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Institution

University of Portsmouth

EducationPortsmouth, 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.


Papers
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Journal ArticleDOI
T. M. C. Abbott, Filipe B. Abdalla1, Filipe B. Abdalla2, S. Allam3  +220 moreInstitutions (50)
TL;DR: The first public data release of the DES DR1 dataset is described in this paper, consisting of reduced single-epoch images, co-add images, and co-added source catalogs, and associated products and services.
Abstract: We describe the first public data release of the Dark Energy Survey, DES DR1, consisting of reduced single-epoch images, co-added images, co-added source catalogs, and associated products and services assembled over the first 3 yr of DES science operations. DES DR1 is based on optical/near-infrared imaging from 345 distinct nights (2013 August to 2016 February) by the Dark Energy Camera mounted on the 4 m Blanco telescope at the Cerro Tololo InterAmerican Observatory in Chile. We release data from the DES wide-area survey covering similar to 5000 deg(2) of the southern Galactic cap in five broad photometric bands, grizY. DES DR1 has a median delivered point-spread function of g = 1.12, r = 0.96, i = 0.88, z = 0.84, and Y = 0.'' 90 FWHM, a photometric precision of <1% in all bands, and an astrometric precision of 151 mas. The median co-added catalog depth for a 1.'' 95 diameter aperture at signal-to-noise ratio (S/N) = 10 is g = 24.33, r = 24.08, i = 23.44, z = 22.69, and Y = 21.44 mag. DES DR1 includes nearly 400 million distinct astronomical objects detected in similar to 10,000 co-add tiles of size 0.534 deg(2) produced from similar to 39,000 individual exposures. Benchmark galaxy and stellar samples contain similar to 310 million and similar to 80 million objects, respectively, following a basic object quality selection. These data are accessible through a range of interfaces, including query web clients, image cutout servers, jupyter notebooks, and an interactive co-add image visualization tool. DES DR1 constitutes the largest photometric data set to date at the achieved depth and photometric precision.

506 citations

Journal ArticleDOI
TL;DR: A validated, paper-based, aggregate weighted track and trigger system (AWTTS) that could serve as a template for a national early warning score (EWS) for the detection of patient deterioration is developed and demonstrated that its performance for predicting mortality (within a range of timescales) is superior to all other published AWTTSs.

495 citations

Journal ArticleDOI
TL;DR: In this article, the authors demonstrate that ionic defects, migrating on timescales significantly longer (above 103 s) than what has so far been explored (from 10−1 to 102 s), abate the initial efficiency by 10−15% after several hours of operation at the maximum power point.
Abstract: Perovskites have been demonstrated in solar cells with a power conversion efficiency of well above 20%, which makes them one of the strongest contenders for next generation photovoltaics. While there are no concerns about their efficiency, very little is known about their stability under illumination and load. Ionic defects and their migration in the perovskite crystal lattice are some of the most alarming sources of degradation, which can potentially prevent the commercialization of perovskite solar cells (PSCs). In this work, we provide direct evidence of electric field-induced ionic defect migration and we isolate their effect on the long-term performance of state-of-the-art devices. Supported by modelling, we demonstrate that ionic defects, migrating on timescales significantly longer (above 103 s) than what has so far been explored (from 10−1 to 102 s), abate the initial efficiency by 10–15% after several hours of operation at the maximum power point. Though these losses are not negligible, we prove that the initial efficiency is fully recovered when leaving the device in the dark for a comparable amount of time. We verified this behaviour over several cycles resembling day/night phases, thus probing the stability of PSCs under native working conditions. This unusual behaviour reveals that research and industrial standards currently in use to assess the performance and the stability of solar cells need to be adjusted for PSCs. Our work paves the way for much needed new testing protocols and figures of merit specifically designed for PSCs.

