
Proceedings Paper
Development of different kind of IFU prototypes for the OPTIMOS-EVE study for the E-ELTFormat | Member Price | Non-Member Price |
---|---|---|
$17.00 | $21.00 |
Paper Abstract
The OPTIMOS-EVE concept provides optical to near-infrared (370-1700 nm) spectroscopy, with three spectral
resolution (5000, 15000 and 30000), with high simultaneous multiplex (at least 200). The optical fibre links are
distributed in four kinds of bundles: several hundreds of mono-object systems with three types of bundles, fibre size
being used to adapt spectral resolution and 30 deployable medium IFUs (about 2"x3"). We are optimising the design of
deployable IFUs to warrant sky subtraction for the faintest extragalactic sources.
This paper gives the design and results of the prototype for the high resolution mode and the preliminary design of a
medium IFU developed in collaboration between the GEPI and the LNA.
Paper Details
Date Published: 13 September 2012
PDF: 7 pages
Proc. SPIE 8450, Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II, 84503G (13 September 2012); doi: 10.1117/12.924812
Published in SPIE Proceedings Vol. 8450:
Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II
Ramón Navarro; Colin R. Cunningham; Eric Prieto, Editor(s)
PDF: 7 pages
Proc. SPIE 8450, Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II, 84503G (13 September 2012); doi: 10.1117/12.924812
Show Author Affiliations
Isabelle Guinouard, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Ligia Souza de Oliviera, Lab. Nacional de Astrofísica (Brazil)
Antonio César de Oliveira, Lab. Nacional de Astrofísica (Brazil)
François Hammer, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Marc Huertas-Company, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Beatriz Barbuy, Univ. de São Paulo (Brazil)
Ligia Souza de Oliviera, Lab. Nacional de Astrofísica (Brazil)
Antonio César de Oliveira, Lab. Nacional de Astrofísica (Brazil)
François Hammer, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Marc Huertas-Company, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Beatriz Barbuy, Univ. de São Paulo (Brazil)
Fanny Chemla, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Jean-Michel Huet, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Hector Flores, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Mathieu Puech, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Simona Mei, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Jean-Michel Huet, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Hector Flores, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Mathieu Puech, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Simona Mei, Observatoire de Paris, CNRS, Univ. Paris Diderot (France)
Published in SPIE Proceedings Vol. 8450:
Modern Technologies in Space- and Ground-based Telescopes and Instrumentation II
Ramón Navarro; Colin R. Cunningham; Eric Prieto, Editor(s)
© SPIE. Terms of Use
