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Research data keyboard_double_arrow_right Dataset 2023Publisher:World Data Center for Climate (WDCC) at DKRZ Authors: von Schuckmann, Karina; Minière, Audrey; Gues, Flora; Cuesta-Valero, Francisco José; +58 Authorsvon Schuckmann, Karina; Minière, Audrey; Gues, Flora; Cuesta-Valero, Francisco José; Kirchengast, Gottfried; Adusumilli, Susheel; Straneo, Fiammetta; Allan, Richard; Barker, Paul M.; Beltrami, Hugo; Boyer, Tim; Cheng, Lijing; Church, John; Desbruyeres, Damien; Dolman, Han; Domingues, Catia M.; García-García, Almudena; Gilson, John; Gorfer, Maximilian; Haimberger, Leopold; Hendricks, Stefan; Hosoda, Shigeki; Johnson, Gregory C.; Killick, Rachel; King, Brian A.; Kolodziejczyk, Nicolas; Korosov, Anton; Krinner, Gerhard; Kuusela, Mikael; Langer, Moritz; Lavergne, Thomas; Lawrence, Isobel; Li, Yuehua; Lyman, John; Marzeion, Ben; Mayer, Michael; MacDougall, Andrew; McDougall, Trevor; Monselesan, Didier Paolo; Nitzbon, Jean; Otosaka, Inès; Peng, Jian; Purkey, Sarah; Roemmich, Dean; Sato, Kanako; Sato, Katsunari; Savita, Abhishek; Schweiger, Axel; Shepherd, Andrew; Seneviratne, Sonia I.; Slater, Donald A.; Slater, Thomas; Simons, Leon; Steiner, Andrea K.; Szekely, Tanguy; Suga, Toshio; Thiery, Wim; Timmermanns, Mary-Louise; Vanderkelen, Inne; Wijffels, Susan E.; Wu, Tonghua; Zemp, Michael;Project: GCOS Earth Heat Inventory - A study under the Global Climate Observing System (GCOS) concerted international effort to update the Earth heat inventory (EHI), and presents an updated international assessment of ocean warming estimates, and new and updated estimates of heat gain in the atmosphere, cryosphere and land over the period from 1960 to present. Summary: The file “GCOS_EHI_1960-2020_Earth_Heat_Inventory_Ocean_Heat_Content_data.nc” contains a consistent long-term Earth system heat inventory over the period 1960-2020. Human-induced atmospheric composition changes cause a radiative imbalance at the top-of-atmosphere which is driving global warming. Understanding the heat gain of the Earth system from this accumulated heat – and particularly how much and where the heat is distributed in the Earth system - is fundamental to understanding how this affects warming oceans, atmosphere and land, rising temperatures and sea level, and loss of grounded and floating ice, which are fundamental concerns for society. This dataset is based on a study under the Global Climate Observing System (GCOS) concerted international effort to update the Earth heat inventory published in von Schuckmann et al. (2020), and presents an updated international assessment of ocean warming estimates, and new and updated estimates of heat gain in the atmosphere, cryosphere and land over the period 1960-2020. The dataset also contains estimates for global ocean heat content over 1960-2020 for different depth layers, i.e., 0-300m, 0-700m, 700-2000m, 0-2000m, 2000-bottom, which are described in von Schuckmann et al. (2022). This version includes an update of heat storage of global ocean heat content, where one additional product (Li et al., 2022) had been included to the initial estimate. The Earth heat inventory had been updated accordingly, considering also the update for continental heat content (Cuesta-Valero et al., 2023).
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2017 SpainPublisher:AMER PHYSICAL SOC Funded by:EC | ANDESEC| ANDESWright, T.; Guerrero, C.; Billowes, J.; Calviño Tavares, Francisco; Cortés Rossell, Guillem Pere;handle: 2117/115901
The radiative capture cross section of a highly pure (99.999%), 6.125(2) grams and 9.56(5)E-4 atoms/barn areal density 238U sample has been measured with the Total Absorption Calorimeter (TAC) in the 185 m flight path at the CERN neutron time-of-flight facility n_TOF. This measurement is in response to the NEA High Priority Request list, which demands an accuracy in this cross section of less than 3% below 25 keV. These data have undergone careful background subtraction, with special care being given to the background originating from neutrons scattered by the 238U sample. Pileup and dead-time effects have been corrected for. The measured cross section covers an energy range between 0.2 eV and 80 keV, with an accuracy that varies with neutron energy, being better than 4% below 25 keV and reaching at most 6% at higher energies.
Universitat Politècn... arrow_drop_down Universitat Politècnica de Catalunya, BarcelonaTech: UPCommons - Global access to UPC knowledgeArticle . 2017License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)Recolector de Ciencia Abierta, RECOLECTAArticle . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticleData sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPCArticle . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCAll Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=2117/115901&type=result"></script>'); --> </script>
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more_vert Universitat Politècn... arrow_drop_down Universitat Politècnica de Catalunya, BarcelonaTech: UPCommons - Global access to UPC knowledgeArticle . 2017License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)Recolector de Ciencia Abierta, RECOLECTAArticle . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticleData sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPCArticle . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCAll Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=2117/115901&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Research , Other literature type 2020Publisher:Zenodo Barker, Michelle; Katz, Daniel S.; Chue Hong, Neil P.; Mentzel, Chris; Ram, Karthik; Jones, Catherine; Treloar, Andrew;{"references": ["Adam, David. 2020. \"Special Report: The Simulations Driving the World's Response to COVID-19.\" Nature 580 (7803): 316\u201318. doi.org/10.1038/d41586-020-01003-6.", "Akhmerov, Anton, Maria Cruz, Niels Drost, Cees Hof, Tomas Knapen, Mateusz Kuzak, Carlos Martinez-Ortiz, Yasemin Turkyilmaz-van der Velden, and Ben van Werkhoven. 2019. \"Raising the Profile of Research Software,\" August. https://doi.org/10.5281/ZENODO.3378572.", "Barton, C. Michael, Marina Alberti, Daniel Ames, Jo-An Atkinson, Jerad Bales, Edmund 5 Burke, Min Chen, et al. 2020. \"Call for Transparency of COVID-19 Models.\" Edited by Jennifer Sills. Science 368 (6490): 482.2-483. https://doi.org/10.1126/science.abb8637.", "Carmack, John. n.d. \"'The Imperial College Epidemic Simulation Code That I Helped a Little on Is Now Public:' / Twitter.\" Twitter. Accessed May 6, 2020. https://twitter.com/id_aa_carmack/status/1254872368763277313.", "Carver, Jeffrey C., Sandra Gesing, Daniel S. Katz, Karthik Ram, and Nicholas Weber. 2018. \"Conceptualization of a US Research Software Sustainability Institute (URSSI).\" Computing in Science & Engineering 20 (3): 4\u20139. https://doi.org/10.1109/MCSE.2018.03221924.", "Cl\u00e9ment-Fontaine, M\u00e9lanie, Roberto Di Cosmo, Bastien Guerry, Patrick MOREAU, and Fran\u00e7ois Pellegrini. 2019. \"Encouraging a Wider Usage of Software Derived from Research.\" Research Report. https://hal.archives-ouvertes.fr/hal-02545142.", "Jim\u00e9nez, Rafael C., Mateusz Kuzak, Monther Alhamdoosh, Michelle Barker, B\u00e9r\u00e9nice Batut, Mikael Borg, Salvador Capella-Gutierrez, et al. 2017. \"Four Simple Recommendations to Encourage Best Practices in Research Software.\" F1000Research 6 (June): 876. https://doi.org/10.12688/f1000research.11407.1.", "Krylov, Anna, Theresa L. Windus, Taylor Barnes, Eliseo Marin-Rimoldi, Jessica A. Nash, Benjamin Pritchard, Daniel G. A. Smith, et al. 2018. \"Perspective: Computational Chemistry Software and Its Advancement as Illustrated through Three Grand Challenge Cases for Molecular Science.\" The Journal of Chemical Physics 149 (18): 180901. https://doi.org/10.1063/1.5052551.", "NSF. 2017. \"Software Infrastructure for Sustained Innovation (SSE, SSI, S2I2): Software Elements, Frameworks and Institute Conceptualizations.\" 2017. https://www.nsf.gov/publications/pub_summ.jsp?ods_key=nsf17526.", "Research Data Alliance. 2020. \"RDA COVID-19 Guidelines and Recommendations.\" RDA. April 23, 2020. https://www.rd-alliance.org/group/rda-covid19-rda-covid19- omics-rda-covid19-epidemiology-rda-covid19-clinical-rda-covid19-0.", "Research Data Alliance. 2020. \"FAIR4RS WG.\" April 28, 2020. https://www.rd-alliance.org/groups/fair- 4-research-software-fair4rs-wg.", "Sheehan, Jeremy. 2016. \"Increasing Access to the Results of Federally Funded Science.\" Whitehouse.Gov. February 22, 2016. https://obamawhitehouse.archives.gov/blog/2016/02/22/increasing-accessresults- federally-funded-science.", "Smith, Arfon M., Daniel S. Katz, Kyle E. Niemeyer, and FORCE11 Software Citation Working Group. 2016. \"Software Citation Principles.\" PeerJ Computer Science 2: e86. https://doi.org/10.7717/peerj-cs.86.", "The HEP Software Foundation, Johannes Albrecht, Antonio Augusto Alves, Guilherme Amadio, Giuseppe Andronico, Nguyen Anh-Ky, Laurent Aphecetche, et al. 2019. \"A Roadmap for HEP Software and Computing R&D for the 2020s.\" Computing and Software for Big Science 3 (1): 7. doi.org/10.1007/s41781-018-0018-8.", "Wilkins-Diehr, Nancy, Michael Zentner, Marlon Pierce, Maytal Dahan, Katherine Lawrence, Linda Hayden, and Nayiri Mullinix. 2018. \"The Science Gateways Community Institute at Two Years.\" In Proceedings of the Practice and Experience on Advanced Research Computing, 1\u20138. Pittsburgh PA USA: ACM. https://doi.org/10.1145/3219104.3219142."]} The Research Software Alliance (ReSA) welcomes this opportunity to inform approaches for ensuring broad public access to the peer-reviewed scholarly publications, data, and code that result from federally-funded scientific research. This submission focuses on how improving the recognition and value of research software can increase the access to unclassified published research, digital scientific data, and code supported by the US Government. ReSA is the international organization representing the research software community. ReSA’s vision is that research software be recognized and valued as a fundamental and vital component of research worldwide.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Research , Other literature type , Preprint 2012Embargo end date: 11 Aug 2016 United KingdomPublisher:Faculty of Economics Funded by:NSF | EFRI: Resilient and Susta...NSF| EFRI: Resilient and Sustainable Interdependent Electric Power and Communications SystemsAuthors: Eager,D.; Hobbs, B.; Bialek, J.;doi: 10.17863/cam.1050
Many governments who preside over liberalised energy markets are developing policies aimed at promoting investment in renewable generation whilst maintaining the level of security of supply customers have come to expect. Of particular interest is the mix and amount of generation investment over time in response to policies promoting high penetrations of variable output renewable power such as wind. Modelling the dynamics of merchant generation investment in market environments can inform the debate. Such models need improved methods to calculate expected output, costs and revenue of thermal generation subject to varying load and random independent thermal outages in a power system with high penetrations of wind. This paper presents a dynamic simulation model of the aggregated Great Britain (GB) generation investment market. The short-term energy market is simulated using probabilistic production costing based on the Mix of Normals distribution technique with a residual load calculation (load net of wind output). Price mark-ups due to market power are accounted for. These models are embedded in a dynamic model in which generation companies use a Value at Risk (VaR) criterion for investment decisions. An `energy-only' market setting is used to estimate the economic profitability of investments and forecast the evolution of security of supply. Simulated results for the GB market case study show a pattern of increased relative security of supply risk during the 2020s. In addition, fixed cost recovery for many new investments can only occur during years in which more frequent supply shortages push energy prices higher. A sensitivity analyses on a number of key model assumptions provides insight into factors affecting the simulated timing and level of generation investment. This is achieved by considering the relative change in simulated levels of security of supply risk metric such as de-rated capacity margins and expected energy unserved. The model can be used as a decision support tool in policy design, in particular how to address the increased `energy-only market revenue risk facing thermal generation, particularly peaking units, that rely on a small number of high price periods to recover fixed costs and make adequate returns on investment.
