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A Single Visualization Technique for Displaying Multiple Metabolite-Phenotype Associations.
To assist with management and interpretation of human metabolomics data, which are rapidly increasing in quantity and complexity, we need better visualization tools. Using a dataset of several hundred metabolite measures profiled in a cohort of ~1500 individuals sampled from a population-based community study, we performed association analyses with eight demographic and clinical traits and outcomes. We compared frequently used existing graphical approaches with a novel 'rain plot' approach to display the results of these analyses. The 'rain plot' combines features of a raindrop plot and a conventional heatmap to convey results of multiple association analyses. A rain plot can simultaneously indicate effect size, directionality, and statistical significance of associations between metabolites and several traits. This approach enables visual comparison features of all metabolites examined with a given trait. The rain plot extends prior approaches and offers complementary information for data interpretation. Additional work is needed in data visualizations for metabolomics to assist investigators in the process of understanding and convey large-scale analysis results effectively, feasibly, and practically
Can residuals of the Solar system foreground explain low multipole anomalies of the CMB ?
The low multipole anomalies of the Cosmic Microwave Background has received
much attention during the last few years. It is still not ascertained whether
these anomalies are indeed primordial or the result of systematics or
foregrounds. An example of a foreground, which could generate some non-Gaussian
and statistically anisotropic features at low multipole range, is the very
symmetric Kuiper Belt in the outer solar system. In this paper, expanding upon
the methods presented by Maris et al. (2011), we investigate the contributions
from the Kuiper Belt objects (KBO) to the WMAP ILC 7 map, whereby we can
minimize the contrast in power between even and odd multipoles in the CMB,
discussed discussed by Kim & Naselsky (2010). We submit our KBO de-correlated
CMB signal to several tests, to analyze its validity, and find that
incorporation of the KBO emission can decrease the quadrupole-octupole
alignment and parity asymmetry problems, provided that the KBO signals has a
non-cosmological dipole modulation, associated with the statistical anisotropy
of the ILC 7 map. Additionally, we show that the amplitude of the dipole
modulation, within a 2 sigma interval, is in agreement with the corresponding
amplitudes, discussed by Lew (2008).Comment: 24 pages, 9 figures, 5 tables. Matches version in JCA
Massive Star Cluster Formation and Destruction in Luminous Infrared Galaxies in GOALS
We present the results of a {\it Hubble Space Telescope} ACS/HRC FUV, ACS/WFC
optical study into the cluster populations of a sample of 22 Luminous Infrared
Galaxies in the Great Observatories All-Sky LIRG Survey. Through integrated
broadband photometry we have derived ages and masses for a total of 484 star
clusters contained within these systems. This allows us to examine the
properties of star clusters found in the extreme environments of LIRGs relative
to lower luminosity star-forming galaxies in the local Universe. We find that
by adopting a Bruzual \& Charlot simple stellar population (SSP) model and
Salpeter initial mass function, the age distribution of clusters declines as
, consistent with the age distribution derived
for the Antennae Galaxies, and interpreted as evidence for rapid cluster
disruption occuring in the strong tidal fields of merging galaxies. The large
number of young clusters identified in the sample also
suggests that LIRGs are capable of producing more high-mass clusters than what
is observed to date in any lower luminosity star-forming galaxy in the local
Universe. The observed cluster mass distribution of is consistent with the canonical -2 power law used to describe the
underlying initial cluster mass function (ICMF) for a wide range of galactic
environments. We interpret this as evidence against mass-dependent cluster
disruption, which would flatten the observed CMF relative to the underlying
ICMF distribution.Comment: 63 pages, 58 Figures, 56 Tables, Accepted for publication in Ap
Finite-size scaling for non-linear rheology of fluids confined in a small space
We perform molecular dynamics simulations in order to examine the rheological
transition of fluids confined in a small space. By performing finite-size
scaling analysis, we demonstrate that this rheological transition results from
the competition between the system size and the length scale of cooperative
particle motion.Comment: 4pages, 8 figure
The Lifetimes and Evolution of Molecular Cloud Cores
We discuss the lifetimes and evolution of clumps and cores formed as
turbulent density fluctuations in nearly isothermal molecular clouds. In the
non-magnetic case, clumps are unlikely to reach a hydrostatic state, and
instead are expected to either proceed directly to collapse, or else
``rebound'' towards the mean pressure and density of the parent cloud.
Rebounding clumps are delayed in their re-expansion by their self-gravity. From
a simple virial calculation, we find re-expansion times of a few free-fall
times. In the magnetic case, we present a series of driven-turbulence,
ideal-MHD isothermal numerical simulations in which we follow the evolution of
clumps and cores in relation to the magnetic criticality of their ``parent
clouds'' (the numerical boxes). In subcritical boxes, magnetostatic clumps do
not form. A few moderately-gravitationally bound clumps form which however are
dispersed by the turbulence in < 1.3 Myr. An estimate of the ambipolar
diffusion (AD) time scale t_AD in these cores gives t_AD > 1.3 Myr, only
slightly longer than the dynamical times. In supercritical boxes, some cores
become locally supercritical and collapse in typical times ~ 1 Myr. We also
observe longer-lived supercritical cores that however do not collapse because
they are smaller than the local Jeans length. Fewer clumps and cores form in
these simulations than in their non-magnetic counterpart. Our results suggest
that a) A fraction of the cores may not form stars, and may correspond to some
of the observed starless cores. b) Cores may be out-of-equilibrium structures,
rather than quasi-magnetostatic ones. c) The magnetic field may help reduce the
star formation efficiency by reducing the probability of core formation, rather
than by significantly delaying the collapse of individual cores.Comment: Accepted in ApJ. Originally submitted as astro-ph/0208245. Completely
rewritten, now including numerical simulations. Animations available at
http://www.astrosmo.unam.mx/~e.vazquez/turbulence_HP/movies/VKSB04.htm
This Is Just A Test: Overcoming High-Stakes Test Anxiety through Relaxation and Gum Chewing When Preparing for the ACT
This study was a replication of a previous study (in which) participants were given relaxation and deep breathing training to help manage test anxiety. The study examined the correlations between relaxation strategies, gum chewing and variables including socioeconomic status, class rank, GPA, and importance of going to college. Participants included 96 high school students (36 males, 60 females), preparing for the ACT (American College Testing). Results indicated that the relaxation intervention had a significant effect in reducing test anxiety
Dynamical Axion Field in Topological Magnetic Insulators
Axions are very light, very weakly interacting particles postulated more than
30 years ago in the context of the Standard Model of particle physics. Their
existence could explain the missing dark matter of the universe. However,
despite intensive searches, they have yet to be detected. In this work, we show
that magnetic fluctuations of topological insulators couple to the
electromagnetic fields exactly like the axions, and propose several experiments
to detect this dynamical axion field. In particular, we show that the axion
coupling enables a nonlinear modulation of the electromagnetic field, leading
to attenuated total reflection. We propose a novel optical modulators device
based on this principle.Comment: 5 pages, 3 figure
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