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SPIE-Int. Soc. Optical Engineering |
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Lucarelli, F. ; Antoranz Canales, Pedro ; Barrio Uña, Juan Abel ; Miranda Pantoja, José Miguel ; Fonseca González, Mª Victoria | SPIE-Int. Soc. Optical Engineering | 2005In this work we have built an electro-optical system for the transmission of low frequency analogue signals through optical fibre. The main goal was to achieve minimum pulse distortion with maximum dynamic range. The system has been used in the [...]texto impreso
Barrio Uña, Juan Abel ; Contreras González, José Luis ; Miranda Pantoja, José Miguel ; López Moya, Marcos ; Tejedor Álvarez, Luis Ángel | SPIE-Int. Soc. Optical Engineering | 2014The Large Size Telescopes, LSTs, located at the center of the Cherenkov Telescope Array, CTA, will be sensitive for low energy gamma-rays. The camera on the LST focal plane is optimized to detect low energy events based on a high photon detectio[...]texto impreso
Martínez-Delgado, I. ; Sánchez-Blanco, E. ; Pérez-Calpena, A. ; García-Vergasa, M.L. ; Maldonado, X.M. ; Gil de Paz, Armando ; Carrasco, E. ; Gallego Maestro, Jesús ; Iglesias-Páramo, J. ; Sánchez Moreno, F.M. ; MEGARA, Team | SPIE-Int. Soc. Optical Engineering | 2016-07-22MEGARA is a third generation spectrograph for the Spanish 10.4m telescope (GTC) providing two observing modes: a large central Integral Field Unit (IFU), called the Large Compact Bundle (LCB), covering a FOV of 12.5 × 11.3 arcsec^(2) , and a Mul[...]texto impreso
Antoranz Canales, Pedro ; Miranda Pantoja, José Miguel ; Fonseca González, Mª Victoria | SPIE-Int. Soc. Optical Engineering | 2005A simple and cost-effective integrated synthesizer of fast light pulses has been designed, analyzed and tested for the characterization of the time response of photo-multipliers (PMT). This synthesizer consists of an integrated pulse generator b[...]texto impreso
Barrio Uña, Juan Abel ; Contreras González, José Luis ; López Moya, Marcos ; Miranda Pantoja, José Miguel ; Tejedor Álvarez, Luis Ángel | SPIE-Int. Soc. Optical Engineering | 2014The Cherenkov Telescope Array (CTA) project aims to implement the world’s largest next generation of Very High Energy gamma-ray Imaging Atmospheric Cherenkov Telescopes devoted to the observation from a few tens of GeV to more than 100 TeV. To v[...]