UltraVISTA survey
E666539
UltraVISTA survey is a deep near-infrared astronomical imaging survey of the COSMOS field designed to study galaxy formation and evolution in the early universe.
All labels observed (3)
| Label | Occurrences |
|---|---|
| UltraVISTA survey canonical | 3 |
| VISTA Deep Extragalactic Observations Survey | 1 |
| VISTA Deep Extragalactic Observations survey | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T7459452 — 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: UltraVISTA survey Context triple: [VISTA, supportsSurvey, UltraVISTA survey]
-
A.
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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B.
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.
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C.
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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D.
OGLE-IV survey
The OGLE-IV survey is a large-scale astronomical sky survey focused on detecting microlensing events and variable stars, conducted with the Warsaw Telescope at Las Campanas Observatory.
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E.
Carnegie-Spitzer-IMACS Survey
The Carnegie-Spitzer-IMACS Survey is an astronomical research project that combines infrared observations from the Spitzer Space Telescope with optical spectroscopy from the IMACS instrument to study the formation and evolution of galaxies across cosmic time.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: UltraVISTA survey Target entity description: UltraVISTA survey is a deep near-infrared astronomical imaging survey of the COSMOS field designed to study galaxy formation and evolution in the early universe.
-
A.
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.
-
B.
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.
-
C.
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.
-
D.
OGLE-IV survey
The OGLE-IV survey is a large-scale astronomical sky survey focused on detecting microlensing events and variable stars, conducted with the Warsaw Telescope at Las Campanas Observatory.
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E.
Carnegie-Spitzer-IMACS Survey
The Carnegie-Spitzer-IMACS Survey is an astronomical research project that combines infrared observations from the Spitzer Space Telescope with optical spectroscopy from the IMACS instrument to study the formation and evolution of galaxies across cosmic time.
- F. None of above. chosen
Statements (46)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical survey
ⓘ
deep extragalactic survey ⓘ near-infrared imaging survey ⓘ |
| band | near-infrared bands ⓘ |
| coordinatesSystem | equatorial coordinates ⓘ |
| cosmologicalRedshiftRange | up to redshift z greater than 6 ⓘ |
| dataAccess |
ESO Science Archive
ⓘ
linked to:
ESO Science Archive Facility
publicly available survey ⓘ |
| dataProduct |
deep near-infrared images
ⓘ
multi-epoch imaging ⓘ public data releases ⓘ |
| depth | very deep near-infrared imaging ⓘ |
| enables |
photometric redshift estimation
ⓘ
selection of high-redshift galaxy candidates ⓘ stellar mass measurements of galaxies ⓘ |
| field | COSMOS field ⓘ |
| filter |
H band
ⓘ
J band ⓘ Ks band ⓘ NB118 narrow-band filter ⓘ Y band ⓘ |
| hostInstitution | ESO VISTA Public Surveys program ⓘ |
| location | Southern Hemisphere sky ⓘ |
| observatory | Paranal Observatory ⓘ |
| organization | European Southern Observatory ⓘ |
| primaryGoal |
study early universe galaxies
ⓘ
study galaxy evolution ⓘ study galaxy formation ⓘ |
| relatedTo |
COSMOS survey
ⓘ
VISTA telescope public surveys ⓘ
linked to:
VISTA Hemisphere Survey
|
| scienceCase |
cosmic star-formation history
ⓘ
evolution of the galaxy stellar mass function ⓘ high-redshift galaxy populations ⓘ large-scale structure at high redshift ⓘ luminous and massive galaxies in the early universe ⓘ mass assembly of galaxies ⓘ quiescent galaxies at high redshift ⓘ star-forming galaxies at high redshift ⓘ |
| skyCoverage |
COSMOS 2 square degree field
ⓘ
linked to:
COSMOS field
|
| startDate | around 2009 ⓘ |
| strategy |
deep-wide coverage
ⓘ
ultra-deep stripes ⓘ |
| surveyType | imaging survey ⓘ |
| telescope | VISTA telescope ⓘ |
| usesInstrument | VIRCAM ⓘ |
| wavelengthRange | near-infrared ⓘ |
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: UltraVISTA survey Description of subject: UltraVISTA survey is a deep near-infrared astronomical imaging survey of the COSMOS field designed to study galaxy formation and evolution in the early universe.
Referenced by (5)
Full triples — surface form annotated when it differs from this entity's canonical label.