487 citations

Journal ArticleDOI
Joshua A. Frieman1, Joshua A. Frieman2, Bruce A. Bassett3, Andrew C. Becker4, Changsu Choi5, D. Cinabro6, F. DeJongh1, Darren L. DePoy7, Ben Dilday2, Mamoru Doi8, Peter M. Garnavich9, Craig J. Hogan4, Jon A. Holtzman10, Myungshin Im5, Saurabh Jha11, Richard Kessler2, Kohki Konishi8, Hubert Lampeitl12, John Marriner1, Jennifer L. Marshall7, D. McGinnis1, G. Miknaitis1, Robert C. Nichol13, J. L. Prieto7, Adam G. Riess14, Adam G. Riess12, Michael Richmond15, Roger W. Romani11, Masao Sako16, Donald P. Schneider17, Mathew Smith13, Naohiro Takanashi8, Kouichi Tokita8, Kurt van der Heyden, Naoki Yasuda8, Chen Zheng11, Jennifer K. Adelman-McCarthy1, James Annis1, Roberto J. Assef7, J. C. Barentine18, J. C. Barentine19, Ralf Bender20, Roger Blandford11, William N. Boroski1, Malcolm N. Bremer21, Howard Brewington19, Chris A. Collins22, Arlin P. S. Crotts23, Jack Dembicky19, Jason D. Eastman7, Alastair C. Edge24, Edmond Edmondson13, Edward C. Elson, Michael E. Eyler25, Alexei V. Filippenko26, Ryan J. Foley26, Stephan Frank7, Ariel Goobar27, Tina Gueth10, James E. Gunn28, Michael Harvanek19, Michael Harvanek29, Ulrich Hopp20, Yutaka Ihara8, Želko Ivezić4, Steven M. Kahn11, Jared Kaplan30, Stephen B. H. Kent1, Stephen B. H. Kent2, William Ketzeback19, S. J. Kleinman31, S. J. Kleinman19, Wolfram Kollatschny32, Richard G. Kron2, Jurek Krzesinski19, D. Lamenti33, Giorgos Leloudas34, Huan Lin1, Dan Long19, John R. Lucey24, Robert H. Lupton28, Elena Malanushenko19, Viktor Malanushenko19, Russet McMillan19, Javier Méndez35, Christopher W. Morgan25, Christopher W. Morgan7, Tomoki Morokuma8, Atsuko Nitta19, Linda Ostman27, Kaike Pan19, Constance M. Rockosi36, A. Kathy Romer37, Pilar Ruiz-Lapuente35, G. Saurage19, K. Schlesinger7, Stephanie A. Snedden19, Jesper Sollerman34, Jesper Sollerman27, Chris Stoughton1, Maximilian Stritzinger34, Mark SubbaRao2, Douglas L. Tucker1, Petri Väisänen, Linda C. Watson7, S. Watters19, J. Craig Wheeler18, Brian Yanny1, Donald G. York2 
TL;DR: The Sloan Digital Sky Survey-II (SDSS-II) as mentioned in this paper is a multi-year project to identify and measure light curves for intermediate-redshift (0.05 < z < 0.35) Type Ia supernovae (SNe Ia) using repeated five-band imaging over an area of 300 sq. deg.
Abstract: The Sloan Digital Sky Survey-II (SDSS-II) has embarked on a multi-year project to identify and measure light curves for intermediate-redshift (0.05 < z < 0.35) Type Ia supernovae (SNe Ia) using repeated five-band (ugriz) imaging over an area of 300 sq. deg. The survey region is a stripe 2.5° wide centered on the celestial equator in the Southern Galactic Cap that has been imaged numerous times in earlier years, enabling construction of a deep reference image for the discovery of new objects. Supernova imaging observations are being acquired between September 1 and November 30 of 2005-7. During the first two seasons, each region was imaged on average every five nights. Spectroscopic follow-up observations to determine supernova type and redshift are carried out on a large number of telescopes. In its first two three-month seasons, the survey has discovered and measured light curves for 327 spectroscopically confirmed SNe Ia, 30 probable SNe Ia, 14 confirmed SNe Ib/c, 32 confirmed SNe II, plus a large number of photometrically identified SNe Ia, 94 of which have host-galaxy spectra taken so far. This paper provides an overview of the project and briefly describes the observations completed during the first two seasons of operation.

486 citations

Journal ArticleDOI
TL;DR: In this paper, the authors explored the views of over 400 business studies, marketing and human resource management undergraduate students on the development of employability skills within their curricula and found that motivation and commitment of learners is an essential prerequisite for effective outcomes.
Abstract: Despite ongoing debate about whether they can and should, most higher education institutions include the development of employability skills within their curricula. However, employers continue to report that graduates are not ready for the world of work, and lack some of the most basic skills needed for successful employment. Research into why this might be abounds from the perspectives of multiple stakeholders, including government, employers, higher education institutions and graduates. Interestingly though, the views of undergraduates, the recipients of this employability development, are not well known. This could be important, because learning theory tells us that motivation and commitment of learners is an essential prerequisite for effective outcomes. So the question is raised as to whether undergraduate students are engaged with employability skills development. This article reports on a study exploring the views of over 400 business studies, marketing and human resource management undergraduate s...

485 citations


Authors

Showing all 5624 results

NameH-indexPapersCitations
Robert C. Nichol187851162994
Gavin Davies1592036149835
Daniel Thomas13484684224
Will J. Percival12947387752
Claudia Maraston10336259178
I. W. Harry9831265338
Timothy Clark95113753665
Kevin Schawinski9537630207
Ashley J. Ross9024846395
Josep Call9045134196
David A. Wake8921446124
L. K. Nuttall8925354834
Stephen Neidle8945732417
Andrew Lundgren8824957347
Rita Tojeiro8722943140
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
202363
2022282
2021961
2020976
2019905
2018850