Research Papers in E... arrow_drop_down All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.17863/cam.1050&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 3 citations 3 popularity Average influence Average impulse Average Powered by BIP!
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For further information contact us at helpdesk@openaire.euResearch data keyboard_double_arrow_right Dataset 2022Publisher:NERC EDS Environmental Information Data Centre Sykes, A.; Vetter, S.H.; Aitkenhead, M.; Dondini, M.; Eory, V.; Goglio, P.; Harris, J.; Hillier, J.; House, J.; Lefebrve, D.; MacLeod, M.; Manning, D.; Medina-Carmona, C.; Mohamed-Yunus, S.; Moran, D.; Myrgiotis, V.; Payen, F.; Rees, B.; Sohi, S.; Williams, M.; Williams, A.; Wollenberg, L.; Smith, P.;The short list of practices is the result of literature review and expert panel input and a step wise process of considering certain critical measures (e.g. increase of soil organic carbon (SOC); greenhouse gas (GHG) emission reduction e.g. carbon dioxide, nitrous oxide, methane; system integration). The list is based on a range of practices already proposed to deliver soil carbon sequestration (SCS). First, specific practices were identified with potential for both a positive impact on SCS at farm level and an uptake rate compatible with global impact. These focus on: (a) optimising crop primary productivity; (b) reducing soil disturbance and managing soil physical properties; (c) minimising deliberate removal of C or lateral transport via erosion; (d) addition of C produced outside the system; (e) provision of additional C inputs within the cropping system. Then, economic and non‐cost barriers and incentives for land managers are considered, along with the potential externalised impacts of implementation. The provided data presents a list of greenhouse gas removal practices for soil organic carbon sequestration, which are suitable under biophysical, economic and social consideration. The list is the result of the first step in analysing the potential of agricultural soils to sequester carbon globally and is part of the NERC funded project Soils-R-GGREAT (NE/P019455/1). The work is based on literature research and expert panel and judgements. The work was supported by the Natural Environment Research Council (NE/P019455/1)
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For further information contact us at helpdesk@openaire.euResearch data keyboard_double_arrow_right Dataset 2023Embargo end date: 26 Jun 2023Publisher:Dryad Authors: Woodruff, Mary J.; Sermersheim, Layne O.; Wolf, Sarah E.; Rosvall, Kimberly A.;Increasingly frequent and intense heatwaves generate new challenges for many organisms. Our understanding of the ecological predictors of thermal vulnerability is improving, yet, at least in endotherms, we are still only beginning to understand one critical component of predicting resilience: exactly how do wild animals cope with sub-lethal heat? In wild endotherms, most prior work focuses on one or a few traits, leaving uncertainty about organismal consequences of heatwaves. Here, we experimentally generated a 2.8 °C heatwave for free-living nestling tree swallows (Tachycineta bicolor). Over a week-long period coinciding with the peak of post-natal growth, we quantified a suite of traits to test the hypotheses that (a) behavioral or (b) physiological responses may be sufficient for coping with inescapable heat. Heat-exposed nestlings increased panting and decreased huddling, but treatment effects on panting dissipated over time, even though heat-induced temperatures remained elevated. Physiologically, we found no effects of heat on: gene expression of three heat shock proteins in blood, muscle, and three brain regions; secretion of circulating corticosterone at baseline or in response to handling; and telomere length. Moreover, heat had a positive effect on growth and a marginal, but not significant, positive effect on subsequent recruitment. These results suggest that nestlings were generally buffered from deleterious effects of heat, with one exception: heat-exposed nestlings exhibited lower gene expression for superoxide dismutase, a key antioxidant defense. Despite this one apparent cost, our thorough organismal investigation indicates general resilience to a heatwave that may, in part, stem from behavioral buffering and acclimation. Our approach provides a mechanistic framework that we hope will improve understanding of species persistence in the face of climate change. See manuscript.
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visibility 11visibility views 11 download downloads 9 Powered bymore_vert All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5061/dryad.s7h44j1c7&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal , Preprint , Other literature type 2014 United Kingdom, Italy, Italy, United Kingdom, Germany, United KingdomPublisher:Springer Nature Funded by:GSRIGSRIAuthors: CERN, 1211, Geneva 23, Switzerland; Aad, G.(CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France); Abbott, B.(Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK, USA); Abdallah, J.(Institute of Physics, Academia Sinica, Taipei, Taiwan); +196 AuthorsCERN, 1211, Geneva 23, Switzerland; Aad, G.(CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France); Abbott, B.(Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK, USA); Abdallah, J.(Institute of Physics, Academia Sinica, Taipei, Taiwan); Abdel Khalek, S.(LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France); Abdinov, O.(Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan); Aben, R.(Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, The Netherlands); Abi, B.(Department of Physics, Oklahoma State University, Stillwater, OK, USA); Abolins, M.(Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA); AbouZeid, O. S.(Department of Physics, University of Toronto, Toronto, ON, Canada); Abramowicz, H.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Abreu, H.(Department of Physics, Technion: Israel Institute of Technology, Haifa, Israel); Abreu, R.(CERN, Geneva, Switzerland); Abulaiti, Y.(Department of Physics, Stockholm University, Stockholm, Sweden; The Oskar Klein Centre, Stockholm, Sweden); Acharya, B. S.(INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine, Italy; ICTP, Trieste, Italy; Dipartimento di Chimica, Fisica e Ambiente, Università di Udine, Udine, Italy); Adamczyk, L.(Faculty of Physics and Applied Computer Science, AGH University of Science and Technology, Kraków, Poland; Marian Smoluchowski Institute of Physics, Jagiellonian University, Kraków, Poland); Adams, D. L.(Physics Department, Brookhaven National Laboratory, Upton, NY, USA); Adelman, J.(Department of Physics, Yale University, New Haven, CT, USA); Adomeit, S.(Fakultät für Physik, Ludwig-Maximilians-Universität München, Munich, Germany); Adye, T.(Particle Physics Department, Rutherford Appleton Laboratory, Didcot, UK); Agatonovic-Jovin, T.(Institute of Physics, University of Belgrade, Belgrade, Serbia; Vinca Institute of Nuclear Sciences, University of Belgrade, Belgrade, Serbia); Aguilar-Saavedra, J. A.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Agustoni, M.(Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University of Bern, Bern, Switzerland); Ahlen, S. P.(Department of Physics, Boston University, Boston, MA, USA); Ahmadov, F.(Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia); Aielli, G.(INFN Sezione di Roma Tor Vergata, Rome, Italy; Dipartimento di Fisica, Università di Roma Tor Vergata, Rome, Italy); Akerstedt, H.(Department of Physics, Stockholm University, Stockholm, Sweden; The Oskar Klein Centre, Stockholm, Sweden); Åkesson, T. P. A.(Fysiska institutionen, Lunds universitet, Lund, Sweden); Akimoto, G.(International Center for Elementary Particle Physics and Department of Physics, The University of Tokyo, Tokyo, Japan); Akimov, A. V.(P.N. Lebedev Institute of Physics, Academy of Sciences, Moscow, Russia); Alberghi, G. L.(INFN Sezione di Bologna, Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy); Albert, J.(Department of Physics and Astronomy, University of Victoria, Victoria, BC, Canada); Albrand, S.(Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France); Alconada Verzini, M. J.(Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina); Aleksa, M.(CERN, Geneva, Switzerland); Aleksandrov, I. N.(Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia); Alexa, C.(National Institute of Physics and Nuclear Engineering, Bucharest, Romania; Physics Department, National Institute for Research and Development of Isotopic and Molecular Technologies, Cluj Napoca, Romania; University Politehnica Bucharest, Bucharest, Romania; West University in Timisoara, Timisoara, Romania); Alexander, G.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Alexandre, G.(Section de Physique, Université de Genève, Geneva, Switzerland); Alexopoulos, T.(Physics Department, National Technical University of Athens, Zografou, Greece); Alhroob, M.(INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine, Italy; ICTP, Trieste, Italy; Dipartimento di Chimica, Fisica e Ambiente, Università di Udine, Udine, Italy); Alimonti, G.(INFN Sezione di Milano, Milan, Italy; Dipartimento di Fisica, Università di Milano, Milan, Italy); Alio, L.(CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France); Alison, J.(Enrico Fermi Institute, University of Chicago, Chicago, IL, USA); Allbrooke, B. M. M.(School of Physics and Astronomy, University of Birmingham, Birmingham, UK); Allison, L. J.(Physics Department, Lancaster University, Lancaster, UK); Allport, P. P.(Oliver Lodge Laboratory, University of Liverpool, Liverpool, UK); Almond, J.(School of Physics and Astronomy, University of Manchester, Manchester, UK); Aloisio, A.(INFN Sezione di Napoli, Naples, Italy; Dipartimento di Fisica, Università di Napoli, Naples, Italy); Alonso, A.(Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark); Alonso, F.(Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina); Alpigiani, C.(School of Physics and Astronomy, Queen Mary University of London, London, UK); Altheimer, A.(Nevis Laboratory, Columbia University, Irvington, NY, USA); Alvarez Gonzalez, B.(Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA); Alviggi, M. G.(INFN Sezione di Napoli, Naples, Italy; Dipartimento di Fisica, Università di Napoli, Naples, Italy); Amako, K.(KEK, High Energy Accelerator Research Organization, Tsukuba, Japan); Amaral Coutinho, Y.(Universidade Federal do Rio De Janeiro COPPE/EE/IF, Rio de Janeiro, Brazil; Federal University of Juiz de Fora (UFJF), Juiz de Fora, Brazil; Federal University of Sao Joao del Rei (UFSJ), Sao Joao del Rei, Brazil; Instituto de Fisica, Universidade de Sao Paulo, São Paulo, Brazil); Amelung, C.(Department of Physics, Brandeis University, Waltham, MA, USA); Amidei, D.(Department of Physics, The University of Michigan, Ann Arbor, MI, USA); Amor Dos Santos, S. P.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Amorim, A.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Amoroso, S.(Fakultät für Mathematik und Physik, Albert-Ludwigs-Universität, Freiburg, Germany); Amram, N.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Amundsen, G.(Department of Physics, Brandeis University, Waltham, MA, USA); Anastopoulos, C.(Department of Physics and Astronomy, University of Sheffield, Sheffield, UK); Ancu, L. S.(Section de Physique, Université de Genève, Geneva, Switzerland); Andari, N.(CERN, Geneva, Switzerland); Andeen, T.(Nevis Laboratory, Columbia University, Irvington, NY, USA); Anders, C. F.(Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; ZITI Institut für technische Informatik, Ruprecht-Karls-Universität Heidelberg, Mannheim, Germany); Anders, G.(CERN, Geneva, Switzerland); Anderson, K. J.(Enrico Fermi Institute, University of Chicago, Chicago, IL, USA); Andreazza, A.(INFN Sezione di Milano, Milan, Italy; Dipartimento di Fisica, Università di Milano, Milan, Italy); Andrei, V.(Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; ZITI Institut für technische Informatik, Ruprecht-Karls-Universität Heidelberg, Mannheim, Germany); Anduaga, X. S.(Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina); Angelidakis, S.(Physics Department, University of Athens, Athens, Greece); Angelozzi, I.(Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, The Netherlands); Anger, P.(Institut für Kern- und Teilchenphysik, Technische Universität Dresden, Dresden, Germany); Angerami, A.(Nevis Laboratory, Columbia University, Irvington, NY, USA); Anghinolfi, F.