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The ALMA Development Program: Roadmap to 2030
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The Atacama Large Millimeter/submillimeter Array (ALMA) is the premier telescope for sensitive, high-resolution observations at millimeter and submillimeter wavelengths. The array consists of fifty 12-m diameter antennas that can be reconfigured to baselines as long as 16 km, twelve 7-m antennas that sample the short visibility spacings, and four 12-m antennas that provide total power capabilities for spectral line and continuum observations. Located in the Atacama desert in northern Chile at an elevation of 5000 m on the Chajnantour plateau, the ALMA site provides excellent observing conditions with low precipitable water vapor. The large number of antennas, the high-altitude site, and excellent receivers with low-noise performance provide an extremely sensitive, flexible instrument for submillimeter imaging.
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Cited by 4 Pith papers
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Dust transport in envelopes of disk-embedded planets: I. Convectively stable envelopes
In convectively stable envelopes of embedded Earth-like planets, the dust-to-gas ratio falls by 2 to 4 orders of magnitude toward the core, because small grains are blocked by the recycling flow and large grains settl...
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REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths
A uniform reanalysis of 74 resolved millimeter-wave debris belts shows belt dust masses fall with age fastest at small radii, most belts are broad, and vertical thickness shows no age trend.
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Dust transport in envelopes of disk-embedded planets: II. Fully convective envelopes
In fully convective envelopes of disk-embedded planets, dust is retained only when convection reaches the disk flow and grains are small enough to be trapped by convective stirring.
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3D-Herschel: Constraining Dust Emission with Panchromatic Modeling of 3D-HST Galaxies
Using a new deblended Herschel catalog, the authors show that UV-to-mid-infrared SED fits recover the star-forming main sequence but under-predict far-infrared luminosity in low-mass galaxies when fixed dust templates...
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