Long-term trends in the VLTI auxiliary telescopes and ESO/APEX pointing models
2012
The database of the relocatable VLTI Auxiliary Telescopes was used to study their stability and long-term trends
in their pointing models. The model parameters are functions of mechanical properties of the telescopes and
station pads. The index error in elevation and non-perpendicularity in elevation depend mainly on telescope
characteristics, while the tilt parameters on the pads. After some trends present in 2007-2010 the mechanical
characteristics of all four VLTI 1.8m telescopes are stabilized. Some tilt trends are still present in recently opened
stations, but unlike in APEX, the tilts are not significantly affected by seasonal temperature variations.
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