Results 181 to 190 of about 5,123 (230)
Chiral Magnon Dynamics in a Kitaev Magnet Revealed by Magneto-Optics
Bachar N +15 more
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A hot white dwarf merger remnant revealed by an ultraviolet detection of carbon. [PDF]
Sahu S +9 more
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Observation of Localized Resonant Phonon Polaritons in Biaxial α-MoO<sub>3</sub> Nanoparticles. [PDF]
Beitner D +7 more
europepmc +1 more source
Bolometers for far-infrared and submillimetre astronomy
Department of Physics, Queen Mary and Westfield College, Mile End Road, London E1 4NS, UK Received 31 August 1999; Available online 19 April 2000. Abstract Important scientific goals of far-infrared and submillimetre astronomy include measurements of anisotropies in the cosmic background radiation, deep imaging surveys for detection of high-red ...
M J Griffin
exaly +3 more sources
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SPICA mission for mid- and far-infrared astronomy
Proceedings of SPIE, 2008SPICA (Space Infrared Telescope for Cosmology and Astrophysics) is an astronomical mission optimized for mid- and far-infrared astronomy with a cryogenically cooled 3.5 m telescope. Its high spatial resolution and unprecedented sensitivity in the mid- and far-infrared will enable us to address a number of key problems in present-day astronomy ...
Takao Nakagawa
exaly +2 more sources
Development of GaAs photoconductors for far-infrared/submillimeter astronomy
SPIE Proceedings, 2004In today's Astronomy, there is little observational results in the spectral window ranging from far-infrared to submillimeter wavelength. As one of the main reason of this, there is no high performance detector in this spectral region. We started the development of the extrinsic photoconductor for this region utlizing shallow donor levels of gallium ...
Kentaroh Watanabe, Moriaki Wakaki
exaly +2 more sources
GaAs BIB photodetector development for far-infrared astronomy
SPIE Proceedings, 2004GaAs photoconductive detectors offer an extended spectral response in the far-infrared (FIR) compared to presently available stressed Ge photoconductors. Furthermore, responsivity at wavelengths up to 330 microns can be reached without having to apply uniaxial stress close to the breaking limit on each pixel.
N M Haegel +2 more
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New balloon-borne telescope for far-infrared astronomy
SPIE Proceedings, 2000We have developed the new balloon-borne telescope, Far Infrared Balloon-Borne Experiment (FIRBE), to survey the far-infrared radiations of star-forming regions. The primary mirror is an offset parabolid with a diameter of 50 cm (F/2) and telescope structure is made from Carbon Fiber Reinforced Plastics to lighten the whole telescope and hold the strain
H Shibai, Mitsunobu Kawada, Yasuo Doi
exaly +2 more sources

