6,193 research outputs found
The Influence of Pregnancy on the Recurrence of Cutaneous Malignant Melanoma in Women
Objective. The aim of this study was to determine whether pregnancy increases the recurrence risk of cutaneous malignant melanoma (CMM) in women with a history of stage I CMM. Methods. The electronic medical databases of Medline and Embase were explored. All 1084 obtained articles were screened on title and abstract using predetermined inclusion and exclusion criteria. A critical appraisal of relevance and validity was conducted on the remaining full text available articles. Results. Two studies were selected. Both studies revealed no significant difference in disease-free survival between women with stage I CMM and the control population. Conclusion. Pregnancy does not increase the recurrence risk of CMM in women with a history of stage I CMM
Field testing a novel high residence positioning system for monitoring the fine‐scale movements of aquatic organisms
1. Acoustic telemetry is an important tool for studying the behaviour of aquatic organisms in the wild.
2. VEMCO high residence (HR) tags and receivers are a recent introduction in the field of acoustic telemetry and can be paired with existing algorithms (e.g. VEMCO positioning system [VPS]) to obtain high‐resolution two‐dimensional positioning data.
3. Here, we present results of the first documented field test of a VPS composed of HR receivers (hereafter, HR‐VPS). We performed a series of stationary and moving trials with HR tags (mean HR transmission period = 1.5 s) to evaluate the precision, accuracy and temporal capabilities of this positioning technology. In addition, we present a sample of data obtained for five European perch Perca fluviatilis implanted with HR tags (mean HR transmission period = 4 s) to illustrate how this technology can estimate the fine‐scale behaviour of aquatic animals.
4. Accuracy and precision estimates (median [5th–95th percentile]) of HR‐VPS positions for all stationary trials were 5.6 m (4.2–10.8 m) and 0.1 m (0.02–0.07 m), respectively, and depended on the location of tags within the receiver array. In moving tests, tracks generated by HR‐VPS closely mimicked those produced by a handheld GPS held over the tag, but these differed in location by an average of ≈9 m.
5. We found that estimates of animal speed and distance travelled for perch declined when positional data for acoustically tagged perch were thinned to mimic longer transmission periods. These data also revealed a trade‐off between capturing real nonlinear animal movements and the inclusion of positioning error.
6. Our results suggested that HR‐VPS can provide more representative estimates of movement metrics and offer an advancement for studying fine‐scale movements of aquatic organisms, but high‐precision survey techniques may be needed to test these systems
Measurement of Jets and Jet Suppression in sqrt(s_NN)=2.76 TeV Lead-Lead Collisions with the ATLAS detector at the LHC
The first results of single jet observables in Pb+Pb collisions at
sqrt(s_NN)=2.76 TeV measured with the ATLAS detector at the LHC are presented.
Full jets are reconstructed with the anti-kt algorithm with R= 0.2 and 0.4,
using an event-by-event subtraction procedure to correct for the effects of the
underlying event including elliptic flow. The geometrically-scaled ratio of jet
yields in central and peripheral events,Rcp, indicates a clear suppression of
jets with ET >100 GeV. The transverse and longitudinal distributions of jet
fragments is also presented. We find little no substantial change to the
fragmentation properties and no significant change in the level of suppression
when moving to the larger jet definition.Comment: 5 pages, 6 figures, proceedings for Quark Matter 2011, Annecy,
France, May 23-28, 201
Time correlations in a confined magnetized free-electron gas
The time-dependent pair correlation functions for a degenerate ideal quantum
gas of charged particles in a uniform magnetic field are studied on the basis
of equilibrium statistics. In particular, the influence of a flat hard wall on
the correlations is investigated, both for a perpendicular and a parallel
orientation of the wall with respect to the field. The coherent and incoherent
parts of the time-dependent structure function in position space are determined
from an expansion in terms of the eigenfunctions of the one-particle
Hamiltonian. For the bulk of the system, the intermediate scattering function
and the dynamical structure factor are derived by taking successive Fourier
transforms. In the vicinity of the wall the time-dependent coherent structure
function is found to decay faster than in the bulk. For coinciding positions
near the wall the form of the structure function turns out to be independent of
the orientation of the wall. Numerical results are shown to corroborate these
findings.Comment: 25 pages, 14 figures, to be published in Journal of Physics
New upper limits on low-frequency radio emission from isolated neutron stars with LOFAR
Neutron stars that show X-ray and -ray pulsed emission must,
somewhere in the magnetosphere, generate electron-positron pairs. Such pairs
are also required for radio emission, but then why do a number of these sources
appear radio quiet? Here, we carried out a deep radio search towards four such
neutron stars that are isolated X-ray/-ray pulsars but for which no
radio pulsations have been detected yet. These sources are 1RXS
J141256.0+792204 (Calvera), PSR J1958+2846, PSR J1932+1916 and SGR J1907+0919.
