A view of the control room, two PCs are used, the one on the left to control the wheather station and the one on the right, controlling the telescope, camera and focuser as well as the dome's slit.
The 40cm RCT F10 telescope with the focuser, adaptive optics and camera attached.
Photos : José Ramón Camblor.
One of the observatoruy goals is to achieve the lowest possible residuals in the astrometric and photometric observations, the MPC publishes the number statistics of astrometric observations per observatory and year, below you can see the graph of these, with a very clear tendency towards minimum dispersion, in the year 2010 the dispersion was +/-034 arc seconds in RA and +/-0.35 in DEC which seems to be near the limits imposed by the average atmospheric seeing of the location.
