Sunyaev–Zel’dovich effect
E651437
The Sunyaev–Zel’dovich effect is a distortion of the cosmic microwave background radiation caused by high-energy electrons in galaxy clusters, used as a powerful probe of large-scale structure and cosmology.
All labels observed (2)
| Label | Occurrences |
|---|---|
| Sunyaev–Zel’dovich cluster catalogs | 1 |
| Sunyaev–Zel’dovich effect canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T7253212 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
Target entity: Sunyaev–Zel’dovich effect Context triple: [South Pole Telescope, researchFocus, Sunyaev–Zel’dovich effect]
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A.
cosmic microwave background
The cosmic microwave background is the faint, nearly uniform afterglow radiation permeating the universe, providing a snapshot of the cosmos about 380,000 years after the Big Bang.
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B.
CMB
CMB is the National Rail station code for Cambridge North railway station in Cambridge, England.
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C.
CMB
CMB is a U.S. Army decoration awarded to medical personnel who provide frontline medical care while engaged in active ground combat.
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D.
CMB
CMB is the three-letter IATA airport code for Bandaranaike International Airport, the main international gateway to Sri Lanka near Colombo.
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E.
Perseus Cluster
The Perseus Cluster is a massive, nearby galaxy cluster dominated by the bright galaxy NGC 1275 and known for its hot X-ray–emitting gas and powerful radio and acoustic phenomena in its intracluster medium.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Sunyaev–Zel’dovich effect Target entity description: The Sunyaev–Zel’dovich effect is a distortion of the cosmic microwave background radiation caused by high-energy electrons in galaxy clusters, used as a powerful probe of large-scale structure and cosmology.
-
A.
cosmic microwave background
The cosmic microwave background is the faint, nearly uniform afterglow radiation permeating the universe, providing a snapshot of the cosmos about 380,000 years after the Big Bang.
-
B.
CMB
CMB is the National Rail station code for Cambridge North railway station in Cambridge, England.
-
C.
CMB
CMB is a U.S. Army decoration awarded to medical personnel who provide frontline medical care while engaged in active ground combat.
-
D.
CMB
CMB is the three-letter IATA airport code for Bandaranaike International Airport, the main international gateway to Sri Lanka near Colombo.
-
E.
Perseus Cluster
The Perseus Cluster is a massive, nearby galaxy cluster dominated by the bright galaxy NGC 1275 and known for its hot X-ray–emitting gas and powerful radio and acoustic phenomena in its intracluster medium.
- F. None of above. chosen
Statements (49)
| Predicate | Object |
|---|---|
| instanceOf |
astrophysical effect
ⓘ
cosmological probe ⓘ radiative transfer phenomenon ⓘ |
| affects | cosmic microwave background radiation NERFINISHED ⓘ |
| causedBy |
high-energy electrons in galaxy clusters
ⓘ
hot intracluster medium ⓘ inverse Compton scattering ⓘ |
| complementaryTo | X-ray cluster observations ⓘ |
| dependsOn | electron pressure along the line of sight ⓘ |
| detectedBy |
Atacama Cosmology Telescope
NERFINISHED
ⓘ
Planck satellite NERFINISHED ⓘ South Pole Telescope NERFINISHED ⓘ |
| distorts |
CMB intensity spectrum
ⓘ
CMB temperature anisotropies ⓘ |
| field |
astrophysics
ⓘ
cosmology ⓘ |
| firstDescribedBy |
Rashid Sunyaev
NERFINISHED
ⓘ
Yakov Zel’dovich NERFINISHED ⓘ |
| firstDescribedIn | 1970s ⓘ |
| hasType |
kinetic Sunyaev–Zel’dovich effect
NERFINISHED
ⓘ
relativistic Sunyaev–Zel’dovich effect NERFINISHED ⓘ thermal Sunyaev–Zel’dovich effect NERFINISHED ⓘ |
| independentOf | redshift of the galaxy cluster ⓘ |
| measuredBy |
CMB experiments
ⓘ
interferometric radio telescopes ⓘ millimeter-wave telescopes ⓘ |
| namedAfter |
Rashid Sunyaev
NERFINISHED
ⓘ
Yakov Zel’dovich NERFINISHED ⓘ |
| observableAs |
CMB temperature decrement at low frequencies
ⓘ
CMB temperature increment at high frequencies ⓘ |
| occursIn |
galaxy clusters
ⓘ
large-scale structure filaments ⓘ |
| probes |
growth of structure in the universe
ⓘ
intracluster medium thermodynamics ⓘ |
| quantifiedBy | Compton y-parameter NERFINISHED ⓘ |
| redshiftIndependenceReason | surface brightness conservation ⓘ |
| relatedTo | X-ray emission from galaxy clusters ⓘ |
| sensitiveTo |
electron density
ⓘ
electron temperature ⓘ |
| theoreticalBasis | inverse Compton scattering of CMB photons ⓘ |
| usedFor |
constraining cosmological parameters
ⓘ
detecting galaxy clusters ⓘ estimating cluster total mass ⓘ mapping baryon distribution in the universe ⓘ measuring Hubble constant ⓘ measuring cluster gas pressure ⓘ probing dark energy ⓘ studying large-scale structure ⓘ |
| uses | cosmic microwave background photons ⓘ |
How these facts were elicited
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You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Subject: Sunyaev–Zel’dovich effect Description of subject: The Sunyaev–Zel’dovich effect is a distortion of the cosmic microwave background radiation caused by high-energy electrons in galaxy clusters, used as a powerful probe of large-scale structure and cosmology.
Referenced by (2)
Full triples — surface form annotated when it differs from this entity's canonical label.