Institution
University of Portsmouth
Education•Portsmouth, Portsmouth, United Kingdom•
About: University of Portsmouth is a education organization based out in Portsmouth, Portsmouth, United Kingdom. It is known for research contribution in the topics: Population & Galaxy. The organization has 5452 authors who have published 14256 publications receiving 424346 citations. The organization is also known as: Portsmouth and Gosport School of Science and Art & Portsmouth and Gosport School of Science and the Arts.
Topics: Population, Galaxy, Redshift, Context (language use), Computer science
Papers published on a yearly basis
Papers
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TL;DR: The Cognitive Interview (CI) is a well-established protocol for interviewing wit- nesses as discussed by the authors, which is based upon established psychological principles of remembering and retrieval of information from memory, and empirical laboratory research on the CI has documented its ability to dramatically improve the number of correct details while only slightly increasing the incorrect details.
Abstract: The Cognitive Interview (CI) is a well-established protocol for interviewing wit- nesses The current article presents a study space analysis of laboratory studies of the CI together with an empirical meta-analysis summarizing the past 25 years of research The study space comprises 57 published articles (65 experiments) on the CI, providing an assessment of the boundary conditions underlying the analysis and application of this interview protocol The current meta-analysis includes 46 pub- lished articles, including 20 articles published since the last meta-analysis conducted a decade earlier (Kohnken, Milne, Memon, & Bull, 1999) Reassuringly for prac- titioners, the findings of the original meta-analysis were replicated with a large and significant increase in correct details and a small increase in errors In addition we found that there were no differences in the rate at which details are confabulated Importantly, the effect sizes were unaffected by the inclusion of recent studies using modified versions of the CI The CI appeared to benefit older adult witnesses even more than younger adults We highlight trends and gaps in research and discuss how our findings can inform policy and training decisions The Cognitive Interview (or CI) is perhaps one of the most successful developments in psychology and law research in the last 25 years It is a method that comprises a series of memory retrieval and communication techniques designed to increase the amount of information that can be obtained from an interviewee The CI was initially developed 25 years ago by psychologists Ed Geiselman and Ron Fisher as a response to the many requests they received from police officers and legal professionals for a method of improving witness inter- views It is based upon established psychological principles of remembering and retrieval of information from memory, and empirical laboratory research on the CI has documented its ability to dramatically improve the number of correct details while only slightly increasing the number of incorrect details (Schrieber & Fisher, 2006; Kohnken et al, 1999; Memon, 2006) Field tests of the CI have also indicated that police officers trained in its techniques gain more information and
412 citations
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California Institute of Technology1, Johns Hopkins University2, University of Arizona3, Monterey Institute for Research in Astronomy4, University of California, Los Angeles5, University of Hawaii at Manoa6, Harvard University7, Dartmouth College8, University of California, Santa Barbara9, Cornell University10, Embry–Riddle Aeronautical University11, University of Missouri–Kansas City12, University of Maryland, College Park13, Clemson University14, University of Illinois at Urbana–Champaign15, Pennsylvania State University16, United States Naval Academy17, University of Portsmouth18, Ludwig Maximilian University of Munich19, Lowell Observatory20
TL;DR: In this article, the authors carried out a highly uniform survey of the near-Earth object (NEO) population at thermal infrared wavelengths ranging from 3 to 22 μm, allowing them to refine estimates of their numbers, sizes, and albedos.