(CERN, Geneva, Switzerland); Anisenkov, A. V.(Budker Institute of Nuclear Physics, SB RAS, Novosibirsk, Russia); Anjos, N.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Annovi, A.(INFN Laboratori Nazionali di Frascati, Frascati, Italy); Antonaki, A.(Physics Department, University of Athens, Athens, Greece); Antonelli, M.(INFN Laboratori Nazionali di Frascati, Frascati, Italy); Antonov, A.(Moscow Engineering and Physics Institute (MEPhI), Moscow, Russia); Antos, J.(Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovak Republic; Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic); Anulli, F.(INFN Sezione di Roma, Rome, Italy; Dipartimento di Fisica, Sapienza Università di Roma, Rome, Italy); Aoki, M.(KEK, High Energy Accelerator Research Organization, Tsukuba, Japan); Aperio Bella, L.(School of Physics and Astronomy, University of Birmingham, Birmingham, UK); Apolle, R.(Department of Physics, Oxford University, Oxford, UK); Arabidze, G.(Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA); Aracena, I.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Arai, Y.(KEK, High Energy Accelerator Research Organization, Tsukuba, Japan); Araque, J. P.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Arce, A. T. H.(Department of Physics, Duke University, Durham, NC, USA); Arguin, J-F.(Group of Particle Physics, University of Montreal, Montreal, QC, Canada); Argyropoulos, S.(DESY, Hamburg and Zeuthen, Germany); Arik, M.(Department of Physics, Bogazici University, Istanbul, Turkey; Department of Physics, Dogus University, Istanbul, Turkey; Department of Physics Engineering, Gaziantep University, Gaziantep, Turkey); Armbruster, A. J.(CERN, Geneva, Switzerland); Arnaez, O.(CERN, Geneva, Switzerland); Arnal, V.(Departamento de Fisica Teorica C-15, Universidad Autonoma de Madrid, Madrid, Spain); Arnold, H.(Fakultät für Mathematik und Physik, Albert-Ludwigs-Universität, Freiburg, Germany); Arratia, M.(Cavendish Laboratory, University of Cambridge, Cambridge, UK); Arslan, O.(Physikalisches Institut, University of Bonn, Bonn, Germany); Artamonov, A.(Institute for Theoretical and Experimental Physics (ITEP), Moscow, Russia); Artoni, G.(Department of Physics, Brandeis University, Waltham, MA, USA); Asai, S.(International Center for Elementary Particle Physics and Department of Physics, The University of Tokyo, Tokyo, Japan); Asbah, N.(DESY, Hamburg and Zeuthen, Germany); Ashkenazi, A.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Åsman, B.(Department of Physics, Stockholm University, Stockholm, Sweden; The Oskar Klein Centre, Stockholm, Sweden); Asquith, L.(High Energy Physics Division, Argonne National Laboratory, Argonne, IL, USA); Assamagan, K.(Physics Department, Brookhaven National Laboratory, Upton, NY, USA); Astalos, R.(Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovak Republic; Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic); Atkinson, M.(Department of Physics, University of Illinois, Urbana, IL, USA); Atlay, N. B.(Fachbereich Physik, Universität Siegen, Siegen, Germany); Auerbach, B.(High Energy Physics Division, Argonne National Laboratory, Argonne, IL, USA); Augsten, K.(Czech Technical University in Prague, Prague, Czech Republic); Aurousseau, M.(Department of Physics, University of Cape Town, Cape Town, South Africa; Department of Physics, University of Johannesburg, Johannesburg, South Africa; School of Physics, University of the Witwatersrand, Johannesburg, South Africa); Avolio, G.(CERN, Geneva, Switzerland); Azuelos, G.(Group of Particle Physics, University of Montreal, Montreal, QC, Canada); Azuma, Y.(International Center for Elementary Particle Physics and Department of Physics, The University of Tokyo, Tokyo, Japan); Baak, M. A.(CERN, Geneva, Switzerland); Baas, A.(Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; ZITI Institut für technische Informatik, Ruprecht-Karls-Universität Heidelberg, Mannheim, Germany); Bacci, C.(INFN Sezione di Roma Tre, Rome, Italy; Dipartimento di Matematica e Fisica, Università Roma Tre, Rome, Italy); Bachacou, H.(DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l’Univers), CEA Saclay (Commissariat à l’Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France); Bachas, K.(Department of Physics, Aristotle University of Thessaloniki, Thessaloniki, Greece); Backes, M.(CERN, Geneva, Switzerland); Backhaus, M.(CERN, Geneva, Switzerland); Backus Mayes, J.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Badescu, E.(National Institute of Physics and Nuclear Engineering, Bucharest, Romania; Physics Department, National Institute for Research and Development of Isotopic and Molecular Technologies, Cluj Napoca, Romania; University Politehnica Bucharest, Bucharest, Romania; West University in Timisoara, Timisoara, Romania); Bagiacchi, P.(INFN Sezione di Roma, Rome, Italy; Dipartimento di Fisica, Sapienza Università di Roma, Rome, Italy); Bagnaia, P.(INFN Sezione di Roma, Rome, Italy; Dipartimento di Fisica, Sapienza Università di Roma, Rome, Italy); Bai, Y.(Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China; Department of Modern Physics, University of Science and Technology of China, Hefei, Anhui, China; Department of Physics, Nanjing University, Nanjing, Jiangsu, China; School of Physics, Shandong University, Jinan, Shandong, China; Physics Department, Shanghai Jiao Tong University, Shanghai, China); Bain, T.(Nevis Laboratory, Columbia University, Irvington, NY, USA); Baines, J. T.(Particle Physics Department, Rutherford Appleton Laboratory, Didcot, UK); Baker, O. K.(Department of Physics, Yale University, New Haven, CT, USA); Balek, P.(Faculty of Mathematics and Physics, Charles University in Prague, Prague, Czech Republic); Balli, F.(DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l’Univers), CEA Saclay (Commissariat à l’Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France); Banas, E.(The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Kraków, Poland); Banerjee, Sw.(Department of Physics, University of Wisconsin, Madison, WI, USA); Bannoura, A. A. E.(Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany); Bansal, V.(Department of Physics and Astronomy, University of Victoria, Victoria, BC, Canada); Bansil, H. S.(School of Physics and Astronomy, University of Birmingham, Birmingham, UK); Barak, L.(Department of Particle Physics, The Weizmann Institute of Science, Rehovot, Israel); Baranov, S. P.(P.N. Lebedev Institute of Physics, Academy of Sciences, Moscow, Russia); Barberio, E. L.(School of Physics, University of Melbourne, Parkville, VIC, Australia); Barberis, D.(INFN Sezione di Genova, Genoa, Italy; Dipartimento di Fisica, Università di Genova, Genova, Italy); Barbero, M.(CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France); Barillari, T.(Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Munich, Germany); Barisonzi, M.(Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany); Barklow, T.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Barlow, N.(Cavendish Laboratory, University of Cambridge, Cambridge, UK); Barnett, B. M.(Particle Physics Department, Rutherford Appleton Laboratory, Didcot, UK); Barnett, R. M.(Physics Division, Lawrence Berkeley National Laboratory and University of California, Berkeley, CA, USA); Barnovska, Z.(LAPP, CNRS/IN2P3 and Université de Savoie, Annecy-le-Vieux, France); Baroncelli, A.(INFN Sezione di Roma Tre, Rome, Italy; Dipartimento di Matematica e Fisica, Università Roma Tre, Rome, Italy); Barone, G.(Section de Physique, Université de Genève, Geneva, Switzerland); Barr, A. J.(Department of Physics, Oxford University, Oxford, UK); Barreiro, F.(Departamento de Fisica Teorica C-15, Universidad Autonoma de Madrid, Madrid, Spain); Barreiro Guimarães da Costa, J.(Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge, MA, USA); Bartoldus, R.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Barton, A. E.(Physics Department, Lancaster University, Lancaster, UK); Bartos, P.(Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovak Republic; Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic); Bartsch, V.(Department of Physics and Astronomy, University of Sussex, Brighton, UK); Bassalat, A.(LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France); Basye, A.(Department of Physics, University of Illinois, Urbana, IL, USA); Bates, R. L.(SUPA-School of Physics and Astronomy, University of Glasgow, Glasgow, UK); Batley, J. R.(Cavendish Laboratory, University of Cambridge, Cambridge, UK); Battaglia, M.(Santa Cruz Institute for Particle Physics, University of California Santa Cruz, Santa Cruz, CA, USA); Battistin, M.(CERN, Geneva, Switzerland); Bauer, F.(DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l’Univers), CEA Saclay (Commissariat à l’Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France); Bawa, H. S.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Beattie, M. D.(Physics Department, Lancaster University, Lancaster, UK); Beau, T.(Laboratoire de Physique Nucléaire et de Hautes Energies, UPMC and Université Paris-Diderot and CNRS/IN2P3, Paris, France); Beauchemin, P. H.(Department of Physics and Astronomy, Tufts University, Medford, MA, USA); Beccherle, R.(INFN Sezione di Pisa, Pisa, Italy; Dipartimento di Fisica E. Fermi, Università di Pisa, Pisa, Italy); Bechtle, P.(Physikalisches Institut, University of Bonn, Bonn, Germany); Beck, H. P.(Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University of Bern, Bern, Switzerland); Becker, K.(Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany); Becker, S.(Fakultät für Physik, Ludwig-Maximilians-Universität München, Munich, Germany); Beckingham, M.(Department of Physics, University of Warwick, Coventry, UK); Becot, C.(LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France); Beddall, A. J.(Department of Physics, Bogazici University, Istanbul, Turkey; Department of Physics, Dogus University, Istanbul, Turkey; Department of Physics Engineering, Gaziantep University, Gaziantep, Turkey); Beddall, A.(Department of Physics, Bogazici University, Istanbul, Turkey; Department of Physics, Dogus University, Istanbul, Turkey; Department of Physics Engineering, Gaziantep University, Gaziantep, Turkey); Bedikian, S.(Department of Physics, Yale University, New Haven, CT, USA); Bednyakov, V. A.(Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia); Bee, C. P.(Departments of Physics and Astronomy and Chemistry, Stony Brook University, Stony Brook, NY, USA); Beemster, L. J.(Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, The Netherlands); Beermann, T. A.(Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany); Begel, M.(Physics Department, Brookhaven National Laboratory, Upton, NY, USA); Behr, K.(Department of Physics, Oxford University, Oxford, UK); Belanger-Champagne, C.(Department of Physics, McGill University, Montreal, QC, Canada); Bell, P. J.(Section de Physique, Université de Genève, Geneva, Switzerland); Bell, W. H.(Section de Physique, Université de Genève, Geneva, Switzerland); Bella, G.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Bellagamba, L.(INFN Sezione di Bologna, Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy); Bellerive, A.(Department of Physics, Carleton University, Ottawa, ON, Canada); Bellomo, M.(Department of Physics, University of Massachusetts, Amherst, MA, USA); Belotskiy, K.(Moscow Engineering and Physics Institute (MEPhI), Moscow, Russia); Beltramello, O.(CERN, Geneva, Switzerland);handle: 2434/242885
This paper presents the electron and photon energy calibration achieved with the ATLAS detector using about 25 fb −1 of LHC proton–proton collision data taken at centre-of-mass energies of s√=7 and 8 TeV. The reconstruction of electron and photon energies is optimised using multivariate algorithms. The response of the calorimeter layers is equalised in data and simulation, and the longitudinal profile of the electromagnetic showers is exploited to estimate the passive material in front of the calorimeter and reoptimise the detector simulation. After all corrections, the Z resonance is used to set the absolute energy scale. For electrons from Z decays, the achieved calibration is typically accurate to 0.05 % in most of the detector acceptance, rising to 0.2 % in regions with large amounts of passive material. The remaining inaccuracy is less than 0.2–1 % for electrons with a transverse energy of 10 GeV, and is on average 0.3 % for photons. The detector resolution is determined with a relative inaccuracy of less than 10 % for electrons and photons up to 60 GeV transverse energy, rising to 40 % for transverse energies above 500 GeV.
