Atacama Large Millimeter/submillimeter Array
E32871
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.
All labels observed (7)
How this entity was disambiguated
This entity first appeared as the object of triple T253489 — 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: Atacama Large Millimeter/submillimeter Array Context triple: [Northern Chile, contains, Atacama Large Millimeter/submillimeter Array]
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A.
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.
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B.
Magellan Clay Telescope
The Magellan Clay Telescope is one of the twin 6.5-meter Magellan telescopes at Las Campanas Observatory in Chile, used for cutting-edge optical and infrared astronomical research.
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C.
Giant Magellan Telescope
The Giant Magellan Telescope is a next-generation, extremely large ground-based optical and infrared telescope designed to achieve unprecedented resolution for astronomical observations.
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D.
Gemini South Observatory
Gemini South Observatory is a major 8.1-meter optical and infrared telescope facility located on Cerro Pachón in Chile, forming the southern half of the international Gemini Observatory.
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E.
Magellan Telescopes
Magellan Telescopes are a pair of 6.5-meter optical-infrared telescopes at Las Campanas Observatory in Chile, used for cutting-edge astronomical research by an international collaboration.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Atacama Large Millimeter/submillimeter Array Target entity description: 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.
-
A.
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.
-
B.
Magellan Clay Telescope
The Magellan Clay Telescope is one of the twin 6.5-meter Magellan telescopes at Las Campanas Observatory in Chile, used for cutting-edge optical and infrared astronomical research.
-
C.
Giant Magellan Telescope
The Giant Magellan Telescope is a next-generation, extremely large ground-based optical and infrared telescope designed to achieve unprecedented resolution for astronomical observations.
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D.
Gemini South Observatory
Gemini South Observatory is a major 8.1-meter optical and infrared telescope facility located on Cerro Pachón in Chile, forming the southern half of the international Gemini Observatory.
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E.
Magellan Telescopes
Magellan Telescopes are a pair of 6.5-meter optical-infrared telescopes at Las Campanas Observatory in Chile, used for cutting-edge astronomical research by an international collaboration.
- F. None of above. chosen
Statements (49)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical observatory
ⓘ
interferometer ⓘ radio telescope array ⓘ |
| abbreviation |
Atacama Large Millimeter/submillimeter Array
self-linksurface differs
ⓘ
surface form:
ALMA
|
| altitude | about 5000 meters above sea level ⓘ |
| angularResolution | milliarcsecond scale at highest frequencies ⓘ |
| bandCoverage | approximately 30 GHz to 950 GHz ⓘ |
| constructionStart | 2004 ⓘ |
| country | Chile ⓘ |
| environment | high-altitude desert ⓘ |
| firstScienceObservations | 2011 ⓘ |
| fundedBy |
East Asia
ⓘ
Europe ⓘ North America ⓘ Chile ⓘ
surface form:
Republic of Chile
|
| hasComponent | Atacama Compact Array ⓘ |
| inaugurationDate | 2013 ⓘ |
| includes |
12 7-meter antennas
ⓘ
4 12-meter total-power antennas ⓘ 50 12-meter antennas ⓘ |
| locatedAt | Chajnantor Plateau ⓘ |
| locatedIn |
Atacama Desert
ⓘ
Chile ⓘ |
| managedBy |
European Southern Observatory
ⓘ
NAOJ ⓘ
surface form:
National Astronomical Observatory of Japan
National Radio Astronomy Observatory ⓘ |
| maximumBaseline | about 16 kilometers ⓘ |
| notableDiscovery |
detailed images of protoplanetary disk HL Tauri
ⓘ
detailed observations of distant star-forming galaxies ⓘ |
| numberOfAntennas | 66 ⓘ |
| observes |
continuum emission
ⓘ
dust emission ⓘ molecular gas ⓘ spectral lines ⓘ |
| operatedBy |
European Southern Observatory
ⓘ
surface form:
ESO
Joint ALMA Observatory ⓘ NAOJ ⓘ National Radio Astronomy Observatory ⓘ
surface form:
NRAO
|
| primaryScienceGoal | study of the cold universe ⓘ |
| reasonForLocation | extremely dry atmosphere suitable for submillimeter observations ⓘ |
| studies |
galaxies in the early universe
ⓘ
molecular clouds ⓘ planet formation ⓘ protoplanetary disks ⓘ star formation ⓘ |
| technology | aperture synthesis ⓘ |
| uses | radio interferometry ⓘ |
| wavelengthRange |
millimeter
ⓘ
submillimeter ⓘ |
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Subject: Atacama Large Millimeter/submillimeter Array Description of subject: 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.
Referenced by (29)
Full triples — surface form annotated when it differs from this entity's canonical label.