Add to ORKGThe VST (VLT Survey Telescope) active optics software must basically provide the analysis of the image coming from the wavefront sensor (a 10x10 subpupils Shack Hartmann device) and the calculation of primary mirror forces and secondary mirror displacements to correct the aberrations of the optical system, instrinsic or originated for thermal and gravity reasons. After the telescope commissioning the VST will be operated by ESO. In this framework, INAF-OAC staff was committed to design and realize the software in a VLT-compliant way. This will smoothen the integration, operation and maintenance of the telescope in the Paranal observatory
The Large Synoptic Survey Telescope (LSST) is an 8-meter class wide-field telescope now under constr...
The VLT Survey Telescope (VST) is a co-operative program between the European Southern Observatory (...
The adapter of the VST telescope hosts many devices handled by the overall telescope control softwar...
The VST active optics software must basically provide the analysis of the image coming from the wave...
The 2.6 m VLT Survey Telescope (VST) is going to be installed at Cerro Paranal (Chile) as a powerful...
The VST (VLT Survey Telescope) is a 2.6 m class Alt-Az telescope to be installed at Mount Paranal in...
The VST (VLT Survey Telescope) is a 2.6 m Alt-Az telescope to be installed at Mount Paranal in Chile...
The VLT Survey Telescope (VST) is a cooperative program between the European Southern Observatory (E...
The VST telescope is equipped with an active optics system based on a wavefront sensor, a set of axi...
The 2.6 m VST telescope is going to be installed at Cerro Paranal (Chile) as a powerful instrument f...
The VST (Very Large Telescope Survey Telescope) is an 2.6 m class Alt-Az telescope which will be ins...
The VST (VLT Survey Telescope) is a 2.6m optical ground-based telescope to be installed in the Cerro...
This paper describes the active optics system of the VLT Survey Telescope, the 2.6-m survey telescop...
The VLT Survey Telescope (VST) is a 2.6 m aperture, wide-field (1°1°), UV to I facility, to be insta...
The VST (Very Large Telescope Survey Telescope) is a 2.6 m wide field survey Alt-Az telescope to be ...
The Large Synoptic Survey Telescope (LSST) is an 8-meter class wide-field telescope now under constr...
The VLT Survey Telescope (VST) is a co-operative program between the European Southern Observatory (...
The adapter of the VST telescope hosts many devices handled by the overall telescope control softwar...
The VST active optics software must basically provide the analysis of the image coming from the wave...
The 2.6 m VLT Survey Telescope (VST) is going to be installed at Cerro Paranal (Chile) as a powerful...
The VST (VLT Survey Telescope) is a 2.6 m class Alt-Az telescope to be installed at Mount Paranal in...
The VST (VLT Survey Telescope) is a 2.6 m Alt-Az telescope to be installed at Mount Paranal in Chile...
The VLT Survey Telescope (VST) is a cooperative program between the European Southern Observatory (E...
The VST telescope is equipped with an active optics system based on a wavefront sensor, a set of axi...
The 2.6 m VST telescope is going to be installed at Cerro Paranal (Chile) as a powerful instrument f...
The VST (Very Large Telescope Survey Telescope) is an 2.6 m class Alt-Az telescope which will be ins...
The VST (VLT Survey Telescope) is a 2.6m optical ground-based telescope to be installed in the Cerro...
This paper describes the active optics system of the VLT Survey Telescope, the 2.6-m survey telescop...
The VLT Survey Telescope (VST) is a 2.6 m aperture, wide-field (1°1°), UV to I facility, to be insta...
The VST (Very Large Telescope Survey Telescope) is a 2.6 m wide field survey Alt-Az telescope to be ...
The Large Synoptic Survey Telescope (LSST) is an 8-meter class wide-field telescope now under constr...
The VLT Survey Telescope (VST) is a co-operative program between the European Southern Observatory (...
The adapter of the VST telescope hosts many devices handled by the overall telescope control softwar...