Abstract: With the NEOWISE portion of the Wide-field Infrared Survey Explorer (WISE) project, we have carried out a highly uniform survey of the near-Earth object (NEO) population at thermal infrared wavelengths ranging from 3 to 22 μm, allowing us to refine estimates of their numbers, sizes, and albedos. The NEOWISE survey detected NEOs the same way whether they were previously known or not, subject to the availability of ground-based follow-up observations, resulting in the discovery of more than 130 new NEOs. The survey's uniform sensitivity, observing cadence, and image quality have permitted extrapolation of the 428 near-Earth asteroids (NEAs) detected by NEOWISE during the fully cryogenic portion of the WISE mission to the larger population. We find that there are 981 ± 19 NEAs larger than 1 km and 20,500 ± 3000 NEAs larger than 100 m. We show that the Spaceguard goal of detecting 90% of all 1 km NEAs has been met, and that the cumulative size distribution is best represented by a broken power law with a slope of 1.32 ± 0.14 below 1.5 km. This power-law slope produces ~13,200 ± 1900 NEAs with D > 140 m. Although previous studies predict another break in the cumulative size distribution below D ~ 50-100 m, resulting in an increase in the number of NEOs in this size range and smaller, we did not detect enough objects to comment on this increase. The overall number for the NEA population between 100 and 1000 m is lower than previous estimates. The numbers of near-Earth comets and potentially hazardous NEOs will be the subject of future work.
410 citations
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TL;DR: The data suggest that the unique spatial distribution of di- and tri-Me K36/H3 plays a role in transcriptional termination and/or early RNA processing in higher eukaryotes.
409 citations
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TL;DR: In this paper, the distribution and thickness of the basal Silurian hot shales have been mapped in detail for the whole North African region, using logs from some 300 exploration wells in Libya, Tunisia, Algeria and Morocco.
407 citations
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California Institute of Technology1, Tel Aviv University2, University of Maryland, College Park3, Goddard Space Flight Center4, University of Wisconsin–Milwaukee5, Stockholm University6, Princeton University7, Liverpool John Moores University8, National Central University9, Hebrew University of Jerusalem10, Australian Research Council11, University of Sydney12, Indian Institute of Astrophysics13, Indian Institute of Science14, Commonwealth Scientific and Industrial Research Organisation15, University of Colorado Boulder16, Columbia University17, University of Washington18, Indian Institute of Technology Bombay19, Inter-University Centre for Astronomy and Astrophysics20, University of California, Berkeley21, Lawrence Berkeley National Laboratory22, George Washington University23, Texas Tech University24, University College London25, University of Leicester26, Space Telescope Science Institute27, National Radio Astronomy Observatory28, University of Southampton29, University of Portsmouth30, Radboud University Nijmegen31, Tokyo Institute of Technology32, Max Planck Society33, Adler Planetarium34, Northwestern University35, University of Oxford36, Weizmann Institute of Science37, Institute for the Physics and Mathematics of the Universe38, San Diego State University39, University of California, Merced40
TL;DR: In this paper, the authors established the physical association of an electromagnetic counterpart EM170817 to gravitational waves (GW 170817) detected from merging neutron stars by synthesizing a panchromatic dataset.
Abstract: Merging neutron stars offer an exquisite laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart EM170817 to gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic dataset, we demonstrate that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis. The weak gamma-rays seen in EM170817 are dissimilar to classical short gamma-ray bursts with ultra-relativistic jets. Instead, we suggest that breakout of a wide-angle, mildly-relativistic cocoon engulfing the jet elegantly explains the low-luminosity gamma-rays, the high-luminosity ultraviolet-optical-infrared and the delayed radio/X-ray emission. We posit that all merging neutron stars may lead to a wide-angle cocoon breakout; sometimes accompanied by a successful jet and sometimes a choked jet.
403 citations
Authors
Showing all 5624 results
Name | H-index | Papers | Citations |
---|---|---|---|
Robert C. Nichol | 187 | 851 | 162994 |
Gavin Davies | 159 | 2036 | 149835 |
Daniel Thomas | 134 | 846 | 84224 |
Will J. Percival | 129 | 473 | 87752 |
Claudia Maraston | 103 | 362 | 59178 |
I. W. Harry | 98 | 312 | 65338 |
Timothy Clark | 95 | 1137 | 53665 |
Kevin Schawinski | 95 | 376 | 30207 |
Ashley J. Ross | 90 | 248 | 46395 |
Josep Call | 90 | 451 | 34196 |
David A. Wake | 89 | 214 | 46124 |
L. K. Nuttall | 89 | 253 | 54834 |
Stephen Neidle | 89 | 457 | 32417 |
Andrew Lundgren | 88 | 249 | 57347 |
Rita Tojeiro | 87 | 229 | 43140 |