All Tables

Table 1: Spectroscopic parameters^a (MHz) of amino acetonitrile.
Table 3: Transitions of amino acetonitrile detected toward Sgr B2(N) with the IRAM 30 m telescope.
Table 4: Parameters of our best-fit LTE model of amino acetonitrile.
Table 5: Measurements obtained toward Sgr B2(N) with the IRAM Plateau de Bure interferometer at 82 GHz.
Table 6: Peak positions of continuum and molecular line emission detected with the PdBI and the ATCA toward Sgr B2(N).
Table 7: Measurements obtained toward Sgr B2(N) with the Australia Telescope Compact Array at 91 GHz.
Table 2: Transitions of amino acetonitrile observed with the IRAM 30 m telescope toward Sgr B2(N). The horizontal lines mark discontinuities in the observed frequency coverage. All lines with $S\mu ^2$ < 20 D² are not listed, since they are expected to be much too weak to be detectable with our sensitivity.