465 research outputs found
Problems in the treatment of malabsorption in CF
ABSTRACT. Several factors play a role in the cause of malabsorption in CF. Besides the enzyme deficiency in the secretion of the exocrine pancreas, decreased bile‐salt concentration in the gut may also be an important factor in the fat malabsorption. The contribution to the fat absorption by other lipases, such as lingual lipase and gastric lipase, remains to he proved. The therapeutic measures are only partly effective because of the breakdown of swalled enzymes by gastric acid. Some improvement is reached by using a new acid‐resistant coating for the enzyme supplement. Newly developed and essential for its success is the application of small coated particles to prevent retention in the stomach, and the easy breakdown of the coating in an alkaline solution. The treatment of the bile salt deficiency has not been successful until now. A trial with additional Tween 80, with the option of supplementing the detergent activity which was found to he successful in Crohn disease, was without marked success. Copyrigh
Moderation in management research: What, why, when and how.
Many theories in management, psychology, and other disciplines rely on moderating variables: those which affect the strength or nature of the relationship between two other variables. Despite the near-ubiquitous nature of such effects, the methods for testing and interpreting them are not always well understood. This article introduces the concept of moderation and describes how moderator effects are tested and interpreted for a series of model types, beginning with straightforward two-way interactions with Normal outcomes, moving to three-way and curvilinear interactions, and then to models with non-Normal outcomes including binary logistic regression and Poisson regression. In particular, methods of interpreting and probing these latter model types, such as simple slope analysis and slope difference tests, are described. It then gives answers to twelve frequently asked questions about testing and interpreting moderator effects
Discovery of VHE Gamma Radiation from IC443 with the MAGIC Telescope
We report the detection of a new source of very high energy (VHE, E_gamma >=
100GeV) gamma-ray emission located close to the Galactic Plane, MAGIC
J0616+225, which is spatially coincident with SNR IC443. The observations were
carried out with the MAGIC telescope in the periods December 2005 - January
2006 and December 2006 - January 2007. Here we present results from this
source, leading to a VHE gamma-ray signal with a statistical significance of
5.7 sigma in the 2006/7 data and a measured differential gamma-ray flux
consistent with a power law, described as dN_gamma/(dA dt dE) = (1.0 +/-
0.2)*10^(-11)(E/0.4 TeV)^(-3.1 +/- 0.3) cm^(-2)s^(-1)TeV^(-1). We briefly
discuss the observational technique used and the procedure implemented for the
data analysis. The results are put in the perspective of the multiwavelength
emission and the molecular environment found in the region of IC443.Comment: Accepted by ApJ Letter
Search for supersymmetric particles in scenarios with a gravitino LSP and stau NLSP
Sleptons, neutralinos and charginos were searched for in the context of
scenarios where the lightest supersymmetric particle is the gravitino. It was
assumed that the stau is the next-to-lightest supersymmetric particle. Data
collected with the DELPHI detector at a centre-of-mass energy near 189 GeV were
analysed combining the methods developed in previous searches at lower
energies. No evidence for the production of these supersymmetric particles was
found. Hence, limits were derived at 95% confidence level.Comment: 31 pages, 14 figure
Cervical Screening within HIV Care: Findings from an HIV-Positive Cohort in Ukraine
HIV-positive women have an increased risk of invasive cervical cancer but cytologic screening is effective in reducing incidence. Little is known about cervical screening coverage or the prevalence of abnormal cytology among HIV-positive women in Ukraine, which has the most severe HIV epidemic in Europe
Observation of Gamma Rays from the Galactic Center with the MAGIC Telescope
Recently, the Galactic Center has been reported to be a source of very high
energy (VHE) gamma-rays by the VERITAS, CANGAROO and HESS experiments. The
energy spectra as measured by these experiments show substantial differences.
In this Letter we present MAGIC observations of the Galactic Center, resulting
in the detection of a differential gamma-ray flux consistent with a steady,
hard-slope power law, described as dN/(dA dt dE) = (2.9+/-0.6)*10^{-12}
(E/TeV)^{-2.2+/-0.2} cm^{-2}s^{-1}TeV^{-1}. The gamma-ray source is centered at
(Ra, Dec)=(17h 45m 20s, -29deg 2'. This result confirms the previous
measurements by the HESS experiment and indicates a steady source of TeV
gamma-rays. We briefly describe the observational technique used, the procedure
implemented for the data analysis, and discuss the results in the perspective
of different models proposed for the acceleration of the VHE gamma-rays.Comment: ApJL submitte
Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303
Microquasars are binary star systems with relativistic radio-emitting jets.
They are potential sources of cosmic rays and laboratories for elucidating the
physics of relativistic jets. Here we report the detection of variable
gamma-ray emission above 100 gigaelectron volts from the microquasar LS I +61
303. Six orbital cycles were recorded. Several detections occur at a similar
orbital phase, suggesting the emission is periodic. The strongest gamma-ray
emission is not observed when the two stars are closest to one another,
implying a strong orbital modulation of the emission or the absorption
processes.Comment: 11 pages with 4 figure
Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303
Microquasars are binary star systems with relativistic radio-emitting jets.
They are potential sources of cosmic rays and laboratories for elucidating the
physics of relativistic jets. Here we report the detection of variable
gamma-ray emission above 100 gigaelectron volts from the microquasar LS I +61
303. Six orbital cycles were recorded. Several detections occur at a similar
orbital phase, suggesting the emission is periodic. The strongest gamma-ray
emission is not observed when the two stars are closest to one another,
implying a strong orbital modulation of the emission or the absorption
processes.Comment: 11 pages with 4 figure
Measurement of Trilinear Gauge Couplings in Collisions at 161 GeV and 172 GeV
Trilinear gauge boson couplings are measured using data taken by DELPHI at 161~GeV and 172~GeV. Values for couplings () are determined from a study of the reactions \eeWW\ and \eeWev, using differential distributions from the final state in which one decays hadronically and the other leptonically, and total cross-section data from other channels. Limits are also derived on neutral couplings from an analysis of the reaction \eegi
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