  The Stellar Observations Network Group prototype telescope at the Teide
Observatory has been operating in scientific mode since March 2014. The first
year of observations has entirely been carried out using the high resolution
echelle spectrograph. Several asteroseismic targets were selected for
scientific and technical verification. A few bright subgiants and one red giant
were chosen since the oscillations in these stars have large amplitudes and the
periods long enough to easily be detected. These targets would also be used for
evaluation of the instruments since long term observations of single targets
would reveal potential problems. In this paper the performance of the first
robotic SONG node is described to illustrate the efficiency and possibilities
in having a robotic telescope.