CORE arrow_drop_down COREArticle . 2014License: CC BYFull-Text: https://eprints.gla.ac.uk/99642/2/99642.pdfData sources: COREEnlightenArticle . 2014License: CC BYFull-Text: http://eprints.gla.ac.uk/99642/2/99642.pdfData sources: CORE (RIOXX-UK Aggregator)European Physical Journal C: Particles and FieldsArticle . 2014Data sources: Oxford University Research ArchiveQueen Mary University of London: Queen Mary Research Online (QMRO)Article . 2014Data sources: Bielefeld Academic Search Engine (BASE)All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=2434/242885&type=result"></script>'); --> </script>
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more_vert CORE arrow_drop_down COREArticle . 2014License: CC BYFull-Text: https://eprints.gla.ac.uk/99642/2/99642.pdfData sources: COREEnlightenArticle . 2014License: CC BYFull-Text: http://eprints.gla.ac.uk/99642/2/99642.pdfData sources: CORE (RIOXX-UK Aggregator)European Physical Journal C: Particles and FieldsArticle . 2014Data sources: Oxford University Research ArchiveQueen Mary University of London: Queen Mary Research Online (QMRO)Article . 2014Data sources: Bielefeld Academic Search Engine (BASE)All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=2434/242885&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2014Embargo end date: 08 Feb 2019 Belgium, Norway, United Kingdom, Italy, Germany, United Kingdom, Portugal, United Kingdom, France, Brazil, United Kingdom, Germany, United Kingdom, United Kingdom, Australia, United Kingdom, United Kingdom, Brazil, France, United KingdomPublisher:Wiley Publicly fundedFunded by:UKRI | Global modelling of local..., FCT | LA 1, UKRI | RootDetect: Remote Detect... +1 projectsUKRI| Global modelling of local biodiversity responses to human impacts ,FCT| LA 1 ,UKRI| RootDetect: Remote Detection and Precision Management of Root Health ,UKRI| Doctoral Training GrantLionel Hernández; Jodi L. Sedlock; Matthew J. Struebig; Vânia Proença; Eike Lena Neuschulz; Åke Berg; Martin Jung; Carolina L. Morales; Biagio D'Aniello; Kristoffer Hylander; Tom M. Fayle; Tom M. Fayle; Tom M. Fayle; Masahiro Ishitani; Carolina A. Robles; Vassiliki Kati; Virginia Aguilar-Barquero; Pedro Beja; Norbertas Noreika; Alexis Cerezo; Juan Paritsis; Szabolcs Sáfián; Nina Farwig; Steven J. Presley; Jörg Brunet; Oliver Schweiger; Thibault Lachat; T. Keith Philips; Igor Lysenko; Nick A. Littlewood; Stephen J. Rossiter; William Oduro; Kiril Vassilev; Michelle L K Harrison; Robert M. Ewers; Loreta Rosselli; Ulrika Samnegård; Felix Herzog; Alvin J. Helden; James I. Watling; Niall O'Dea; Olivia Norfolk; Víctor H. Luja; Carlos A. Peres; Eliana Martínez; Michael R. Willig; Jimmy Cabra-García; Douglas Sheil; Douglas Sheil; J. Leighton Reid; Tim Diekötter; Tim Diekötter; Nicolás Pelegrin; Antonio Felicioli; Lauchlan H. Fraser; Hollie Booth; Hollie Booth; Gilbert B. Adum; Grzegorz Mikusiński; Victoria Lantschner; Paola J. Isaacs-Cubides; Nor Rasidah Hashim; Annika M. Felton; Lawrence N. Hudson; Tibor Magura; Susan G. Letcher; Akihiro Nakamura; Anelena L Carvalho; Birgit Jauker; Béla Tóthmérész; Neil Aldrin D. Mallari; Neil Aldrin D. Mallari; Marco Silva Gottschalk; Eleanor M. Slade; Andrey S. Zaitsev; Shoji Naoe; Carsten F. Dormann; Mats Jonsell; Diego Higuera-Diaz; Lars Edenius; Péter Batáry; Violette Le Féon; Ben Darvill; Alain Dejean; Alain Dejean; Erin M. Bayne; Carlos H. Vergara; Luz Piedad Romero-Duque; Mick E. Hanley; Christopher D. Williams; Christian Hébert; Isabel Brito; Rolando Cerda; Yana T. Reis; Gretchen LeBuhn; Erika Buscardo; Erika Buscardo; Bertrand Dumont; James R. Miller; Jenni G. Garden; Lucinda Kirkpatrick; Allan H. Smith-Pardo; Allan H. Smith-Pardo; Dario Furlani; John-André Henden; Jochen H. Bihn; Yik Hei Sung; James Grogan; Manuel Esteban Lucas-Borja; John C. Z. Woinarski; Ádám Kőrösi; Ádám Kőrösi; Kaoru Maeto; Gábor L. Lövei; Stefan Abrahamczyk; Paolo Giordani; Lander Baeten; Morgan Garon; Argyrios Choimes; Argyrios Choimes; Danilo Bandini Ribeiro; Inge Armbrecht; Laurent Rousseau; Theodora Petanidou; Helena Castro; Mary N Muchane; Nicole M. Nöske; Nicholas J. Berry; Fernando A. B. Silva; Guiomar Nates-Parra; Pedro Giovâni da Silva; Muchai Muchane; Hannah J. White; Mats Dynesius; Bruno K. C. Filgueiras; Eric Katovai; Jörg U. Ganzhorn; Mounir Louhaichi; Christof Schüepp; Jort Verhulst; Stuart Connop; Matthieu Chauvat; Vena Kapoor; Katja Poveda; Marcelo A. Aizen; Eva Knop; Jörn P. W. Scharlemann; Jörn P. W. Scharlemann; Caragh G. Threlfall; Aaron D. Gove; Aaron D. Gove; Jonathan P. Sadler; Job Aben; Daniel F. R. Cleary; Erika Marin-Spiotta; Caleb Ofori-Boateng; Caleb Ofori-Boateng; Victoria Kemp; Dario A Navarrete Gutierrez; Francis Q. Brearley; Yanping Wang; David L P Correia; Jean-Philippe Légaré; Marino Quaranta; Gentile Francesco Ficetola; Adam J. Vanbergen; Zoltán Elek; Sydney A. Cameron; Jane C. Stout; Chris O. Oke; Ben Collen; Jorge Ari Noriega; Jörg Römbke; Ramón A. Sosa; Simon G. Dures; Simon G. Dures; Alejandro A. Castro-Luna; Joseph E. Hawes; Joseph E. Hawes; Adriana De Palma; Adriana De Palma; Steven J. Fonte; Hans Verboven; Marc Ancrenaz; Andy Purvis; Andy Purvis; Helen Phillips; Helen Phillips; Barbara A. Richardson; Daisuke Fukuda; Carlos A. López-Quintero; Yuan Pan; Badrul Azhar; Katrin Böhning-Gaese; Alejandro Parra-H; Alejandro Parra-H; Ben Phalan; Rebecca A. Senior; Navjot S. Sodhi; Jos Barlow;doi: 10.17863/cam.36177
pmc: PMC4278822
Biodiversity continues to decline in the face of increasing anthropogenic pressures such as habitat destruction, exploitation, pollution and introduction of alien species. Existing global databases of species' threat status or population time series are dominated by charismatic species. The collation of datasets with broad taxonomic and biogeographic extents, and that support computation of a range of biodiversity indicators, is necessary to enable better understanding of historical declines and to project - and avert - future declines. We describe and assess a new database of more than 1.6 million samples from 78 countries representing over 28,000 species, collated from existing spatial comparisons of local-scale biodiversity exposed to different intensities and types of anthropogenic pressures, from terrestrial sites around the world. The database contains measurements taken in 208 (of 814) ecoregions, 13 (of 14) biomes, 25 (of 35) biodiversity hotspots and 16 (of 17) megadiverse countries. The database contains more than 1% of the total number of all species described, and more than 1% of the described species within many taxonomic groups - including flowering plants, gymnosperms, birds, mammals, reptiles, amphibians, beetles, lepidopterans and hymenopterans. The dataset, which is still being added to, is therefore already considerably larger and more representative than those used by previous quantitative models of biodiversity trends and responses. The database is being assembled as part of the PREDICTS project (Projecting Responses of Ecological Diversity In Changing Terrestrial Systems - http://www.predicts.org.uk). We make site-level summary data available alongside this article. The full database will be publicly available in 2015.
CORE arrow_drop_down Repositório do INPAArticle . 2014License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)James Cook University, Australia: ResearchOnline@JCUArticle . 2014Full-Text: http://dx.doi.org/10.1002/ece3.1303Data sources: Bielefeld Academic Search Engine (BASE)Imperial College London: SpiralArticle . 2015License: CC BYFull-Text: http://hdl.handle.net/10044/1/23623Data sources: Bielefeld Academic Search Engine (BASE)Queen Mary University of London: Queen Mary Research Online (QMRO)Article . 2017License: CC BYData sources: Bielefeld Academic Search Engine (BASE)CGIAR CGSpace (Consultative Group on International Agricultural Research)Article . 2015License: CC BYFull-Text: https://hdl.handle.net/10568/68192Data sources: Bielefeld Academic Search Engine (BASE)The University of Melbourne: Digital RepositoryArticle . 2014License: CC BYFull-Text: http://hdl.handle.net/11343/263351Data sources: Bielefeld Academic Search Engine (BASE)Publikationenserver der Georg-August-Universität GöttingenArticle . 2014 . Peer-reviewedLicense: CC BYRepositório Institucional da Universidade de AveiroArticle . 2014Data sources: Repositório Institucional da Universidade de AveiroHochschulschriftenserver - Universität Frankfurt am MainArticle . 2017Data sources: Hochschulschriftenserver - Universität Frankfurt am MainMunin - Open Research ArchiveArticle . 2014 . Peer-reviewedData sources: Munin - Open Research ArchiveQueen's University Belfast Research PortalArticle . 2014Data sources: Bielefeld Academic Search Engine (BASE)Publication Server of Goethe University Frankfurt am MainArticle . 2017License: CC BYData sources: Bielefeld Academic Search Engine (BASE)University of East Anglia: UEA Digital RepositoryArticle . 2014Data sources: Bielefeld Academic Search Engine (BASE)All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.17863/cam.36177&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 155 citations 155 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!
