Zobrazeno 1 - 10
of 31
pro vyhledávání: '"E. Gubbini"'
Autor:
E. Gubbini, Jennifer Kaminski, A. Mecsaci, Frank Grupp, K. Gawlik, A. Mottaghibonab, D. Penka, M. Dubowy, Hans Thiele
Publikováno v:
International Conference on Space Optics — ICSO 2018.
The Euclid payload features two instruments that are observing the sky simultaneously. The visual light high spatial resolution imager (VIS) and the Near Infrared Spectrometer and Photometer (NISP). A Korsch type telescope with 1,2m diameter feeds bo
Autor:
B. Hilber, B. Kusch, A. Mottaghibonab, M. Gerstmeier, T. Sedlmaier, Christof Bodendorf, E. Gubbini, D. Penka, Hans Thiele, A. Mecsaci, Frank Grupp, M. Vongehr, H. Gebler, C. Wimmer, A. Meister, Reinhard O. Katterloher, A. Bode, N. Geis, Ralf Bender, A. Boesz, C. Gal, T. Leberle
Publikováno v:
International Conference on Space Optics — ICSO 2014.
The Near-Infrared Spectrometer and Photometer (NISP) is one of the key instruments on-board the Euclid satellite, one of the major mission of ESA’s 2015 Cosmic Vision program. The instrument is located at the payload of the Euclid satellite, and it
Autor:
M. Dubowy, E. Gubbini, M. Vongehr, Frank Grupp, Hans Thiele, D. Penka, C. Wimmer, Ralf Bender, K. Gawlik, C. Gal, A. Mottaghibonab, A. Mecsaci
Publikováno v:
SPIE Proceedings.
The Near Infrared Spectro-Photometer Optical assembly (NIOA) of EUCLID satellite requires high precision large lens holders with different lens materials, shapes and diameters. The aspherical lenses are glued into their separate CTE matched lens hold
Autor:
A. Bode, C. Wimmer, Hans Thiele, A. Mecsaci, Ralf Bender, A. Meister, K. Gawlik, A. Mottaghibonab, A. Kuisl, M. Dubowy, E. Gubbini, Frank Grupp, C. Gal
Publikováno v:
SPIE Proceedings.
The Near Infrared Spectrometer and Photometer (NISP) of the EUCLID satellite project encompasses high precision large lens mounts of 168 mm diameter that are operated at cryogenic temperatures down to 135K. The four lenses of the optical system are m
Publikováno v:
Journal of Physics B: Atomic, Molecular and Optical Physics. 39:S381-S387
We have investigated atomic ionization dynamics in krypton with circularly polarized light from a Ti-Sapphire laser in the intensity regime between 1016 W cm−2 and 1018 W cm−2. We have measured the yields of highly charged ions stemming from the
Publikováno v:
Journal of Physics B: Atomic, Molecular and Optical Physics. 38:L87-L93
We have studied the ionization process of Kr atoms in strong laser fields by measuring the laser intensity dependence of highly charged ion yields. The measurements have been performed in an intensity regime between 1016 W cm−2 and 1018 W cm−2, w
Autor:
W. Sandner, U. Eichmann, F. Eggenstein, H. Schönagel, E. Gubbini, M Schnürer, G. Reichardt, G. Kommol, M.P. Kalashnikov, Peter V. Nickles
Publikováno v:
Vacuum. 76:45-49
Terawatt laser systems are affected by the problem that optical components, typically installed in vacuum, get contaminated with carbon. In this paper, we describe an “on-line” cleaning system, based on a radiofrequency discharge, to avoid carbon
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 78:657-662
In this paper new measurements of physical properties of high resistivity silicon used in high-energy detectors are presented. The obtained data contribute to the understanding of the causes which produce damage of the electronic characteristics of t
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 426:477-485
In this paper, new measurements of physical properties of high-resistivity silicon, used in high-energy detectors, are presented. The obtained data contribute to the understanding of the causes which damage the electronic characteristics of the detec
Autor:
A. Aleksandrov, S. Busch, S.T. Avetisyan, M.P. Kalachnikov, H. Schonnagel, A. Kudryaschov, P. V. Nickles, Matthias Schnürer, E. Gubbini, U. Eichmann
Publikováno v:
2003 Conference on Lasers and Electro-Optics Europe (CLEO/Europe 2003) (IEEE Cat. No.03TH8666).
The quality of the laser beam wave front is one of the most important parameters limiting the laser intensity available for laser-matter interactions. Application of an adaptive mirror can substantially improve the wave front parameters, thus increas