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Compilation of Technical Papers on ALMA Receivers
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The Atacama Large Millimeter/submillimeter Array (ALMA) is the world's leading instrument for high-resolution imaging of the 0.3 to 10 mm wavelength sky. This interferometer exemplifies successful international collaboration even down to its individual components, including its telescope dishes and receivers produced in global partnerships. Over the past roughly ten years of ALMA operation, these receivers have been responsible for nearly ten thousand publications, as carefully monitored by the online ALMA Science Archive. However, the citations of the relevant receiver papers have not managed to grow together with their use in the astronomical community, which points out an information gap among the astronomical community. To overcome this gap, this memo provides a comprehensive list of receiver references, which was created in direct contact with the receiver groups.
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RIOJA. JWST and ALMA unveil the inhomogeneous and complex ISM structure in a star-forming galaxy at $z=6.81$
For the z=6.81 galaxy COS-2987, [OIII] line ratios from JWST and ALMA rule out a single-component ionized gas and favor a two-phase ISM with a compact dense component and an extended diffuse component.
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