SPT-3G survey
E651443
The SPT-3G survey is a cosmic microwave background observation program using the third-generation camera on the South Pole Telescope to map the sky with high sensitivity and resolution for cosmology research.
All labels observed (1)
| Label | Occurrences |
|---|---|
| SPT-3G survey canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T7253255 — 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: SPT-3G survey Context triple: [South Pole Telescope, associatedSurvey, SPT-3G survey]
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A.
MIPSGAL survey
The MIPSGAL survey is a Spitzer Space Telescope legacy program that mapped the inner Milky Way in mid-infrared wavelengths to study Galactic structure, star formation, and interstellar dust.
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B.
GLIMPSE survey
The GLIMPSE survey is a Spitzer Space Telescope mid-infrared imaging project that mapped the inner Milky Way to study its structure and star-forming regions.
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C.
OGLE-III survey
OGLE-III survey was a major phase of the Optical Gravitational Lensing Experiment that conducted extensive long-term photometric monitoring of millions of stars to study microlensing events and variable objects in the sky.
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D.
CANDELS survey
The CANDELS survey is a major Hubble Space Telescope deep-imaging program designed to study the formation and evolution of galaxies across cosmic time.
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E.
Carnegie Irvine Galaxy Survey
The Carnegie Irvine Galaxy Survey is an astronomical project that provides detailed optical imaging and analysis of nearby galaxies to study their structure, formation, and evolution.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: SPT-3G survey Target entity description: The SPT-3G survey is a cosmic microwave background observation program using the third-generation camera on the South Pole Telescope to map the sky with high sensitivity and resolution for cosmology research.
-
A.
MIPSGAL survey
The MIPSGAL survey is a Spitzer Space Telescope legacy program that mapped the inner Milky Way in mid-infrared wavelengths to study Galactic structure, star formation, and interstellar dust.
-
B.
GLIMPSE survey
The GLIMPSE survey is a Spitzer Space Telescope mid-infrared imaging project that mapped the inner Milky Way to study its structure and star-forming regions.
-
C.
OGLE-III survey
OGLE-III survey was a major phase of the Optical Gravitational Lensing Experiment that conducted extensive long-term photometric monitoring of millions of stars to study microlensing events and variable objects in the sky.
-
D.
CANDELS survey
The CANDELS survey is a major Hubble Space Telescope deep-imaging program designed to study the formation and evolution of galaxies across cosmic time.
-
E.
Carnegie Irvine Galaxy Survey
The Carnegie Irvine Galaxy Survey is an astronomical project that provides detailed optical imaging and analysis of nearby galaxies to study their structure, formation, and evolution.
- F. None of above. chosen
Statements (45)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical survey
ⓘ
cosmic microwave background survey ⓘ |
| aimsTo |
constrain cosmological parameters
ⓘ
detect galaxy clusters via the Sunyaev–Zel’dovich effect ⓘ map the microwave sky with high angular resolution ⓘ map the microwave sky with high sensitivity ⓘ measure polarization anisotropies of the CMB ⓘ measure temperature anisotropies of the CMB ⓘ probe neutrino properties ⓘ study large-scale structure via CMB lensing ⓘ test models of dark energy ⓘ test models of inflation ⓘ |
| benefitsFrom | low atmospheric water vapor at South Pole ⓘ |
| collaboration | South Pole Telescope collaboration NERFINISHED ⓘ |
| country | Antarctica NERFINISHED ⓘ |
| dataType |
CMB polarization maps
ⓘ
CMB temperature maps ⓘ millimeter-wave sky maps ⓘ |
| environment | high, dry Antarctic plateau ⓘ |
| field |
astrophysics
ⓘ
cosmology ⓘ |
| goal | produce high signal-to-noise CMB maps for cosmology research ⓘ |
| hostFacility | South Pole Telescope facility NERFINISHED ⓘ |
| hostTelescopeAperture | 10-meter dish ⓘ |
| location |
Amundsen–Scott South Pole Station
NERFINISHED
ⓘ
South Pole NERFINISHED ⓘ |
| observes | cosmic microwave background ⓘ |
| observingSiteAltitude | ~2800 meters ⓘ |
| predecessor |
SPT-SZ survey
NERFINISHED
ⓘ
SPTpol survey NERFINISHED ⓘ |
| relatedProject | SPT-3G experiment NERFINISHED ⓘ |
| scienceCategory |
CMB lensing
ⓘ
cluster cosmology ⓘ large-scale structure ⓘ neutrino cosmology ⓘ secondary CMB anisotropies ⓘ |
| scienceCategory |
dark energy studies
ⓘ
inflationary cosmology ⓘ |
| skyCoverage | wide-area southern sky survey ⓘ |
| startEra | late 2010s ⓘ |
| surveyType | ground-based CMB survey ⓘ |
| telescopeGeneration | third-generation camera ⓘ |
| usesInstrument | SPT-3G camera ⓘ |
| usesTelescope | South Pole Telescope NERFINISHED ⓘ |
| wavelengthBand | millimeter ⓘ |
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: SPT-3G survey Description of subject: The SPT-3G survey is a cosmic microwave background observation program using the third-generation camera on the South Pole Telescope to map the sky with high sensitivity and resolution for cosmology research.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.