thermal Sunyaev-Zel'dovich effect
GPTKB entity
Statements (24)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
gptkb:astrophysical_effect
|
| gptkbp:alsoKnownAs |
gptkb:tSZ_effect
|
| gptkbp:amendedBy |
CMB photon energy
|
| gptkbp:causedBy |
gptkb:inverse_Compton_scattering
|
| gptkbp:describes |
distortion of cosmic microwave background
|
| gptkbp:discoveredIn |
1970
|
| gptkbp:firstDescribed |
Sunyaev and Zel'dovich
|
| gptkbp:frequencyDependence |
distinct spectral signature
|
| gptkbp:involves |
hot electron gas
|
| gptkbp:namedAfter |
gptkb:Rashid_Sunyaev
gptkb:Yakov_Zel'dovich |
| gptkbp:observedBy |
microwave telescopes
|
| gptkbp:occurredIn |
galaxy clusters
|
| gptkbp:relatedTo |
gptkb:cosmology
gptkb:kinetic_Sunyaev-Zel'dovich_effect astrophysics |
| gptkbp:usedFor |
measuring cluster properties
estimating Hubble constant studying large-scale structure |
| gptkbp:bfsParent |
gptkb:kinematic_Sunyaev-Zel'dovich_effect
gptkb:tSZ_effect gptkb:Sunyaev-Zel'dovich_effect |
| gptkbp:bfsLayer |
8
|
| https://www.w3.org/2000/01/rdf-schema#label |
thermal Sunyaev-Zel'dovich effect
|