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pro vyhledávání: '"Michele D. De La Peña"'
Autor:
Michele D. De La Peña, Douglas M. Summers, Joar Brynnel, Douglas Fisher, Christopher Cox, C. Biddick, Stephen R. Hooper, Joseph Kraus, Tom Sargent, John M. Hill, Taras Golota, Christian Veillet, K. Summers
Publikováno v:
SPIE Proceedings.
The LBTO software and IT group was originally responsible for development of the Telescope Control System (TCS) software, and build-out of observatory Information Technology (IT) infrastructure. With major construction phases of the observatory mostl
Autor:
Norm Cushing, Andrew Rakich, Fulvio De Bonis, Michele D. De La Peña, Luca Fini, Jacopo Farinato, Frank Kittmann, Chris Biddick, Harald Baumeister, Carmelo Arcidiacono, Florian Briegel, Maria Bergomi, Simone Esposito, Jörg-Uwe Pott, Al Conrad, A. Brunelli, Lorenzo Busoni, Martin Kuerster, Matthieu Brangier, Xianyu Zhang, Richard F. Green, Lars Mohr, Tom Herbst, Juergen Berwein, Jan Trowitzsch, Ralph Hofferbert, Valentina Viotto, Alfio Puglisi, Ralf-Rainer Rohloff, Werner Laun, Joar Brynnel, Thomas Bertram, Peter Bizenberger, Roberto Ragazzoni, Aleksei Pavlov, Daniel Meschke
Publikováno v:
SPIE Proceedings.
LINC-NIRVANA will employ four wave front sensors to realize multi-conjugate correction on both arms of a Fizeau interferometer for LBT. Of these, one of the two ground-layer wave front sensors, together with its infrared test camera, comprise a stand
Autor:
Michele D. De La Peña, Chris Biddick, Norman J. Cushing, Torsten Leibold, Dave Thompson, John M. Hill
Publikováno v:
SPIE Proceedings.
The software group at the Large Binocular Telescope Observatory (LBTO) 1 used logs and telemetry related to telescope control system behavior to investigate improving the operational efficiency of the telescope. Our investigation unearthed several su
Publikováno v:
SPIE Proceedings.
The Large Binocular Telescope (LBT) consists of two 8.4-meter primary mirrors on a common mount. When the telescope is complete, to complement the two primaries there will be two 0.9-meter adaptive secondaries and two tertiary mirror flats that all w