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Carmen S. Menoni

Researcher at Colorado State University

Publications -  450
Citations -  5718

Carmen S. Menoni is an academic researcher from Colorado State University. The author has contributed to research in topics: Laser & Extreme ultraviolet lithography. The author has an hindex of 33, co-authored 426 publications receiving 4467 citations. Previous affiliations of Carmen S. Menoni include Lebedev Physical Institute & National Science Foundation.

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Crystal data for high-pressure phases of silicon

TL;DR: Crystallographic data are presented in phase I (cubic, diamond), II (tetragonal, ..beta..-Sn), V (simple hexagonal), VII (hexagonal close-packed), and the metastable phase III (body-centered-cubIC (BC8)) and on the coexistence of the phases.
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Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences

Richard J. Abbott, +1695 more
TL;DR: In this article, the authors reported the observation of gravitational waves from two compact binary coalescences in LIGO's and Virgo's third observing run with properties consistent with neutron star-black hole (NSBH) binaries.
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Ultrahigh 22 nm resolution coherent diffractive imaging using a desktop 13 nm high harmonic source

TL;DR: A significant advance in image resolution and capabilities for desktop soft x-ray microscopes that will enable widespread applications in nanoscience and nanotechnology and shows that unique information about the sample can be obtained by extracting 3-D information at very high numerical apertures.
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High numerical aperture tabletop soft x-ray diffraction microscopy with 70-nm resolution

TL;DR: A versatile soft x-ray diffraction microscope with 70- to 90-nm resolution with high numerical aperture imaging and near-diffraction-limited resolution is reported by using two different tabletop coherent softx-ray sources—a soft x -ray laser and a high-harmonic source.
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Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo’s third observing run

Richard J. Abbott, +1681 more
- 15 Jul 2021 - 
TL;DR: In this article, the authors report results of a search for an isotropic gravitational-wave background (GWB) using data from Advanced LIGO's and Advanced Virgo's third observing run (O3) combined with upper limits from the earlier O1 and O2 runs.