Fig. 2
Predicted rotational spectrum of methoxyamine at the temperature of 120 K and its overlap with approximate frequency coverage of several astrophysical facilities (IRAM: Institut de Radioastronomie Millimétrique; HERSCHEL/HIFI: Herschel-Heterodyne Instrument for the Far-Infrared; GBT: Green Bank Telescope; APEX: Atacama Pathfinder Experiment telescope; ALMA: Atacama Large Millimeter/submillimeter Array; ARO: Arizona Radio Observatory; JCMT: James Clerk Maxwell Telescope; CARMA: Combined Array for Research in Millimeter-wave Astronomy). The frequency region studied in this work is highlighted in gray.
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