visibility 87visibility views 87 download downloads 186 Powered bymore_vert CORE arrow_drop_down Repositório do INPAArticle . 2014License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)James Cook University, Australia: ResearchOnline@JCUArticle . 2014Full-Text: http://dx.doi.org/10.1002/ece3.1303Data sources: Bielefeld Academic Search Engine (BASE)Imperial College London: SpiralArticle . 2015License: CC BYFull-Text: http://hdl.handle.net/10044/1/23623Data sources: Bielefeld Academic Search Engine (BASE)Queen Mary University of London: Queen Mary Research Online (QMRO)Article . 2017License: CC BYData sources: Bielefeld Academic Search Engine (BASE)CGIAR CGSpace (Consultative Group on International Agricultural Research)Article . 2015License: CC BYFull-Text: https://hdl.handle.net/10568/68192Data sources: Bielefeld Academic Search Engine (BASE)The University of Melbourne: Digital RepositoryArticle . 2014License: CC BYFull-Text: http://hdl.handle.net/11343/263351Data sources: Bielefeld Academic Search Engine (BASE)Publikationenserver der Georg-August-Universität GöttingenArticle . 2014 . Peer-reviewedLicense: CC BYRepositório Institucional da Universidade de AveiroArticle . 2014Data sources: Repositório Institucional da Universidade de AveiroHochschulschriftenserver - Universität Frankfurt am MainArticle . 2017Data sources: Hochschulschriftenserver - Universität Frankfurt am MainMunin - Open Research ArchiveArticle . 2014 . Peer-reviewedData sources: Munin - Open Research ArchiveQueen's University Belfast Research PortalArticle . 2014Data sources: Bielefeld Academic Search Engine (BASE)Publication Server of Goethe University Frankfurt am MainArticle . 2017License: CC BYData sources: Bielefeld Academic Search Engine (BASE)University of East Anglia: UEA Digital RepositoryArticle . 2014Data sources: Bielefeld Academic Search Engine (BASE)All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.17863/cam.36177&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2002 ItalyPublisher:Kluwer Academic, Boston , Paesi Bassi Neil L. Rose; Roland Psenner; Andrea Lami; Anna Agusti-Panareda; Peter G. Appleby; Øyvind A. Schnell; Richard Tessadri; Roy Thompson; Karin A. Koinig; Karin A. Koinig; Christian Kamenik; Roland Schmidt; Miroslava Prazakova;Changes in microfossils (diatoms, chrysophytes, chironomids and cladocera remains), geochemistry and deposition of atmospheric pollutants have been investigated in the sediment records of the alpine lake Gossenkollesee ( Tyrol, Austria) spanning the last two centuries. The sediment records were compared with seasonal and annual air temperature trends calculated for the elevation (2417 m a. s. l.) and the geographical position (47degrees13'46"N, 11degrees00'51"E) of the lake, and with precipitation records available since 1866 from Innsbruck. Temperature trends followed a 20 30 year oscillation between cold and warm periods. Regarding long-term changes, temperature trends showed a U-shaped trend between 1780 and 1950, followed by a steep increase since 1975.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Other literature type 2023Publisher:OpenAlex Lewis G. Halsey; Vincent Careau; Philip N. Ainslie; Heliodoro Alemán-Mateo; Lene Frost Andersen; Liam Anderson; Lenore Arab; Issad Baddou; Linda G. Bandini; Kweku Bedu-Addo; Ellen E. Blaak; Stéphane Blanc; A. Bonomi; Carlijn V. C. Bouten; Pascal Bovet; Søren Brage; Maciej S. Buchowski; Nancy F. Butte; Stefan Gerardus Camps; Regina C. Casper; Graeme L. Close; Lisa H. Colbert; Jamie A. Cooper; Richard Cooper; Prasangi Dabare; Sai Krupa Das; Peter S. W. Davies; Sanjoy Deb; Christine Delisle Nyström; William H. Dietz; Lara R. Dugas; Simon Eaton; Ulf Ekelund; Asmaa El Hamdouchi; Sonja Entringer; Terrence Forrester; Barry W. Fudge; Melanie B. Gillingham; Annelies H. C. Goris; Michael Gurven; Hinke Haisma; Catherine Hambly; Daniel Hoffman; Marije B. Hoos; Sumei Hu; Noorjehan Joonas; Annemiek Joosen; Peter T. Katzmarzyk; Kitty P. Kempen; Misaka Kimura; William E. Kraus; Wantanee Kriengsinyos; Rebecca Kuriyan; Robert F. Kushner; Estelle V. Lambert; Pulani Lanerolle; Christel Larsson; Nader Lessan; Marie Löf; Corby K. Martin; Eric Matsiko; G.A.L. Meijer; James C. Morehen; James P. Morton; Aviva Must; Marian L. Neuhouser; Theresa A. Nicklas; Robert Ojiambo; Kirsi H. Pietiläinen; Yannis Pitsiladis; Jacob Plange‐Rhule; Guy Plasqui; Ross L. Prentice; Roberto Rabinovich; Susan B. Racette; David A Raichen; Éric Ravussin; Leanne M. Redman; John J. Reilly; Rebecca M. Reynolds; Susan B. Roberts; Dulani Samaranayake; Luís B. Sardinha; Albertine J. Schuit; Analiza M. Silva; Srishti Sinha; Anders Sjödin; Eric Stice; Albert J. Stunkard; Samuel S. Urlacher; Mauro E. Valencia; Giulio Valenti; Ludo M. Van Etten; Edgar A. Van Mil; Jeanine A. Verbunt; Jonathan C. K. Wells; George Wilson; Brian M. Wood; Tsukasa Yoshida; Xueying Zhang;Il existe une variation considérablement plus importante des taux métaboliques entre les hommes qu'entre les femmes, en termes de dépense énergétique (EE) basale, d'activité et totale (quotidienne). Une explication possible est que l'EE est associée à des caractéristiques sexuelles masculines (qui sont connues pour varier plus que d'autres traits) telles que la musculature et la capacité athlétique. De tels traits pourraient être prédits pour être les plus importants pendant les périodes de l'adolescence et du début de l'âge adulte, lorsque le comportement sexuel se développe et culmine. Nous avons testé cette hypothèse sur un grand ensemble de données en comparant la quantité de variation masculine et la variation féminine de l'EE totale, de l'EE d'activité et de l'EE basale, à différents stades de la vie, ainsi que plusieurs traits morphologiques : hauteur, masse sans graisse et masse grasse. L'EE totale, et dans une certaine mesure aussi l'activité EE, présentent une variation masculine (GMV) considérablement plus importante chez les jeunes adultes, puis une diminution du degré de GMV chez les individus de plus en plus âgés. On peut soutenir que l'EE basale, ainsi que la morphométrie, ne présentent pas ce motif. Ces résultats suggèrent que les caractéristiques sexuelles masculines uniques peuvent ne pas présenter de pic de GMV chez les jeunes adultes, mais l'activité totale et peut-être aussi l'activité EE, associées à de nombreux traits morphologiques et physiologiques combinés, présentent le GMV le plus en évidence au cours des étapes de la vie reproductive. Existe una variación considerablemente mayor en las tasas metabólicas entre los hombres que entre las mujeres, en términos de gasto energético (EE) basal, de actividad y total (diario). Una posible explicación es que la EE se asocia con características sexuales masculinas (que se sabe que varían más que otros rasgos) como la musculatura y la capacidad atlética. Se podría predecir que tales rasgos son más prominentes durante los períodos de adolescencia y adultez temprana, cuando el comportamiento sexual se desarrolla y alcanza su punto máximo. Probamos esta hipótesis en un gran conjunto de datos comparando la cantidad de variación masculina y la variación femenina en EE total, EE de actividad y EE basal, en diferentes etapas de la vida, junto con varios rasgos morfológicos: altura, masa libre de grasa y masa grasa. La EE total, y hasta cierto punto también la EE de actividad, exhiben una variación masculina (GMV) considerablemente mayor en adultos jóvenes, y luego una disminución en el grado de GMV en individuos progresivamente mayores. Podría decirse que el EE basal, y también la morfometría, no exhiben este patrón. Estos hallazgos sugieren que las características sexuales masculinas individuales pueden no exhibir un GMV máximo en la edad adulta joven, sin embargo, el EE total y quizás también la actividad, asociada con muchos rasgos morfológicos y fisiológicos combinados, exhiben el GMV de manera más prominente durante las etapas de la vida reproductiva. There is considerably greater variation in metabolic rates between men than between women, in terms of basal, activity and total (daily) energy expenditure (EE). One possible explanation is that EE is associated with male sexual characteristics (which are known to vary more than other traits) such as musculature and athletic capacity. Such traits might be predicted to be most prominent during periods of adolescence and young adulthood, when sexual behaviour develops and peaks. We tested this hypothesis on a large dataset by comparing the amount of male variation and female variation in total EE, activity EE and basal EE, at different life stages, along with several morphological traits: height, fat free mass and fat mass. Total EE, and to some degree also activity EE, exhibit considerable greater male variation (GMV) in young adults, and then a decrease in the degree of GMV in progressively older individuals. Arguably, basal EE, and also morphometrics, do not exhibit this pattern. These findings suggest that single male sexual characteristics may not exhibit peak GMV in young adulthood, however total and perhaps also activity EE, associated with many morphological and physiological traits combined, do exhibit GMV most prominently during the reproductive life stages. هناك تباين أكبر بكثير في معدلات التمثيل الغذائي بين الرجال منه بين النساء، من حيث الإنفاق الأساسي والنشاط وإجمالي الطاقة (اليومية). أحد التفسيرات المحتملة هو أن EE يرتبط بالخصائص الجنسية للذكور (والتي من المعروف أنها تختلف أكثر من السمات الأخرى) مثل العضلات والقدرة الرياضية. قد يُتوقع أن تكون هذه السمات أكثر بروزًا خلال فترات المراهقة ومرحلة الشباب، عندما يتطور السلوك الجنسي ويصل إلى ذروته. اختبرنا هذه الفرضية على مجموعة بيانات كبيرة من خلال مقارنة كمية تباين الذكور وتباين الإناث في إجمالي الطاقة الكهربائية والنشاط والطاقة الكهربائية القاعدية، في مراحل الحياة المختلفة، إلى جانب العديد من السمات المورفولوجية: الطول والكتلة الخالية من الدهون وكتلة الدهون. يُظهر إجمالي التقييم البيئي، وإلى حد ما أيضًا نشاط التقييم البيئي، تباينًا أكبر بكثير بين الذكور (GMV) لدى الشباب، ثم انخفاضًا في درجة التقييم الطبي العام لدى الأفراد الأكبر سنًا بشكل تدريجي. يمكن القول إن EE القاعدية، وكذلك القياسات الشكلية، لا تظهر هذا النمط. تشير هذه النتائج إلى أن الخصائص الجنسية للذكور العازبين قد لا تظهر ذروة GMV في مرحلة الشباب، ولكن إجمالي وربما أيضًا النشاط EE، المرتبط بالعديد من السمات المورفولوجية والفسيولوجية مجتمعة، يظهر GMV بشكل بارز خلال مراحل الحياة الإنجابية.
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Research data keyboard_double_arrow_right Dataset 2023Publisher:World Data Center for Climate (WDCC) at DKRZ Authors: von Schuckmann, Karina; Minière, Audrey; Gues, Flora; Cuesta-Valero, Francisco José; +58 Authorsvon Schuckmann, Karina; Minière, Audrey; Gues, Flora; Cuesta-Valero, Francisco José; Kirchengast, Gottfried; Adusumilli, Susheel; Straneo, Fiammetta; Allan, Richard; Barker, Paul M.; Beltrami, Hugo; Boyer, Tim; Cheng, Lijing; Church, John; Desbruyeres, Damien; Dolman, Han; Domingues, Catia M.; García-García, Almudena; Gilson, John; Gorfer, Maximilian; Haimberger, Leopold; Hendricks, Stefan; Hosoda, Shigeki; Johnson, Gregory C.; Killick, Rachel; King, Brian A.; Kolodziejczyk, Nicolas; Korosov, Anton; Krinner, Gerhard; Kuusela, Mikael; Langer, Moritz; Lavergne, Thomas; Lawrence, Isobel; Li, Yuehua; Lyman, John; Marzeion, Ben; Mayer, Michael; MacDougall, Andrew; McDougall, Trevor; Monselesan, Didier Paolo; Nitzbon, Jean; Otosaka, Inès; Peng, Jian; Purkey, Sarah; Roemmich, Dean; Sato, Kanako; Sato, Katsunari; Savita, Abhishek; Schweiger, Axel; Shepherd, Andrew; Seneviratne, Sonia I.; Slater, Donald A.; Slater, Thomas; Simons, Leon; Steiner, Andrea K.; Szekely, Tanguy; Suga, Toshio; Thiery, Wim; Timmermanns, Mary-Louise; Vanderkelen, Inne; Wijffels, Susan E.; Wu, Tonghua; Zemp, Michael;Project: GCOS Earth Heat Inventory - A study under the Global Climate Observing System (GCOS) concerted international effort to update the Earth heat inventory (EHI), and presents an updated international assessment of ocean warming estimates, and new and updated estimates of heat gain in the atmosphere, cryosphere and land over the period from 1960 to present. Summary: The file “GCOS_EHI_1960-2020_Earth_Heat_Inventory_Ocean_Heat_Content_data.nc” contains a consistent long-term Earth system heat inventory over the period 1960-2020. Human-induced atmospheric composition changes cause a radiative imbalance at the top-of-atmosphere which is driving global warming. Understanding the heat gain of the Earth system from this accumulated heat – and particularly how much and where the heat is distributed in the Earth system - is fundamental to understanding how this affects warming oceans, atmosphere and land, rising temperatures and sea level, and loss of grounded and floating ice, which are fundamental concerns for society. This dataset is based on a study under the Global Climate Observing System (GCOS) concerted international effort to update the Earth heat inventory published in von Schuckmann et al. (2020), and presents an updated international assessment of ocean warming estimates, and new and updated estimates of heat gain in the atmosphere, cryosphere and land over the period 1960-2020. The dataset also contains estimates for global ocean heat content over 1960-2020 for different depth layers, i.e., 0-300m, 0-700m, 700-2000m, 0-2000m, 2000-bottom, which are described in von Schuckmann et al. (2022). This version includes an update of heat storage of global ocean heat content, where one additional product (Li et al., 2022) had been included to the initial estimate. The Earth heat inventory had been updated accordingly, considering also the update for continental heat content (Cuesta-Valero et al., 2023).
