effect lets the telescope detect galaxy clusters as they imprint signals on the microwave background.

• Dark flowBroader topic: Its thermal component can obscure the much smaller motion-dependent signal.

• Galaxy groups and clustersRelated: Its signal reveals hot cluster gas even when a cluster is distant.

• Submillimetre astronomyBroader topic: Its spectral signal is measured at submillimetre wavelengths to study clusters across cosmic distances.