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on their morphology. A step to optimise the image processing parameters, which will help to obtain average 2D classes, will then be necessary. Subsequently, it will be possible to verify the quality of the 2D classes
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photoluminescence imaging (HMSPL) to detect and study previously unrecognized anatomical and chemical contrasts that enable better identification of the whole or partial specimens analyzed. - Data processing and
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galaxies. VIEWS leverages the capabilities of the James Webb Space Telescope cycle 3 project GO5018 to provide high-resolution imaging and spectroscopy of six selected Brightest Cluster Galaxies. Two
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four main objectives: - Design and fabricate foam-bonded granular materials, by controlling formulation parameters, shaping processes, and binder solidification. - Characterize the microstructure
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/ constrain their planetary systems , (ii) analyse the spectropolarimetric data with Zeeman-Doppler imaging (ZDI) to reconstruct the evolving stellar magnetic topologies and characterize the underlying dynamo
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data storage, enabling the encoding of text, images, videos, and more into nucleotide sequences. While DNA data storage technologies are advancing rapidly, computation on large DNA-encoded databases
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unprecedented precision. - Procedures on rodents, such as: stereotactic brain surgery, cochlear injections, tissue sampling, tagging, etc. - Immunohistochemistry - Confocal imaging - Image analysis and 3D