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technologies for X-ray, gamma-ray, and particle detection aimed at advancing next-generation gamma-ray imaging, radiation imaging, and spectroscopy technologies for diverse applications in quantum sensing
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group for experimental astroparticle physics of Prof. David Berge at the Humboldt-Universität zu Berlin is engaged in the gamma-ray telescope system H.E.S.S., preparations for the CTAO gamma-ray
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range of sol-gel and electrochemical deposition methods. The successful candidate will also carry out a range of X-ray characterisation methods, including Bragg, small angle and reflectivity methods
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Center for Astrophysics | Harvard & Smithsonian | Cambridge, Massachusetts | United States | about 21 hours ago
, the Magellan Telescopes in Chile, and the Submillimeter Array in Hawai’i. Fellows participate in ground- and space-based observing programs including but not limited to the Chandra X-ray Observatory, the Event
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strongly preferred. Candidates should be proficient in micro-computed tomography (micro-CT) imaging and analysis. Experience performing mouse surgery is preferred. A demonstrated publication record and
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. Working closely with Professor Gregory Warr and his team, the successful candidate will have experience in the design, execution and analysis of neutron and X-ray small-angle scattering experiments
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coherent plan for the duration of the appointment of research expected to make a valuable contribution to the candidate’s field is required, as well as evidence of active participation in the successful
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multimodal workflow on integrating hyperspectral imaging, X-ray fluorescence, and RGB images. You will be given ample opportunity to apply for funding and grants in collaboration with Naturalis researchers and
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-qualification experience. Applicants are invited to contact Mr Rai Yiu at telephone number 2766 6043 or via email at [email protected] for further information. Conditions of Service For full-time appointment(s
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-resolution imaging at the micron scale remains hindered by limitations imposed by its sub-millimeter wavelengths [1 THz ~ 300 µm]. This necessitates the need to transcend the diffraction limit of THz waves