QUIJOTE experiment
E599490
The QUIJOTE experiment is a cosmology project using microwave telescopes to study the polarization of the cosmic microwave background and Galactic emission from the Teide Observatory in Spain.
All labels observed (2)
| Label | Occurrences |
|---|---|
| BOOMERanG experiment | 1 |
| QUIJOTE experiment canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T6580128 — 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: QUIJOTE experiment Context triple: [Teide Observatory, hosts, QUIJOTE experiment]
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A.
DUNE experiment
The DUNE experiment is a major international neutrino physics project designed to study neutrino oscillations, matter–antimatter asymmetry, and proton decay using intense neutrino beams and massive underground detectors.
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B.
DIRAC experiment
The DIRAC experiment is a high-energy physics project at CERN designed to study pionium (a bound state of a π⁺ and π⁻ meson) to test predictions of low-energy quantum chromodynamics.
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C.
AMS-02 experiment
The AMS-02 experiment is a state-of-the-art particle physics detector mounted on the International Space Station to study cosmic rays and search for dark matter and antimatter in space.
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D.
COMPASS experiment
The COMPASS experiment is a high-energy physics experiment at CERN designed to study the structure and dynamics of hadrons using intense muon and hadron beams.
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E.
ALICE experiment
The ALICE experiment is a major detector at CERN’s Large Hadron Collider designed to study quark–gluon plasma and the physics of heavy-ion collisions.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: QUIJOTE experiment Target entity description: The QUIJOTE experiment is a cosmology project using microwave telescopes to study the polarization of the cosmic microwave background and Galactic emission from the Teide Observatory in Spain.
-
A.
DUNE experiment
The DUNE experiment is a major international neutrino physics project designed to study neutrino oscillations, matter–antimatter asymmetry, and proton decay using intense neutrino beams and massive underground detectors.
-
B.
DIRAC experiment
The DIRAC experiment is a high-energy physics project at CERN designed to study pionium (a bound state of a π⁺ and π⁻ meson) to test predictions of low-energy quantum chromodynamics.
-
C.
AMS-02 experiment
The AMS-02 experiment is a state-of-the-art particle physics detector mounted on the International Space Station to study cosmic rays and search for dark matter and antimatter in space.
-
D.
COMPASS experiment
The COMPASS experiment is a high-energy physics experiment at CERN designed to study the structure and dynamics of hadrons using intense muon and hadron beams.
-
E.
ALICE experiment
The ALICE experiment is a major detector at CERN’s Large Hadron Collider designed to study quark–gluon plasma and the physics of heavy-ion collisions.
- F. None of above. chosen
Statements (47)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical survey
ⓘ
cosmology experiment ⓘ microwave polarization experiment ⓘ |
| aimsTo |
characterize Galactic foregrounds for CMB studies
ⓘ
constrain cosmological parameters related to inflation ⓘ measure polarization of the microwave sky ⓘ support future CMB polarization missions ⓘ |
| collaborationType | international collaboration ⓘ |
| country | Spain ⓘ |
| dataType |
intensity maps
ⓘ
multi-frequency sky maps ⓘ polarization maps ⓘ |
| environment | ground-based ⓘ |
| field |
astrophysics
ⓘ
cosmology ⓘ |
| focusesOn |
large-scale CMB polarization
ⓘ
polarization ⓘ |
| hasComponent |
QUIJOTE telescopes
NERFINISHED
ⓘ
multi-frequency polarimeters ⓘ |
| hasScientificGoal |
improve understanding of Galactic foregrounds at microwave frequencies
ⓘ
provide complementary data to satellite CMB missions ⓘ study large-scale structure of the microwave sky ⓘ |
| hostObservatory | Teide Observatory NERFINISHED ⓘ |
| locatedAt | Teide Observatory NERFINISHED ⓘ |
| locatedIn |
Canary Islands
ⓘ
Tenerife NERFINISHED ⓘ |
| measures |
Stokes Q parameter
ⓘ
Stokes U parameter ⓘ total intensity ⓘ |
| observatoryAltitude | approximately 2400 meters ⓘ |
| observes |
Galactic dust emission
ⓘ
Galactic synchrotron emission ⓘ cosmic microwave background ⓘ |
| observingStrategy |
large-area sky survey
ⓘ
multi-frequency observations ⓘ |
| relatedTo |
B-mode polarization searches
ⓘ
Galactic magnetic field studies ⓘ Planck mission NERFINISHED ⓘ |
| researchArea |
Galactic emission
ⓘ
cosmic microwave background polarization ⓘ foreground characterization ⓘ |
| scientificDiscipline | observational cosmology ⓘ |
| status | operational ⓘ |
| supports | foreground separation for CMB experiments ⓘ |
| telescopeMountType | alt-azimuth mount ⓘ |
| usesInstrumentType | microwave telescope ⓘ |
| wavelengthRange | microwave ⓘ |
How these facts were elicited
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
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: QUIJOTE experiment Description of subject: The QUIJOTE experiment is a cosmology project using microwave telescopes to study the polarization of the cosmic microwave background and Galactic emission from the Teide Observatory in Spain.
Referenced by (2)
Full triples — surface form annotated when it differs from this entity's canonical label.