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)
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 ⓘ |
Referenced by (29)
Full triples — surface form annotated when it differs from this entity's canonical label.
subject surface form:
Northern Chile
this entity surface form:
Atacama Large Millimeter Array
this entity surface form:
ALMA Observatory
this entity surface form:
ALMA
Atacama Large Millimeter/submillimeter Array
→
abbreviation
→
Atacama Large Millimeter/submillimeter Array
self-linksurface differs
ⓘ
this entity surface form:
ALMA
this entity surface form:
Atacama Large Millimeter Array
this entity surface form:
ALMA
this entity surface form:
Atacama Large Millimeter/submillimeter Array Observatory
this entity surface form:
ALMA
this entity surface form:
ALMA 12-m array
this entity surface form:
ALMA Observatory
this entity surface form:
Atacama Large Millimeter/submillimeter Array antennas
this entity surface form:
ALMA Observatory