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About ALMA
Origins
Global Collaboration
Privileged Location
How ALMA works
How does ALMA see?
Capabilities
Deep Field
Early Galaxy Formation
Star and planet formation
Detecting extrasolar planets under formation
Stars
The Sun
Evolved stars
Dust and molecules in space (Astrochemistry)
Technologies
Antennas
Receivers
Optic fiber
Correlator
Interferometry
Transporters
How ALMA Observations are carried out
Discoveries
ALMA in Chile
Benefits for the Community
Chile: Astronomical Capital
Astronomic Research in Chile
Chilean Astronomy Development Fund
Human Resources and Technology
Collaboration with Universities
Astroinformatics
Medicine at high altitudes
Telecommunications Infrastructure
Local community support
Education and Outreach
Immunities
The people
The ALMA Board
ALMA Management
The ALMA Committees
ASAC Members List
JAO Science Team
The Workers at ALMA
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LIVE from Chajnantor
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Astronomers make most distant detection yet of fluorine in star-forming galaxy
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ALMA Scientists Detect Signs of Water in a Galaxy Far, Far Away
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A Cosmic Whodunit: ALMA Study Confirms What’s Robbing Galaxies of Their Star-Forming Gas
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ALMA celebrates 10 years of science
#ALMAnames
Winning names for antennas after popular poll
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ALMA celebrates 10 years of its first image with a contest to name its antennas
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ALMA Unveil Galaxies at Cosmic Dawn That Were Hiding Behind the Dust
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ALMA Scientists Uncover the Mystery of Early Massive Galaxies Running on Empty
Interview to Ed Fomalont
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ALMA Reveals Carbon-Rich, Organic Birth Environments of Planets
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Dense Molecular Clouds in the Center of Milky Way are Unable to Form Stars
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ALMA Goes to New (Wave)Lengths
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