5,618 research outputs found
Towards an understanding of third-order galaxy-galaxy lensing
Third-order galaxy-galaxy lensing (G3L) is a next generation galaxy-galaxy
lensing technique that either measures the excess shear about lens pairs or the
excess shear-shear correlations about lenses. It is clear that these statistics
assess the three-point correlations between galaxy positions and projected
matter density. For future applications of these novel statistics, we aim at a
more intuitive understanding of G3L to isolate the main features that possibly
can be measured. We construct a toy model ("isolated lens model"; ILM) for the
distribution of galaxies and associated matter to determine the measured
quantities of the two G3L correlation functions and traditional galaxy-galaxy
lensing (GGL) in a simplified context. The ILM presumes single lens galaxies to
be embedded inside arbitrary matter haloes that, however, are statistically
independent ("isolated") from any other halo or lens position. In the ILM, the
average mass-to-galaxy number ratio of clusters of any size cannot change. GGL
and galaxy clustering alone cannot distinguish an ILM from any more complex
scenario. The lens-lens-shear correlator in combination with second-order
statistics enables us to detect deviations from a ILM, though. This can be
quantified by a difference signal defined in the paper. We demonstrate with the
ILM that this correlator picks up the excess matter distribution about galaxy
pairs inside clusters. The lens-shear-shear correlator is sensitive to
variations among matter haloes. In principle, it could be devised to constrain
the ellipticities of haloes, without the need for luminous tracers, or maybe
even random halo substructure. [Abridged]Comment: 14 pages, 3 figures, 1 table, accepted by A&A; some
"lens-shear-shear" were falsely "lens-lens-shear
A perspective on consultancy teams and technology in applied sport psychology
Objectives and method: This article introduces the concept of consultancy teams to a sport psychology readership, presenting an overview of initial applications and findings of this approach in applied settings. Although the notion and application of consultancy teams in therapeutic settings has been around for many years (e.g., Weakland, Fisch, Watzlawick, & Bodin, 1974), they have yet to be explored within our discipline. Here, we present the theoretical foundations and historical application of consultancy team models, outlining our experience of using consultancy teams in an applied sport psychology setting. Moving towards the development of expertise and excellence in team consultancy methods, we subsequently describe how this process was assisted with the use of technology (i.e., the iPsych system).
Results and conclusions: When consultancy teams practice it is necessary for one practitioner (the primary practitioner) to conduct the session with the client. The remaining team (the observation team) allows the primary practitioner maximum involvement with the client, while simultaneously assisting them to solve the presenting problem. The implications of working in this manner, alongside the novel use of technology, are considered with respect to the consultancy process and the development of excellence in training (neophyte) and existing practitioners. It is hoped that this article will provoke interest among sport psychologists in this way of consulting and direct thought towards other novel approaches to delivering interventions.</p
Terror management and cognitive-experiential self-theory: Evidence that terror management occurs in the experiential system.
Stereotypes and terror management: Evidence that mortality salience enhances stereotypic thinking and preferences.
Stereotypes and terror management: Evidence that mortality salience enhances stereotypic thinking and preferences.
A prototype system for detecting the radio-frequency pulse associated with cosmic ray air showers
The development of a system to detect the radio-frequency (RF) pulse
associated with extensive air showers of cosmic rays is described. This work
was performed at the CASA/MIA array in Utah, with the intention of designing
equipment that can be used in conjunction with the Auger Giant Array. A small
subset of data (less than 40 out of a total of 600 hours of running time),
taken under low-noise conditions, permitted upper limits to be placed on the
rate for pulses accompanying showers of energies around eV.Comment: 53 pages, LaTeX, 19 figures, published in Nuclear Instruments and
Methods. Revised version; some references update
First detection of galaxy-galaxy-galaxy lensing in RCS. A new tool for studying the matter environment of galaxy pairs
The weak gravitational lensing effect, small coherent distortions of galaxy
images by means of a gravitational tidal field, can be used to study the
relation between the matter and galaxy distribution. In this context, weak
lensing has so far only been used for considering a second-order correlation
function that relates the matter density and galaxy number density as a
function of separation. We implement two new, third-order correlation functions
that have recently been suggested in the literature, and apply them to the
Red-Sequence Cluster Survey. We demonstrate that it is possible, even with
already existing data, to make significant measurements of third-order lensing
correlations. We develop an optimised computer code for the correlation
functions. To test its reliability a set of tests are performed. The
correlation functions are transformed to aperture statistics, which allow easy
tests for remaining systematics in the data. In order to further verify the
robustness of our measurement, the signal is shown to vanish when randomising
the source ellipticities. Finally, the lensing signal is compared to crude
predictions based on the halo-model. On angular scales between roughly 1 arcmin
and 11 arcmin a significant third-order correlation between two lens positions
and one source ellipticity is found. We discuss this correlation function as a
novel tool to study the average matter environment of pairs of galaxies.
Correlating two source ellipticities and one lens position yields a less
significant but nevertheless detectable signal on a scale of 4 arcmin. Both
signals lie roughly within the range expected by theory which supports their
cosmological origin.[ABRIDGED]Comment: 15 pages, 12 figures, accepted by A&A; minor change
The health of mothers of children with a life-limiting condition : a protocol for comparative cohort study using the Clinical Practice Research Datalink
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