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2017 SpainPublisher:AMER PHYSICAL SOC Funded by:EC | ANDESEC| ANDESWright, T.; Guerrero, C.; Billowes, J.; Calviño Tavares, Francisco; Cortés Rossell, Guillem Pere;handle: 2117/115901
The radiative capture cross section of a highly pure (99.999%), 6.125(2) grams and 9.56(5)E-4 atoms/barn areal density 238U sample has been measured with the Total Absorption Calorimeter (TAC) in the 185 m flight path at the CERN neutron time-of-flight facility n_TOF. This measurement is in response to the NEA High Priority Request list, which demands an accuracy in this cross section of less than 3% below 25 keV. These data have undergone careful background subtraction, with special care being given to the background originating from neutrons scattered by the 238U sample. Pileup and dead-time effects have been corrected for. The measured cross section covers an energy range between 0.2 eV and 80 keV, with an accuracy that varies with neutron energy, being better than 4% below 25 keV and reaching at most 6% at higher energies.
Universitat Politècn... arrow_drop_down Universitat Politècnica de Catalunya, BarcelonaTech: UPCommons - Global access to UPC knowledgeArticle . 2017License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)Recolector de Ciencia Abierta, RECOLECTAArticle . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticleData sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPCArticle . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCAll Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=2117/115901&type=result"></script>'); --> </script>
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more_vert Universitat Politècn... arrow_drop_down Universitat Politècnica de Catalunya, BarcelonaTech: UPCommons - Global access to UPC knowledgeArticle . 2017License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)Recolector de Ciencia Abierta, RECOLECTAArticle . 2017License: CC BY NC NDData sources: Recolector de Ciencia Abierta, RECOLECTARecolector de Ciencia Abierta, RECOLECTAArticleData sources: Recolector de Ciencia Abierta, RECOLECTAUPCommons. Portal del coneixement obert de la UPCArticle . 2017License: CC BY NC NDData sources: UPCommons. Portal del coneixement obert de la UPCAll Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=2117/115901&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Research , Other literature type 2020Publisher:Zenodo Barker, Michelle; Katz, Daniel S.; Chue Hong, Neil P.; Mentzel, Chris; Ram, Karthik; Jones, Catherine; Treloar, Andrew;{"references": ["Adam, David. 2020. \"Special Report: The Simulations Driving the World's Response to COVID-19.\" Nature 580 (7803): 316\u201318. doi.org/10.1038/d41586-020-01003-6.", "Akhmerov, Anton, Maria Cruz, Niels Drost, Cees Hof, Tomas Knapen, Mateusz Kuzak, Carlos Martinez-Ortiz, Yasemin Turkyilmaz-van der Velden, and Ben van Werkhoven. 2019. \"Raising the Profile of Research Software,\" August. https://doi.org/10.5281/ZENODO.3378572.", "Barton, C. Michael, Marina Alberti, Daniel Ames, Jo-An Atkinson, Jerad Bales, Edmund 5 Burke, Min Chen, et al. 2020. \"Call for Transparency of COVID-19 Models.\" Edited by Jennifer Sills. Science 368 (6490): 482.2-483. https://doi.org/10.1126/science.abb8637.", "Carmack, John. n.d. \"'The Imperial College Epidemic Simulation Code That I Helped a Little on Is Now Public:' / Twitter.\" Twitter. Accessed May 6, 2020. https://twitter.com/id_aa_carmack/status/1254872368763277313.", "Carver, Jeffrey C., Sandra Gesing, Daniel S. Katz, Karthik Ram, and Nicholas Weber. 2018. \"Conceptualization of a US Research Software Sustainability Institute (URSSI).\" Computing in Science & Engineering 20 (3): 4\u20139. https://doi.org/10.1109/MCSE.2018.03221924.", "Cl\u00e9ment-Fontaine, M\u00e9lanie, Roberto Di Cosmo, Bastien Guerry, Patrick MOREAU, and Fran\u00e7ois Pellegrini. 2019. \"Encouraging a Wider Usage of Software Derived from Research.\" Research Report. https://hal.archives-ouvertes.fr/hal-02545142.", "Jim\u00e9nez, Rafael C., Mateusz Kuzak, Monther Alhamdoosh, Michelle Barker, B\u00e9r\u00e9nice Batut, Mikael Borg, Salvador Capella-Gutierrez, et al. 2017. \"Four Simple Recommendations to Encourage Best Practices in Research Software.\" F1000Research 6 (June): 876. https://doi.org/10.12688/f1000research.11407.1.", "Krylov, Anna, Theresa L. Windus, Taylor Barnes, Eliseo Marin-Rimoldi, Jessica A. Nash, Benjamin Pritchard, Daniel G. A. Smith, et al. 2018. \"Perspective: Computational Chemistry Software and Its Advancement as Illustrated through Three Grand Challenge Cases for Molecular Science.\" The Journal of Chemical Physics 149 (18): 180901. https://doi.org/10.1063/1.5052551.", "NSF. 2017. \"Software Infrastructure for Sustained Innovation (SSE, SSI, S2I2): Software Elements, Frameworks and Institute Conceptualizations.\" 2017. https://www.nsf.gov/publications/pub_summ.jsp?ods_key=nsf17526.", "Research Data Alliance. 2020. \"RDA COVID-19 Guidelines and Recommendations.\" RDA. April 23, 2020. https://www.rd-alliance.org/group/rda-covid19-rda-covid19- omics-rda-covid19-epidemiology-rda-covid19-clinical-rda-covid19-0.", "Research Data Alliance. 2020. \"FAIR4RS WG.\" April 28, 2020. https://www.rd-alliance.org/groups/fair- 4-research-software-fair4rs-wg.", "Sheehan, Jeremy. 2016. \"Increasing Access to the Results of Federally Funded Science.\" Whitehouse.Gov. February 22, 2016. https://obamawhitehouse.archives.gov/blog/2016/02/22/increasing-accessresults- federally-funded-science.", "Smith, Arfon M., Daniel S. Katz, Kyle E. Niemeyer, and FORCE11 Software Citation Working Group. 2016. \"Software Citation Principles.\" PeerJ Computer Science 2: e86. https://doi.org/10.7717/peerj-cs.86.", "The HEP Software Foundation, Johannes Albrecht, Antonio Augusto Alves, Guilherme Amadio, Giuseppe Andronico, Nguyen Anh-Ky, Laurent Aphecetche, et al. 2019. \"A Roadmap for HEP Software and Computing R&D for the 2020s.\" Computing and Software for Big Science 3 (1): 7. doi.org/10.1007/s41781-018-0018-8.", "Wilkins-Diehr, Nancy, Michael Zentner, Marlon Pierce, Maytal Dahan, Katherine Lawrence, Linda Hayden, and Nayiri Mullinix. 2018. \"The Science Gateways Community Institute at Two Years.\" In Proceedings of the Practice and Experience on Advanced Research Computing, 1\u20138. Pittsburgh PA USA: ACM. https://doi.org/10.1145/3219104.3219142."]} The Research Software Alliance (ReSA) welcomes this opportunity to inform approaches for ensuring broad public access to the peer-reviewed scholarly publications, data, and code that result from federally-funded scientific research. This submission focuses on how improving the recognition and value of research software can increase the access to unclassified published research, digital scientific data, and code supported by the US Government. ReSA is the international organization representing the research software community. ReSA’s vision is that research software be recognized and valued as a fundamental and vital component of research worldwide.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Research , Other literature type , Preprint 2012Embargo end date: 11 Aug 2016 United KingdomPublisher:Faculty of Economics Funded by:NSF | EFRI: Resilient and Susta...NSF| EFRI: Resilient and Sustainable Interdependent Electric Power and Communications SystemsAuthors: Eager,D.; Hobbs, B.; Bialek, J.;doi: 10.17863/cam.1050
Many governments who preside over liberalised energy markets are developing policies aimed at promoting investment in renewable generation whilst maintaining the level of security of supply customers have come to expect. Of particular interest is the mix and amount of generation investment over time in response to policies promoting high penetrations of variable output renewable power such as wind. Modelling the dynamics of merchant generation investment in market environments can inform the debate. Such models need improved methods to calculate expected output, costs and revenue of thermal generation subject to varying load and random independent thermal outages in a power system with high penetrations of wind. This paper presents a dynamic simulation model of the aggregated Great Britain (GB) generation investment market. The short-term energy market is simulated using probabilistic production costing based on the Mix of Normals distribution technique with a residual load calculation (load net of wind output). Price mark-ups due to market power are accounted for. These models are embedded in a dynamic model in which generation companies use a Value at Risk (VaR) criterion for investment decisions. An `energy-only' market setting is used to estimate the economic profitability of investments and forecast the evolution of security of supply. Simulated results for the GB market case study show a pattern of increased relative security of supply risk during the 2020s. In addition, fixed cost recovery for many new investments can only occur during years in which more frequent supply shortages push energy prices higher. A sensitivity analyses on a number of key model assumptions provides insight into factors affecting the simulated timing and level of generation investment. This is achieved by considering the relative change in simulated levels of security of supply risk metric such as de-rated capacity margins and expected energy unserved. The model can be used as a decision support tool in policy design, in particular how to address the increased `energy-only market revenue risk facing thermal generation, particularly peaking units, that rely on a small number of high price periods to recover fixed costs and make adequate returns on investment.
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For further information contact us at helpdesk@openaire.euResearch data keyboard_double_arrow_right Dataset 2022Publisher:NERC EDS Environmental Information Data Centre Sykes, A.; Vetter, S.H.; Aitkenhead, M.; Dondini, M.; Eory, V.; Goglio, P.; Harris, J.; Hillier, J.; House, J.; Lefebrve, D.; MacLeod, M.; Manning, D.; Medina-Carmona, C.; Mohamed-Yunus, S.; Moran, D.; Myrgiotis, V.; Payen, F.; Rees, B.; Sohi, S.; Williams, M.; Williams, A.; Wollenberg, L.; Smith, P.;The short list of practices is the result of literature review and expert panel input and a step wise process of considering certain critical measures (e.g. increase of soil organic carbon (SOC); greenhouse gas (GHG) emission reduction e.g. carbon dioxide, nitrous oxide, methane; system integration). The list is based on a range of practices already proposed to deliver soil carbon sequestration (SCS). First, specific practices were identified with potential for both a positive impact on SCS at farm level and an uptake rate compatible with global impact. These focus on: (a) optimising crop primary productivity; (b) reducing soil disturbance and managing soil physical properties; (c) minimising deliberate removal of C or lateral transport via erosion; (d) addition of C produced outside the system; (e) provision of additional C inputs within the cropping system. Then, economic and non‐cost barriers and incentives for land managers are considered, along with the potential externalised impacts of implementation. The provided data presents a list of greenhouse gas removal practices for soil organic carbon sequestration, which are suitable under biophysical, economic and social consideration. The list is the result of the first step in analysing the potential of agricultural soils to sequester carbon globally and is part of the NERC funded project Soils-R-GGREAT (NE/P019455/1). The work is based on literature research and expert panel and judgements. The work was supported by the Natural Environment Research Council (NE/P019455/1)
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For further information contact us at helpdesk@openaire.euResearch data keyboard_double_arrow_right Dataset 2023Embargo end date: 26 Jun 2023Publisher:Dryad Authors: Woodruff, Mary J.; Sermersheim, Layne O.; Wolf, Sarah E.; Rosvall, Kimberly A.;Increasingly frequent and intense heatwaves generate new challenges for many organisms. Our understanding of the ecological predictors of thermal vulnerability is improving, yet, at least in endotherms, we are still only beginning to understand one critical component of predicting resilience: exactly how do wild animals cope with sub-lethal heat? In wild endotherms, most prior work focuses on one or a few traits, leaving uncertainty about organismal consequences of heatwaves. Here, we experimentally generated a 2.8 °C heatwave for free-living nestling tree swallows (Tachycineta bicolor). Over a week-long period coinciding with the peak of post-natal growth, we quantified a suite of traits to test the hypotheses that (a) behavioral or (b) physiological responses may be sufficient for coping with inescapable heat. Heat-exposed nestlings increased panting and decreased huddling, but treatment effects on panting dissipated over time, even though heat-induced temperatures remained elevated. Physiologically, we found no effects of heat on: gene expression of three heat shock proteins in blood, muscle, and three brain regions; secretion of circulating corticosterone at baseline or in response to handling; and telomere length. Moreover, heat had a positive effect on growth and a marginal, but not significant, positive effect on subsequent recruitment. These results suggest that nestlings were generally buffered from deleterious effects of heat, with one exception: heat-exposed nestlings exhibited lower gene expression for superoxide dismutase, a key antioxidant defense. Despite this one apparent cost, our thorough organismal investigation indicates general resilience to a heatwave that may, in part, stem from behavioral buffering and acclimation. Our approach provides a mechanistic framework that we hope will improve understanding of species persistence in the face of climate change. See manuscript.
