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#1Andreas Erik Gejl Madsen (University of Southern Denmark)
#2René Lynge EriksenH-Index: 15
Last. Jesper GlückstadH-Index: 30
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Computer Generated Holography (CGH) promises unprecedented capabilities for a variety of applications in Optics and Photonics. However, one of the biggest challenges for CGHs is the fundamental tradeoff between algorithm runtime and achieved reconstruction fidelity and efficiency while maintaining light projections at real-time frame rates. In addition, the light projection quality achieved by most CGH-modalities are rather low due to the mismatch between the optical wave propagation of the appl...
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#1Jonathan PradellesH-Index: 8
#2L. Perraud (UGA: University of Grenoble)H-Index: 2
Last. Patrick SchiavoneH-Index: 14
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2D curvilinear patterns are more and more present in the lithography landscape. For the related devices, the line edge roughness (LER) is, as well as for lines and spaces, a critical figure of merit. In this article we propose to use a dedicated edge detection algorithm to measure LER of 2D curvilinear patterns on CD-SEM images. We present an original method to validate the algorithm, in the context of roughness measurement. It is based on the generation of realistic synthetic CD-SEM images with...
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#2Jack H. NobleH-Index: 29
Last. Matthieu ChabanasH-Index: 12
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During tumor resection surgery, intraoperative ultrasound images of the brain show anatomical structures like the sulci , falx cerebri and tentorium cerebelli , as well as the tumor. After resection started, the resection cavity is also visible. These elements help with the localization and tumor resection, and can be used to register the preoperative MRI to intraoperative images, to compensate for the tissue deformation occurring during surgery. In this work, we compare single-and multi-class s...
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#1Mélanie Donnez (UGA: University of Grenoble)
Last. Matthieu Chabanas (UGA: University of Grenoble)H-Index: 12
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The simulation of realistic ultrasound (US) images has many applications in image-guided surgery such as image registration, data augmentation, or educational purposes. In this paper we simulated intraoperative US images of the brain after tumor resection surgery. In a first stage, a Generative Adversarial Networks generated an US image with resection from a resection cavity map. While the cavity texture can be realistic, surrounding structures are usually not anatomically coherent. Thus, a seco...
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#1Tamara Dupuy (UGA: University of Grenoble)
Last. Sandrine Voros (UGA: University of Grenoble)H-Index: 16
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The accuracy of biopsy sampling and the related tumor localization are major issues for prostate cancer diagnosis and therapy. However, the ability to navigate accurately to biopsy targets faces several difficulties coming from both transrectal ultrasound (TRUS) image guidance properties and prostate motion or deformation. To reduce inaccuracy and exam duration, the main objective of this study is to develop a real-time navigation assistance. The aim is to provide the current probe position and ...
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#1Qiang Wang (Edin.: University of Edinburgh)H-Index: 27
#1Qiang Wang (Edin.: University of Edinburgh)H-Index: 7
Last. Marta VallejoH-Index: 5
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Deep learning technologies have been successfully applied to automatic diagnostics of ex-vivo lung cancer with fluorescence lifetime imaging endomicroscopy (FLIM). Recent advance in convolutional neural networks (CNNs) by splitting input features for multi-scale feature extraction as a feature-level aggregation, has achieved further improvement in visual recognition. However, due to the splitting, correlations among input features are no longer retained. To exploit the advantages of hierarchical...
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#1Masashi Hazumi (KEK)H-Index: 104
#2Peter A. R. Ade (Cardiff University)H-Index: 178
Last. Andrea Zonca (UCSD: University of California, San Diego)H-Index: 148
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In May 2019, LiteBIRD was selected as JAXA’s strategic L-class satellite #2 targeting a launch in 2020s with a H3 rocket. Its mission is to map the polarization of the cosmic microwave background (CMB) over the full sky at large angular scales with unprecedented precision. LiteBIRD will allow us to make a crucial test of cosmic inflation and quantum gravity theories behind it. It will also provide us with valuable information on astrophysics. Full-sky surveys for three years at a Lagrangian poin...
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#1Kenji Kiuchi (UTokyo: University of Tokyo)H-Index: 5
#2Shunsuke Adachi (Kyoto University)H-Index: 73
Last. Ningfeng Zhu (UPenn: University of Pennsylvania)H-Index: 14
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The Simons Observatory (SO) will be a cosmic microwave background (CMB) survey experiment with three small-aperture telescopes (SATs) and one large-aperture telescope (LAT), which will observe from the Atacama Desert in Chile. In total, SO will field over 60,000 transition-edge sensor (TES) bolometers in six spectral bands centered between 27 and 280 GHz in order to achieve the sensitivity necessary to measure or constrain numerous cosmological quantities. The SATs are optimized for a primordial...
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#1Yutaro Sekimoto (UTokyo: University of Tokyo)H-Index: 19
#1Yutaro Sekimoto (UTokyo: University of Tokyo)H-Index: 18
Last. A. Zonca (UCSD: University of California, San Diego)H-Index: 67
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LiteBIRD has been selected as JAXA’s strategic large mission in the 2020s, to observe the cosmic microwave background (CMB) B-mode polarization over the full sky at large angular scales. The challenges of LiteBIRD are the wide field-of-view (FoV) and broadband capabilities of millimeter-wave polarization measurements, which are derived from the system requirements. The possible paths of stray light increase with a wider FoV and the far sidelobe knowledge of -56 dB is a challenging optical requir...
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#1Julien Girard (STScI: Space Telescope Science Institute)H-Index: 63
#2Sebastiaan Y. Haffert (UA: University of Arizona)H-Index: 3
Last. Christoph U. KellerH-Index: 46
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We present recent results obtained with the VLT/MUSE Integral Field Spectrograph fed by the 4LGSF and its laser tomography adaptive optics module GALACSI. While this so-called narrow-field mode of MUSE was not designed to perform directly imaging of exoplanets and outflows, we show that it can be a game changer to detect and characterize young exoplanets with a prominent emission lines (i.e Hα, tracer of accretion), at moderate contrasts. These performances are achieved thanks to the combo of a ...
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