287 research outputs found
QUALITY OF LIFE OF PATIENTS WITH METABOLIC SYNDROME IS IMPROVED AFTER WHOLE BODY VIBRATION EXERCISES
Background: Whole body vibration exercises (WBVE) improve the quality of life (QoL) of different populations.
Metabolic syndrome patients (MetS) may be favored by physical activity. Questionnaires are used to assess the QoL.
The aim was to evaluate the QoL of patients with MetS that have undergone WBVE with a brief WHOQOL
(WHOQOL-BREF).
Material and Methods: MetS patients were randomly divided into three groups: (i) control group (CG), (ii) treated
with WBVE once per week (WBVE1) and (iii) treated with WBVE twice per week (WBVE2). In the first session, the
patient was sat in a chair in front of the platform with the feet on its base in 3 peak to peak displacements (2.5, 5.0 and
7.5 mm) and frequency of 5 Hz was used. From the second to the last session, patients were subjected to the same
protocol, however they were standing on the base of the platform and the frequency was increased up to 14 Hz. The
patients fulfilled the WHOQOL-BREF before the first and after the last sessions. Cronbach coefficients were
determined to each domain of the WHOQOL-BREF and test Wilcoxon (
Characterising the KMP-11 and HSP-70 recombinant antigens' humoral immune response profile in chagasic patients
11 pages, 6 figures.-- The pre-publication history for this paper can be accessed
here:
http://www.biomedcentral.com/1471-2334/9/186/pre
pubBackground: Antigen specificity and IgG subclass could be significant in the natural history of
Chagas' disease. The relationship between the different stages of human Chagas' disease and the
profiles of total IgG and its subclasses were thus analysed here; they were directed against a crude
T. cruzi extract and three recombinant antigens: the T. cruzi kinetoplastid membrane protein-11
(rKMP-11), an internal fragment of the T. cruzi HSP-70 protein192-433, and the entire Trypanosoma
rangeli HSP-70 protein.
Methods: Seventeen Brazilian acute chagasic patients, 50 Colombian chronic chagasic patients (21
indeterminate and 29 cardiopathic patients) and 30 healthy individuals were included. Total IgG and
its subtypes directed against the above-mentioned recombinant antigens were determined by
ELISA tests.
Results: The T. cruzi KMP-11 and T. rangeli HSP-70 recombinant proteins were able to distinguish
both acute from chronic chagasic patients and infected people from healthy individuals. Specific
antibodies to T. cruzi crude antigen in acute patients came from IgG3 and IgG4 subclasses whereas
IgG1 and IgG3 were the prevalent isotypes in indeterminate and chronic chagasic patients. By
contrast, the specific prominent antibodies in all disease stages against T. cruzi KMP-11 and T. rangeli
HSP-70 recombinant antigens were the IgG1 subclass.This work was supported by Colciencias Research project No. 1203-333-
18692. IDF was supported by Colciencias and the Universidad Javeriana's
Young Researcher 2008 Programme (BogotĂĄ, Colombia). MCT and MCL
were supported by P06-CTS-02242 Grant from PAI (Junta de Andalucia)
and RICET-RD06/0021-0014, Spain. MS received financial support from the
Brazilian agency - CNPq.Peer reviewe
Measurement of the cosmic ray spectrum above eV using inclined events detected with the Pierre Auger Observatory
A measurement of the cosmic-ray spectrum for energies exceeding
eV is presented, which is based on the analysis of showers
with zenith angles greater than detected with the Pierre Auger
Observatory between 1 January 2004 and 31 December 2013. The measured spectrum
confirms a flux suppression at the highest energies. Above
eV, the "ankle", the flux can be described by a power law with
index followed by
a smooth suppression region. For the energy () at which the
spectral flux has fallen to one-half of its extrapolated value in the absence
of suppression, we find
eV.Comment: Replaced with published version. Added journal reference and DO
Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
The Auger Engineering Radio Array (AERA) is part of the Pierre Auger
Observatory and is used to detect the radio emission of cosmic-ray air showers.
