Morita Array

E665895

The Morita Array is a subset of the Atacama Large Millimeter/submillimeter Array (ALMA) consisting of closely spaced, smaller antennas designed to improve imaging of extended astronomical objects at millimeter and submillimeter wavelengths.

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All labels observed (1)

Label Occurrences
Morita Array canonical 1

Statements (40)

Predicate Object
instanceOf interferometric array
radio telescope array
alsoKnownAs ACA NERFINISHED
Atacama Compact Array NERFINISHED
bandCoverage ALMA Bands 3–10 (with configuration-dependent availability)
continent South America
contributesTo ALMA uv-coverage at short spacings
country Chile
designedFor high-fidelity imaging of diffuse emission
imaging extended astronomical objects
environment high-altitude, dry site
hasComponent 12-meter total power antennas
7-meter antenna array
improves ALMA imaging of extended sources
locatedAt Llano de Chajnantor Observatory NERFINISHED
locatedAtAltitude about 5000 meters
locatedIn Atacama Desert
Chile
namedAfter Koh-ichiro Morita NERFINISHED
operatedBy ALMA Observatory NERFINISHED
European Southern Observatory NERFINISHED
National Astronomical Observatory of Japan NERFINISHED
National Radio Astronomy Observatory NERFINISHED
organizationPartner ESO NERFINISHED
NAOJ NERFINISHED
NRAO NERFINISHED
partOf Atacama Large Millimeter/submillimeter Array NERFINISHED
primaryFunction to improve ALMA sensitivity to large angular scales
to provide short baselines for ALMA
purpose to complement the main ALMA 12-meter array
scienceGoals cosmic star formation
study of molecular clouds
study of nearby galaxies
study of protoplanetary disks
site Chajnantor Plateau NERFINISHED
telescopeType ground-based observatory
usesTechnique aperture synthesis
radio interferometry
wavelengthRange millimeter
submillimeter

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

Atacama Compact Array alsoKnownAs Morita Array