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We show that, adopting our cross section database, we are able to provide a good fit of a complete sample of CR observables, including: leptonic and hadronic spectra measured at Earth, the local interstellar spectra measured by Voyager, and the gamma-ray emissivities from Fermi-LAT collaboration.
The same group recently reported a similar cross section database of ∼200 lipids measured via TWIMS, exhibiting better than 3% interlaboratory reproducibility for over 98% of the database composition.
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While the majority of applications of TWIMS has utilized the ion mobility as an analytical separation, some efforts have been made on developing TWIMS-derived collision cross section databases to facilitate the use of ion mobility measurements for identification and characterization purposes.
NIST currently has three databases available: an XPS Database, an Electron Elastic-Scattering Cross-Section Database, and an Electron Inelastic-Mean-Free-Path Database.
We explore this relationship using a cross-section database of households in the city of Granada, distinguishing between electrical and non-electrical water-saving appliances.
Unfortunately, our cross-section database does not allow us to adequately address the potential endogeneity bias from a statistical point of view.
The high-throughput and high precision associated with this instrument has facilitated the development of a large nitrogen-based collision cross-section database.
We also refer to the seismic cross-section databases (ERI, 2006; JAMSTEC, 2006).
The purpose of this work is to develop methodologies for adapting the feed-back model for multiparameter cross-section databases of codes DRAGON and DONJON to dynamic core heterogeneity.
Complementary with existing collision cross-section databases reporting uniform-field measurements in helium and nitrogen gas, the combined result of these efforts will facilitate the use of ion mobility measurement toward analyte classification and identification purposes.
The total mass attenuation coefficients have been calculated at energies from 10 keV to 1 GeV using the XCOM (version 3.1) computer program and cross- section database for elements from Z=1 to 100.
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