These observations are compared to the data of the surface detector stations of
the Observatory, which provide well-calibrated information on the cosmic-ray
energies and arrival directions. The response of the radio stations in the 30
to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of
the incoming electric field. For the latter, the energy deposit per area is
determined from the radio pulses at each observer position and is interpolated
using a two-dimensional function that takes into account signal asymmetries due
to interference between the geomagnetic and charge-excess emission components.
The spatial integral over the signal distribution gives a direct measurement of
the energy transferred from the primary cosmic ray into radio emission in the
AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air
shower arriving perpendicularly to the geomagnetic field. This radiation energy
-- corrected for geometrical effects -- is used as a cosmic-ray energy
estimator. Performing an absolute energy calibration against the
surface-detector information, we observe that this radio-energy estimator
scales quadratically with the cosmic-ray energy as expected for coherent
emission. We find an energy resolution of the radio reconstruction of 22% for
the data set and 17% for a high-quality subset containing only events with at
least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO
Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy
We measure the energy emitted by extensive air showers in the form of radio
emission in the frequency range from 30 to 80 MHz. Exploiting the accurate
energy scale of the Pierre Auger Observatory, we obtain a radiation energy of
15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV
arriving perpendicularly to a geomagnetic field of 0.24 G, scaling
quadratically with the cosmic-ray energy. A comparison with predictions from
state-of-the-art first-principle calculations shows agreement with our
measurement. The radiation energy provides direct access to the calorimetric
energy in the electromagnetic cascade of extensive air showers. Comparison with
our result thus allows the direct calibration of any cosmic-ray radio detector
against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI.
Supplemental material in the ancillary file
Production of Single W Bosons at LEP
We report on the observation of single W boson production in a data sample collected by the L3 detector at LEP2. The signal consists of large missing energy final states with a single energetic lepton or two hadronic jets. The cross-section is measured to be at the centre of mass energy \sqrt{s}=172 \GeV{}, consistent with the Standard Model expectation. From this measurement the following limits on the anomalous WW gauge couplings are derived at 95\% CL: and
Measurement of the Average Lifetime of b-Hadrons in Z Decays
We present a measurement of the average b-hadron lifetime at the collider LEP. Using hadronic Z decays collected in the period from 1991 to 1994, two independent analyses have been performed. In the first one, the b-decay position is reconstructed as a secondary vertex of hadronic b-decay particles. The second analysis is an updated measurement of using the impact parameter of leptons with high momentum and high transverse momentum. The combined result is \begin{center} . \end{center} In addition, we measure the average charged b-decay multiplicity and the normalized average b-energy at LEP to be \begin{center} , \end{center} \begin{center} \end{center
Genome of Herbaspirillum seropedicae Strain SmR1, a Specialized Diazotrophic Endophyte of Tropical Grasses
The molecular mechanisms of plant recognition, colonization, and nutrient exchange between diazotrophic endophytes and plants are scarcely known. Herbaspirillum seropedicae is an endophytic bacterium capable of colonizing intercellular spaces of grasses such as rice and sugar cane. The genome of H. seropedicae strain SmR1 was sequenced and annotated by The ParanĂĄ State Genome ProgrammeâGENOPAR. The genome is composed of a circular chromosome of 5,513,887 bp and contains a total of 4,804 genes. The genome sequence revealed that H. seropedicae is a highly versatile microorganism with capacity to metabolize a wide range of carbon and nitrogen sources and with possession of four distinct terminal oxidases. The genome contains a multitude of protein secretion systems, including type I, type II, type III, type V, and type VI secretion systems, and type IV pili, suggesting a high potential to interact with host plants. H. seropedicae is able to synthesize indole acetic acid as reflected by the four IAA biosynthetic pathways present. A gene coding for ACC deaminase, which may be involved in modulating the associated plant ethylene-signaling pathway, is also present. Genes for hemagglutinins/hemolysins/adhesins were found and may play a role in plant cell surface adhesion. These features may endow H. seropedicae with the ability to establish an endophytic life-style in a large number of plant species
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