Searching at lower radio frequencies, where the radio beam is thought to be
wider, increases the chances of detecting these sources, compared to the
earlier higher-frequency searches. We thus carried a search for periodic and
single-pulse radio emission with the LOFAR radio telescope at 150 MHz. We used
the known periods, and searched a wide range of dispersion measures, as the
distances are not well constrained. We did not detect pulsed emission from any
of the four sources. However, we put very constraining upper limits on the
radio flux density at 150 MHz, of 1.4 mJy.Comment: 7 pages, 2 figures, 1 table. Accepted for publication in Astronomy &
Astrophysic
Gastroenteritis in sentinel general practices,The Netherlands.
From 1996 to 1999, the incidence of gastroenteritis in general practices and the role of a broad range of pathogens in the Netherlands were studied. All patients with gastroenteritis who had visited a general practitioner were reported. All patients who had visited a general practitioner for gastroenteritis (cases) and an equal number of patients visiting for nongastrointestinal symptoms (controls) were invited to participate in a case-control study. The incidence of gastroenteritis was 79.7 per 10,000 person years. Campylobacter was detected most frequently (10% of cases), followed by Giardia lamblia (5%), rotavirus (5%), Norwalk-like viruses (5%) and Salmonella (4%). Our study found that in the Netherlands (population 15.6 million), an estimated 128,000 persons each year consult their general practitioner for gastroenteritis, slightly less than in a comparable study in 1992 to 1993. A pathogen could be detected in almost 40% of patients (bacteria 16%, viruses 15%, parasites 8%)
VLBI for Gravity Probe B. V. Proper Motion and Parallax of the Guide Star, IM Pegasi
We present the principal astrometric results of the very-long-baseline
interferometry (VLBI) program undertaken in support of the Gravity Probe B
(GP-B) relativity mission. VLBI observations of the GP-B guide star, the RS CVn
binary IM Pegasi (HR 8703), yielded positions at 35 epochs between 1997 and
2005. We discuss the statistical assumptions behind these results and our
methods for estimating the systematic errors. We find the proper motion of IM
Peg in an extragalactic reference frame closely related to the International
Celestial Reference Frame 2 (ICRF2) to be -20.83 +- 0.03 +- 0.09 mas/yr in
right ascension and -27.27 +- 0.03 +- 0.09 mas/yr in declination. For each
component the first uncertainty is the statistical standard error and the
second is the total standard error (SE) including plausible systematic errors.
We also obtain a parallax of 10.37 +- 0.07 mas (distance: 96.4 +- 0.7 pc), for
which there is no evidence of any significant contribution of systematic error.
Our parameter estimates for the ~25-day-period orbital motion of the stellar
radio emission have SEs corresponding to ~0.10 mas on the sky in each
coordinate. The total SE of our estimate of IM Peg's proper motion is ~30%
smaller than the accuracy goal set by the GP-B project before launch: 0.14
mas/yr for each coordinate of IM Peg's proper motion. Our results ensure that
the uncertainty in IM Peg's proper motion makes only a very small contribution
to the uncertainty of the GP-B relativity tests.Comment: Accepted for publication in the Astrophysical Journal Supplement
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