Long Wavelength Array collaboration
E355023
The Long Wavelength Array collaboration is a scientific consortium that operates low-frequency radio telescope arrays to study the universe at meter and decameter wavelengths, including phenomena such as the early universe, cosmic rays, and solar and planetary radio emissions.
All labels observed (2)
| Label | Occurrences |
|---|---|
| Long Wavelength Array collaboration canonical | 1 |
| Long Wavelength Array project | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T3397005 — 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.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Long Wavelength Array collaboration Context triple: [Owens Valley Radio Observatory, hasCollaboration, Long Wavelength Array collaboration]
-
A.
Atacama Compact Array
The Atacama Compact Array is a subset of smaller, closely spaced radio telescopes within the ALMA observatory designed to improve imaging of extended astronomical objects at millimeter and submillimeter wavelengths.
-
B.
Allen Telescope Array
The Allen Telescope Array is a large, multi-dish radio telescope facility in California designed primarily for simultaneous radio astronomy and the search for extraterrestrial intelligence.
-
C.
Atacama Large Millimeter/submillimeter Array
The Atacama Large Millimeter/submillimeter Array is a powerful astronomical observatory composed of dozens of radio antennas that study the cold universe—such as star and planet formation—by observing millimeter and submillimeter wavelengths.
-
D.
Arecibo L-band Feed Array survey
The Arecibo L-band Feed Array survey is a major radio astronomy project that used the Arecibo telescope’s multi-beam receiver to map neutral hydrogen and study the large-scale structure and dynamics of galaxies.
-
E.
Very Long Baseline Array
The Very Long Baseline Array is a continent-spanning network of ten radio telescopes used for high-resolution astronomical observations through very long baseline interferometry.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: Long Wavelength Array collaboration Target entity description: The Long Wavelength Array collaboration is a scientific consortium that operates low-frequency radio telescope arrays to study the universe at meter and decameter wavelengths, including phenomena such as the early universe, cosmic rays, and solar and planetary radio emissions.
-
A.
Atacama Compact Array
The Atacama Compact Array is a subset of smaller, closely spaced radio telescopes within the ALMA observatory designed to improve imaging of extended astronomical objects at millimeter and submillimeter wavelengths.
-
B.
Allen Telescope Array
The Allen Telescope Array is a large, multi-dish radio telescope facility in California designed primarily for simultaneous radio astronomy and the search for extraterrestrial intelligence.
-
C.
Atacama Large Millimeter/submillimeter Array
The Atacama Large Millimeter/submillimeter Array is a powerful astronomical observatory composed of dozens of radio antennas that study the cold universe—such as star and planet formation—by observing millimeter and submillimeter wavelengths.
-
D.
Arecibo L-band Feed Array survey
The Arecibo L-band Feed Array survey is a major radio astronomy project that used the Arecibo telescope’s multi-beam receiver to map neutral hydrogen and study the large-scale structure and dynamics of galaxies.
-
E.
Very Long Baseline Array
The Very Long Baseline Array is a continent-spanning network of ten radio telescopes used for high-resolution astronomical observations through very long baseline interferometry.
- F. None of above. chosen
Statements (31)
| Predicate | Object |
|---|---|
| instanceOf |
astronomy collaboration
ⓘ
radio astronomy consortium ⓘ scientific collaboration ⓘ |
| associatedWith |
Long Wavelength Array station LWA-SV
ⓘ
linked to:
Long Wavelength Array station
Long Wavelength Array station LWA1 ⓘ
linked to:
Long Wavelength Array station
|
| country |
United States
ⓘ
linked to:
United States of America
|
| dataType |
all-sky low-frequency radio images
ⓘ
radio interferometric data ⓘ |
| field |
astrophysics
ⓘ
radio astronomy ⓘ space physics ⓘ |
| focus |
space weather-related radio emissions
ⓘ
time-domain astrophysics at low radio frequencies ⓘ transient radio phenomena ⓘ |
| goal | study the universe at low radio frequencies ⓘ |
| instrumentType |
aperture synthesis array
ⓘ
dipole antenna array ⓘ |
| operates |
Long Wavelength Array
ⓘ
linked to:
Long Wavelength Array station
low-frequency radio telescope arrays ⓘ |
| researchArea |
cosmology
ⓘ
heliophysics ⓘ high-energy astrophysics ⓘ planetary science ⓘ |
| studies |
cosmic rays
ⓘ
early universe ⓘ low-frequency radio sky ⓘ planetary radio emissions ⓘ solar radio emissions ⓘ |
| usesFrequencyRange | low radio frequencies ⓘ |
| usesWavelengthRange |
decameter wavelengths
ⓘ
meter wavelengths ⓘ |
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.
Instruction
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.
Input
Subject: Long Wavelength Array collaboration Description of subject: The Long Wavelength Array collaboration is a scientific consortium that operates low-frequency radio telescope arrays to study the universe at meter and decameter wavelengths, including phenomena such as the early universe, cosmic rays, and solar and planetary radio emissions.
Referenced by (2)
Full triples — surface form annotated when it differs from this entity's canonical label.
linked to: Long Wavelength Array collaboration