Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Jess Köhler"'
Publikováno v:
Physica B: Condensed Matter. 253:222-237
Optical and magneto-optical properties of the non-collinear ferromagnet U 3 P 4 are studied theoretically over the broad energy range of 0—12 eV. The calculations are carried out in the framework of the local density functional theory treating the
Publikováno v:
Physical Review B. 55:R10153-R10156
Autor:
Catarina Alves de Oliveira, Bernhard Dorner, Peter Viggo Jakobsen, Marco Sirianni, Xavier Gnata, Pierre Ferruit, Jess Köhler, Guido De Marchi, Torsten Böker, Giovanna Giardino, Stephan M. Birkmann
Publikováno v:
Astronomy & Astrophysics. 592:A113
Context: The NIRSpec instrument for the James Webb Space Telescope (JWST) can be operated in multiobject (MOS), long-slit, and integral field (IFU) mode with spectral resolutions from 100 to 2700. Its MOS mode uses about a quarter of a million indivi
Autor:
Manfred-Georg Kolm, Guido De Marchi, Werner Hupfer, Aurélien Pons, Xavier Gnata, Torsten Böker, Laure Piquéras, Pierre-Jacques Legay, Arlette Pécontal-Rousset, Jess Köhler, P. Ferruit, Stephan M. Birkmann, Emeline Legros, Marco Sirianni, Bernhard Dorner, Ralf Ehrenwinkler, Aurélien Jarno
Publikováno v:
SPIE Proceedings.
The James Webb Space Telescope (JWST) is the successor mission to the Hubble Space Telescope and will operate in the near- and mid-infrared wavelength ranges. One of the four science instruments on board the spacecraft is the multi-object spectrograp
Autor:
Torsten Böker, Robert Lemke, Jess Köhler, Stephan M. Birkmann, Karl Honnen, Bernhard Dorner, Xavier Gnata, Manfred Kolm, Giorgio Bagnasco, Markus Melf, Peter Rumler, Maurice te Plate, Jean-Christophe Salvignol, Peter Viggo Jakobsen, Marc Maschmann, Peter Jensen, Paolo Strada, Marco Sirianni, Jean-Francois Pittet, P. Ferruit, Guido De Marchi
Publikováno v:
SPIE Proceedings.
The Near Infrared Spectrograph (NIRSpec) is one of the four science instruments aboard the James Webb Space Telescope (JWST) scheduled for launch in 2014. NIRSpec is sensitive in the wavelength range from ~ 0.6 to 5.0 μm and will be capable of obtai