2,629 research outputs found
A computer operated mass spectrometer system
Digital computer system for processing mass spectrometer output dat
C*-Structure and K-Theory of Boutet de Monvel's Algebra
We consider the norm closure of the algebra of all operators of order and
class zero in Boutet de Monvel's calculus on a manifold with boundary .
We first describe the image and the kernel of the continuous extension of the
boundary principal symbol to . If the is connected and is not empty,
we then show that the K-groups of are topologically determined. In case the
manifold, its boundary and the tangent space of the interior have torsion-free
K-theory, we prove that is isomorphic to the direct sum of
and , for i=0,1, with denoting the compact
ideal and the tangent bundle of the interior of . Using Boutet de
Monvel's index theorem, we also prove this result for i=1 without assuming the
torsion-free hypothesis. We also give a composition sequence for .Comment: Final version, to appear in J. Reine Angew. Math. Improved
K-theoretic result
Environmental metabolomics : databases and tools for data analysis
© The Author(s), 2015. This article is distributed under the terms of the Creative Commons Attribution License. The definitive version was published in Marine Chemistry 177 (2015): 366–373, doi:10.1016/j.marchem.2015.06.012.Metabolomics is the study of small molecules, or ‘metabolites’, that are the end products of biological processes. While -omics technologies such as genomics, transcriptomics, and proteomics measure the metabolic potential of organisms, metabolomics provides detailed information on the organic compounds produced during metabolism and found within cells and in the environment. Improvements in analytical techniques have expanded our understanding of metabolomics and developments in computational tools have made metabolomics data accessible to a broad segment of the scientific community. Yet, metabolomics methods have only been applied to a limited number of projects in the marine environment. Here, we review analysis techniques for mass spectrometry data and summarize the current state of metabolomics databases. We then describe a boutique database developed in our laboratory for efficient data analysis and selection of mass spectral targets for metabolite identification. The code to implement the database is freely available on GitHub (https://github.com/joefutrelle/domdb). Data organization and analysis are critical, but often under-appreciated, components of metabolomics research. Future advances in environmental metabolomics will take advantage of continued development of new tools that facilitate analysis of large metabolomics datasets.The field data populating the database comes from scientific cruises funded by grants from the National Science Foundation to EBK and KL (Atlantic Ocean, OCE-1154320) and E.V. Armbrust (Pacific Ocean, OCE-1205233). The laboratory experiment with coastal seawater was funded by a grant from the Gulf of Mexico Research Initiative to EBK and H.K. White. The laboratory experiments with microbial isolates and the database development are funded by the Gordon and Betty Moore Foundation through Grant GBMF3304 to EBK
Development of the combined method of hardening of the surface of aluminium
Представлены результаты, полученные при исследовании фазового и элементного состава, дефектной субструктуры поверхности технически чистого алюминия марки А7, подвергнутого комбинированной обработке, сочетающей напыление металлической пленки, электронно-пучковое перемешивание системы пленка/подложка и последующее азотирование в плазме газового разряда низкого давления. Выполнен анализ закономерностей, выявлены режимы воздействия, позволяющие кратно повышать микротвердость и износостойкость материала.The results are presented, received at research of phase and elemental composition, defective substructureof surface technically pure aluminium of the A7, subjected to the combined processing combining spraying metalfilm, electron-beam mixing of system film/substrate and subsequent nitriding in plasma of the gas discharge of lowpressure. The analysis of regularities is made, revealed the modes of influence allowing multiple to raise amicrohardness and wear resistance of material
Ten per cent polarized optical emission from GRB 090102
The nature of the jets and the role of magnetic fields in gamma-ray bursts
(GRB) remains unclear. In a baryon-dominated jet only weak, tangled fields
generated in situ through shocks would be present. In an alternative model,
jets are threaded with large scale magnetic fields that originate at the
central engine and which accelerate and collimate the jets. The way to
distinguish between the models is to measure the degree of polarization in
early-time emission, however previous claims of gamma-ray polarization have
been controversial. Here we report that the early optical emission from GRB
090102 was polarized at the level of P=10+/-1%, indicating the presence of
large-scale fields originating in the expanding fireball. If the degree of
polarization and its position angle were variable on timescales shorter than
our 60-s exposure, then the peak polarization may have been larger than 10 per
cent.Comment: 16 pages, 4 figures. Published in Nature (2009), Vol. 462, p767-76
Mixing Quantum and Classical Mechanics
Using a group theoretical approach we derive an equation of motion for a
mixed quantum-classical system. The quantum-classical bracket entering the
equation preserves the Lie algebra structure of quantum and classical
mechanics: The bracket is antisymmetric and satisfies the Jacobi identity, and,
therefore, leads to a natural description of interaction between quantum and
classical degrees of freedom. We apply the formalism to coupled quantum and
classical oscillators and show how various approximations, such as the
mean-field and the multiconfiguration mean-field approaches, can be obtained
from the quantum-classical equation of motion.Comment: 31 pages, LaTeX2
Diffuse Galactic Soft Gamma-Ray Emission
The Galactic diffuse soft gamma-ray (30-800 keV) emission has been measured
from the Galactic Center by the HIREGS balloon-borne germanium spectrometer to
determine the spectral characteristics and origin of the emission. The
resulting Galactic diffuse continuum is found to agree well with a single
power-law (plus positronium) over the entire energy range, consistent with RXTE
and COMPTEL/CGRO observations at lower and higher energies, respectively. We
find no evidence of spectral steepening below 200 keV, as has been reported in
previous observations. The spatial distribution along the Galactic ridge is
found to be nearly flat, with upper limits set on the longitudinal gradient,
and with no evidence of an edge in the observed region. The soft gamma-ray
diffuse spectrum is well modeled by inverse Compton scattering of interstellar
radiation off of cosmic-ray electrons, minimizing the need to invoke
inefficient nonthermal bremsstrahlung emission. The resulting power requirement
is well within that provided by Galactic supernovae. We speculate that the
measured spectrum provides the first direct constraints on the cosmic-ray
electron spectrum below 300 MeV.Comment: 26 pages, 7 figure, submitted to Ap
The 1999 Hercules X-1 Anomalous Low State
A failed main-on in the 35d cycle of Her X-1 was observed with the Rossi
X-Ray Timing Explorer (RXTE) on 1999 April 26. Exceptions to the normal 35d
cycle have been seen only twice before; in 1983 and again 1993. We present
timing and spectral results of this latest Anomalous Low State (ALS) along with
comparisons to the main-on and normal low states. Pulsations were observed in
the 3-18 keV band with a fractional RMS variation of (0.037+-0.003). Spectral
analysis indicates that the ALS spectrum has the same shape as the main-on but
is modified by heavy absorption and scattering. We find that 70% of the
observed emission has passed through a cold absorber (N_H=5.0x10^{23}cm^{-2}).
This partially absorbing spectral fit can be applied to the normal low state
with similar results. We find that the ALS observations may be interpreted as a
decrease in inclination of the accretion disk causing the central X-Ray source
to be obscured over the entire 35d cycle.Comment: revised text, 6 revised figures, accepted for publication in Ap
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