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Autor:
Yus, Jorge F. García, Dent, Bill, Brisbin, Drew, Chang, Chin-Shin, Gómez, Laura, Nakos, Theodoros
Publikováno v:
SPIE 11449, Observatory Operations: Strategies, Processes, and Systems VIII, 114491U (17 December 2020)
After eight observing Cycles, the Atacama Large Millimeter-submillimeter Array (ALMA) is capable of observing in eight different bands (covering a frequency range from 84 to 950 GHz), with 66 antennas and two correlators. For the current Cycle (7), A
Externí odkaz:
http://arxiv.org/abs/2101.03427