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visibility 11visibility views 11 download downloads 9 Powered bymore_vert All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5061/dryad.s7h44j1c7&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal , Preprint , Other literature type 2014 United Kingdom, Italy, Italy, United Kingdom, Germany, United KingdomPublisher:Springer Nature Funded by:GSRIGSRIAuthors: CERN, 1211, Geneva 23, Switzerland; Aad, G.(CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France); Abbott, B.(Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK, USA); Abdallah, J.(Institute of Physics, Academia Sinica, Taipei, Taiwan); +196 AuthorsCERN, 1211, Geneva 23, Switzerland; Aad, G.(CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France); Abbott, B.(Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK, USA); Abdallah, J.(Institute of Physics, Academia Sinica, Taipei, Taiwan); Abdel Khalek, S.(LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France); Abdinov, O.(Institute of Physics, Azerbaijan Academy of Sciences, Baku, Azerbaijan); Aben, R.(Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, The Netherlands); Abi, B.(Department of Physics, Oklahoma State University, Stillwater, OK, USA); Abolins, M.(Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA); AbouZeid, O. S.(Department of Physics, University of Toronto, Toronto, ON, Canada); Abramowicz, H.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Abreu, H.(Department of Physics, Technion: Israel Institute of Technology, Haifa, Israel); Abreu, R.(CERN, Geneva, Switzerland); Abulaiti, Y.(Department of Physics, Stockholm University, Stockholm, Sweden; The Oskar Klein Centre, Stockholm, Sweden); Acharya, B. S.(INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine, Italy; ICTP, Trieste, Italy; Dipartimento di Chimica, Fisica e Ambiente, Università di Udine, Udine, Italy); Adamczyk, L.(Faculty of Physics and Applied Computer Science, AGH University of Science and Technology, Kraków, Poland; Marian Smoluchowski Institute of Physics, Jagiellonian University, Kraków, Poland); Adams, D. L.(Physics Department, Brookhaven National Laboratory, Upton, NY, USA); Adelman, J.(Department of Physics, Yale University, New Haven, CT, USA); Adomeit, S.(Fakultät für Physik, Ludwig-Maximilians-Universität München, Munich, Germany); Adye, T.(Particle Physics Department, Rutherford Appleton Laboratory, Didcot, UK); Agatonovic-Jovin, T.(Institute of Physics, University of Belgrade, Belgrade, Serbia; Vinca Institute of Nuclear Sciences, University of Belgrade, Belgrade, Serbia); Aguilar-Saavedra, J. A.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Agustoni, M.(Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University of Bern, Bern, Switzerland); Ahlen, S. P.(Department of Physics, Boston University, Boston, MA, USA); Ahmadov, F.(Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia); Aielli, G.(INFN Sezione di Roma Tor Vergata, Rome, Italy; Dipartimento di Fisica, Università di Roma Tor Vergata, Rome, Italy); Akerstedt, H.(Department of Physics, Stockholm University, Stockholm, Sweden; The Oskar Klein Centre, Stockholm, Sweden); Åkesson, T. P. A.(Fysiska institutionen, Lunds universitet, Lund, Sweden); Akimoto, G.(International Center for Elementary Particle Physics and Department of Physics, The University of Tokyo, Tokyo, Japan); Akimov, A. V.(P.N. Lebedev Institute of Physics, Academy of Sciences, Moscow, Russia); Alberghi, G. L.(INFN Sezione di Bologna, Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy); Albert, J.(Department of Physics and Astronomy, University of Victoria, Victoria, BC, Canada); Albrand, S.(Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France); Alconada Verzini, M. J.(Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina); Aleksa, M.(CERN, Geneva, Switzerland); Aleksandrov, I. N.(Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia); Alexa, C.(National Institute of Physics and Nuclear Engineering, Bucharest, Romania; Physics Department, National Institute for Research and Development of Isotopic and Molecular Technologies, Cluj Napoca, Romania; University Politehnica Bucharest, Bucharest, Romania; West University in Timisoara, Timisoara, Romania); Alexander, G.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Alexandre, G.(Section de Physique, Université de Genève, Geneva, Switzerland); Alexopoulos, T.(Physics Department, National Technical University of Athens, Zografou, Greece); Alhroob, M.(INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine, Italy; ICTP, Trieste, Italy; Dipartimento di Chimica, Fisica e Ambiente, Università di Udine, Udine, Italy); Alimonti, G.(INFN Sezione di Milano, Milan, Italy; Dipartimento di Fisica, Università di Milano, Milan, Italy); Alio, L.(CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France); Alison, J.(Enrico Fermi Institute, University of Chicago, Chicago, IL, USA); Allbrooke, B. M. M.(School of Physics and Astronomy, University of Birmingham, Birmingham, UK); Allison, L. J.(Physics Department, Lancaster University, Lancaster, UK); Allport, P. P.(Oliver Lodge Laboratory, University of Liverpool, Liverpool, UK); Almond, J.(School of Physics and Astronomy, University of Manchester, Manchester, UK); Aloisio, A.(INFN Sezione di Napoli, Naples, Italy; Dipartimento di Fisica, Università di Napoli, Naples, Italy); Alonso, A.(Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark); Alonso, F.(Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina); Alpigiani, C.(School of Physics and Astronomy, Queen Mary University of London, London, UK); Altheimer, A.(Nevis Laboratory, Columbia University, Irvington, NY, USA); Alvarez Gonzalez, B.(Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA); Alviggi, M. G.(INFN Sezione di Napoli, Naples, Italy; Dipartimento di Fisica, Università di Napoli, Naples, Italy); Amako, K.(KEK, High Energy Accelerator Research Organization, Tsukuba, Japan); Amaral Coutinho, Y.(Universidade Federal do Rio De Janeiro COPPE/EE/IF, Rio de Janeiro, Brazil; Federal University of Juiz de Fora (UFJF), Juiz de Fora, Brazil; Federal University of Sao Joao del Rei (UFSJ), Sao Joao del Rei, Brazil; Instituto de Fisica, Universidade de Sao Paulo, São Paulo, Brazil); Amelung, C.(Department of Physics, Brandeis University, Waltham, MA, USA); Amidei, D.(Department of Physics, The University of Michigan, Ann Arbor, MI, USA); Amor Dos Santos, S. P.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Amorim, A.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Amoroso, S.(Fakultät für Mathematik und Physik, Albert-Ludwigs-Universität, Freiburg, Germany); Amram, N.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Amundsen, G.(Department of Physics, Brandeis University, Waltham, MA, USA); Anastopoulos, C.(Department of Physics and Astronomy, University of Sheffield, Sheffield, UK); Ancu, L. S.(Section de Physique, Université de Genève, Geneva, Switzerland); Andari, N.(CERN, Geneva, Switzerland); Andeen, T.(Nevis Laboratory, Columbia University, Irvington, NY, USA); Anders, C. F.(Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; ZITI Institut für technische Informatik, Ruprecht-Karls-Universität Heidelberg, Mannheim, Germany); Anders, G.(CERN, Geneva, Switzerland); Anderson, K. J.(Enrico Fermi Institute, University of Chicago, Chicago, IL, USA); Andreazza, A.(INFN Sezione di Milano, Milan, Italy; Dipartimento di Fisica, Università di Milano, Milan, Italy); Andrei, V.(Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; ZITI Institut für technische Informatik, Ruprecht-Karls-Universität Heidelberg, Mannheim, Germany); Anduaga, X. S.(Instituto de Física La Plata, Universidad Nacional de La Plata and CONICET, La Plata, Argentina); Angelidakis, S.(Physics Department, University of Athens, Athens, Greece); Angelozzi, I.(Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, The Netherlands); Anger, P.(Institut für Kern- und Teilchenphysik, Technische Universität Dresden, Dresden, Germany); Angerami, A.(Nevis Laboratory, Columbia University, Irvington, NY, USA); Anghinolfi, F.(CERN, Geneva, Switzerland); Anisenkov, A. V.(Budker Institute of Nuclear Physics, SB RAS, Novosibirsk, Russia); Anjos, N.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Annovi, A.(INFN Laboratori Nazionali di Frascati, Frascati, Italy); Antonaki, A.(Physics Department, University of Athens, Athens, Greece); Antonelli, M.(INFN Laboratori Nazionali di Frascati, Frascati, Italy); Antonov, A.(Moscow Engineering and Physics Institute (MEPhI), Moscow, Russia); Antos, J.(Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovak Republic; Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic); Anulli, F.(INFN Sezione di Roma, Rome, Italy; Dipartimento di Fisica, Sapienza Università di Roma, Rome, Italy); Aoki, M.(KEK, High Energy Accelerator Research Organization, Tsukuba, Japan); Aperio Bella, L.(School of Physics and Astronomy, University of Birmingham, Birmingham, UK); Apolle, R.(Department of Physics, Oxford University, Oxford, UK); Arabidze, G.(Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA); Aracena, I.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Arai, Y.(KEK, High Energy Accelerator Research Organization, Tsukuba, Japan); Araque, J. P.(Laboratorio de Instrumentacao e Fisica Experimental de Particulas-LIP, Lisbon, Portugal; Faculdade de Ciências, Universidade de Lisboa, Lisbon, Portugal; Department of Physics, University of Coimbra, Coimbra, Portugal; Centro de Física Nuclear da Universidade de Lisboa, Lisbon, Portugal; Departamento de Fisica, Universidade do Minho, Braga, Portugal; Departamento de Fisica Teorica y del Cosmos and CAFPE, Universidad de Granada, Granada, Spain; Dep Fisica and CEFITEC of Faculdade de Ciencias e Tecnologia, Universidade Nova de Lisboa, Caparica, Portugal); Arce, A. T. H.(Department of Physics, Duke University, Durham, NC, USA); Arguin, J-F.(Group of Particle Physics, University of Montreal, Montreal, QC, Canada); Argyropoulos, S.(DESY, Hamburg and Zeuthen, Germany); Arik, M.(Department of Physics, Bogazici University, Istanbul, Turkey; Department of Physics, Dogus University, Istanbul, Turkey; Department of Physics Engineering, Gaziantep University, Gaziantep, Turkey); Armbruster, A. J.(CERN, Geneva, Switzerland); Arnaez, O.(CERN, Geneva, Switzerland); Arnal, V.(Departamento de Fisica Teorica C-15, Universidad Autonoma de Madrid, Madrid, Spain); Arnold, H.(Fakultät für Mathematik und Physik, Albert-Ludwigs-Universität, Freiburg, Germany); Arratia, M.(Cavendish Laboratory, University of Cambridge, Cambridge, UK); Arslan, O.(Physikalisches Institut, University of Bonn, Bonn, Germany); Artamonov, A.(Institute for Theoretical and Experimental Physics (ITEP), Moscow, Russia); Artoni, G.(Department of Physics, Brandeis University, Waltham, MA, USA); Asai, S.(International Center for Elementary Particle Physics and Department of Physics, The University of Tokyo, Tokyo, Japan); Asbah, N.(DESY, Hamburg and Zeuthen, Germany); Ashkenazi, A.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Åsman, B.(Department of Physics, Stockholm University, Stockholm, Sweden; The Oskar Klein Centre, Stockholm, Sweden); Asquith, L.(High Energy Physics Division, Argonne National Laboratory, Argonne, IL, USA); Assamagan, K.(Physics Department, Brookhaven National Laboratory, Upton, NY, USA); Astalos, R.(Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovak Republic; Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic); Atkinson, M.(Department of Physics, University of Illinois, Urbana, IL, USA); Atlay, N. B.(Fachbereich Physik, Universität Siegen, Siegen, Germany); Auerbach, B.(High Energy Physics Division, Argonne National Laboratory, Argonne, IL, USA); Augsten, K.(Czech Technical University in Prague, Prague, Czech Republic); Aurousseau, M.(Department of Physics, University of Cape Town, Cape Town, South Africa; Department of Physics, University of Johannesburg, Johannesburg, South Africa; School of Physics, University of the Witwatersrand, Johannesburg, South Africa); Avolio, G.(CERN, Geneva, Switzerland); Azuelos, G.(Group of Particle Physics, University of Montreal, Montreal, QC, Canada); Azuma, Y.(International Center for Elementary Particle Physics and Department of Physics, The University of Tokyo, Tokyo, Japan); Baak, M. A.(CERN, Geneva, Switzerland); Baas, A.(Kirchhoff-Institut für Physik, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany; ZITI Institut für technische Informatik, Ruprecht-Karls-Universität Heidelberg, Mannheim, Germany); Bacci, C.(INFN Sezione di Roma Tre, Rome, Italy; Dipartimento di Matematica e Fisica, Università Roma Tre, Rome, Italy); Bachacou, H.(DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l’Univers), CEA Saclay (Commissariat à l’Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France); Bachas, K.(Department of Physics, Aristotle University of Thessaloniki, Thessaloniki, Greece); Backes, M.(CERN, Geneva, Switzerland); Backhaus, M.(CERN, Geneva, Switzerland); Backus Mayes, J.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Badescu, E.(National Institute of Physics and Nuclear Engineering, Bucharest, Romania; Physics Department, National Institute for Research and Development of Isotopic and Molecular Technologies, Cluj Napoca, Romania; University Politehnica Bucharest, Bucharest, Romania; West University in Timisoara, Timisoara, Romania); Bagiacchi, P.(INFN Sezione di Roma, Rome, Italy; Dipartimento di Fisica, Sapienza Università di Roma, Rome, Italy); Bagnaia, P.(INFN Sezione di Roma, Rome, Italy; Dipartimento di Fisica, Sapienza Università di Roma, Rome, Italy); Bai, Y.(Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China; Department of Modern Physics, University of Science and Technology of China, Hefei, Anhui, China; Department of Physics, Nanjing University, Nanjing, Jiangsu, China; School of Physics, Shandong University, Jinan, Shandong, China; Physics Department, Shanghai Jiao Tong University, Shanghai, China); Bain, T.(Nevis Laboratory, Columbia University, Irvington, NY, USA); Baines, J. T.(Particle Physics Department, Rutherford Appleton Laboratory, Didcot, UK); Baker, O. K.(Department of Physics, Yale University, New Haven, CT, USA); Balek, P.(Faculty of Mathematics and Physics, Charles University in Prague, Prague, Czech Republic); Balli, F.(DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l’Univers), CEA Saclay (Commissariat à l’Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France); Banas, E.(The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Kraków, Poland); Banerjee, Sw.(Department of Physics, University of Wisconsin, Madison, WI, USA); Bannoura, A. A. E.(Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany); Bansal, V.(Department of Physics and Astronomy, University of Victoria, Victoria, BC, Canada); Bansil, H. S.(School of Physics and Astronomy, University of Birmingham, Birmingham, UK); Barak, L.(Department of Particle Physics, The Weizmann Institute of Science, Rehovot, Israel); Baranov, S. P.(P.N. Lebedev Institute of Physics, Academy of Sciences, Moscow, Russia); Barberio, E. L.(School of Physics, University of Melbourne, Parkville, VIC, Australia); Barberis, D.(INFN Sezione di Genova, Genoa, Italy; Dipartimento di Fisica, Università di Genova, Genova, Italy); Barbero, M.(CPPM, Aix-Marseille Université and CNRS/IN2P3, Marseille, France); Barillari, T.(Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Munich, Germany); Barisonzi, M.(Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany); Barklow, T.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Barlow, N.(Cavendish Laboratory, University of Cambridge, Cambridge, UK); Barnett, B. M.(Particle Physics Department, Rutherford Appleton Laboratory, Didcot, UK); Barnett, R. M.(Physics Division, Lawrence Berkeley National Laboratory and University of California, Berkeley, CA, USA); Barnovska, Z.(LAPP, CNRS/IN2P3 and Université de Savoie, Annecy-le-Vieux, France); Baroncelli, A.(INFN Sezione di Roma Tre, Rome, Italy; Dipartimento di Matematica e Fisica, Università Roma Tre, Rome, Italy); Barone, G.(Section de Physique, Université de Genève, Geneva, Switzerland); Barr, A. J.(Department of Physics, Oxford University, Oxford, UK); Barreiro, F.(Departamento de Fisica Teorica C-15, Universidad Autonoma de Madrid, Madrid, Spain); Barreiro Guimarães da Costa, J.(Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge, MA, USA); Bartoldus, R.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Barton, A. E.(Physics Department, Lancaster University, Lancaster, UK); Bartos, P.(Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovak Republic; Department of Subnuclear Physics, Institute of Experimental Physics of the Slovak Academy of Sciences, Kosice, Slovak Republic); Bartsch, V.(Department of Physics and Astronomy, University of Sussex, Brighton, UK); Bassalat, A.(LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France); Basye, A.(Department of Physics, University of Illinois, Urbana, IL, USA); Bates, R. L.(SUPA-School of Physics and Astronomy, University of Glasgow, Glasgow, UK); Batley, J. R.(Cavendish Laboratory, University of Cambridge, Cambridge, UK); Battaglia, M.(Santa Cruz Institute for Particle Physics, University of California Santa Cruz, Santa Cruz, CA, USA); Battistin, M.(CERN, Geneva, Switzerland); Bauer, F.(DSM/IRFU (Institut de Recherches sur les Lois Fondamentales de l’Univers), CEA Saclay (Commissariat à l’Energie Atomique et aux Energies Alternatives), Gif-sur-Yvette, France); Bawa, H. S.(SLAC National Accelerator Laboratory, Stanford, CA, USA); Beattie, M. D.(Physics Department, Lancaster University, Lancaster, UK); Beau, T.(Laboratoire de Physique Nucléaire et de Hautes Energies, UPMC and Université Paris-Diderot and CNRS/IN2P3, Paris, France); Beauchemin, P. H.(Department of Physics and Astronomy, Tufts University, Medford, MA, USA); Beccherle, R.(INFN Sezione di Pisa, Pisa, Italy; Dipartimento di Fisica E. Fermi, Università di Pisa, Pisa, Italy); Bechtle, P.(Physikalisches Institut, University of Bonn, Bonn, Germany); Beck, H. P.(Albert Einstein Center for Fundamental Physics and Laboratory for High Energy Physics, University of Bern, Bern, Switzerland); Becker, K.(Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany); Becker, S.(Fakultät für Physik, Ludwig-Maximilians-Universität München, Munich, Germany); Beckingham, M.(Department of Physics, University of Warwick, Coventry, UK); Becot, C.(LAL, Université Paris-Sud and CNRS/IN2P3, Orsay, France); Beddall, A. J.(Department of Physics, Bogazici University, Istanbul, Turkey; Department of Physics, Dogus University, Istanbul, Turkey; Department of Physics Engineering, Gaziantep University, Gaziantep, Turkey); Beddall, A.(Department of Physics, Bogazici University, Istanbul, Turkey; Department of Physics, Dogus University, Istanbul, Turkey; Department of Physics Engineering, Gaziantep University, Gaziantep, Turkey); Bedikian, S.(Department of Physics, Yale University, New Haven, CT, USA); Bednyakov, V. A.(Joint Institute for Nuclear Research, JINR Dubna, Dubna, Russia); Bee, C. P.(Departments of Physics and Astronomy and Chemistry, Stony Brook University, Stony Brook, NY, USA); Beemster, L. J.(Nikhef National Institute for Subatomic Physics and University of Amsterdam, Amsterdam, The Netherlands); Beermann, T. A.(Fachbereich C Physik, Bergische Universität Wuppertal, Wuppertal, Germany); Begel, M.(Physics Department, Brookhaven National Laboratory, Upton, NY, USA); Behr, K.(Department of Physics, Oxford University, Oxford, UK); Belanger-Champagne, C.(Department of Physics, McGill University, Montreal, QC, Canada); Bell, P. J.(Section de Physique, Université de Genève, Geneva, Switzerland); Bell, W. H.(Section de Physique, Université de Genève, Geneva, Switzerland); Bella, G.(Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel); Bellagamba, L.(INFN Sezione di Bologna, Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, Bologna, Italy); Bellerive, A.(Department of Physics, Carleton University, Ottawa, ON, Canada); Bellomo, M.(Department of Physics, University of Massachusetts, Amherst, MA, USA); Belotskiy, K.(Moscow Engineering and Physics Institute (MEPhI), Moscow, Russia); Beltramello, O.(CERN, Geneva, Switzerland);handle: 2434/242885
This paper presents the electron and photon energy calibration achieved with the ATLAS detector using about 25 fb −1 of LHC proton–proton collision data taken at centre-of-mass energies of s√=7 and 8 TeV. The reconstruction of electron and photon energies is optimised using multivariate algorithms. The response of the calorimeter layers is equalised in data and simulation, and the longitudinal profile of the electromagnetic showers is exploited to estimate the passive material in front of the calorimeter and reoptimise the detector simulation. After all corrections, the Z resonance is used to set the absolute energy scale. For electrons from Z decays, the achieved calibration is typically accurate to 0.05 % in most of the detector acceptance, rising to 0.2 % in regions with large amounts of passive material. The remaining inaccuracy is less than 0.2–1 % for electrons with a transverse energy of 10 GeV, and is on average 0.3 % for photons. The detector resolution is determined with a relative inaccuracy of less than 10 % for electrons and photons up to 60 GeV transverse energy, rising to 40 % for transverse energies above 500 GeV.
CORE arrow_drop_down COREArticle . 2014License: CC BYFull-Text: https://eprints.gla.ac.uk/99642/2/99642.pdfData sources: COREEnlightenArticle . 2014License: CC BYFull-Text: http://eprints.gla.ac.uk/99642/2/99642.pdfData sources: CORE (RIOXX-UK Aggregator)European Physical Journal C: Particles and FieldsArticle . 2014Data sources: Oxford University Research ArchiveQueen Mary University of London: Queen Mary Research Online (QMRO)Article . 2014Data sources: Bielefeld Academic Search Engine (BASE)All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=2434/242885&type=result"></script>'); --> </script>
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more_vert CORE arrow_drop_down COREArticle . 2014License: CC BYFull-Text: https://eprints.gla.ac.uk/99642/2/99642.pdfData sources: COREEnlightenArticle . 2014License: CC BYFull-Text: http://eprints.gla.ac.uk/99642/2/99642.pdfData sources: CORE (RIOXX-UK Aggregator)European Physical Journal C: Particles and FieldsArticle . 2014Data sources: Oxford University Research ArchiveQueen Mary University of London: Queen Mary Research Online (QMRO)Article . 2014Data sources: Bielefeld Academic Search Engine (BASE)All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=2434/242885&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2014Embargo end date: 08 Feb 2019 Belgium, Norway, United Kingdom, Italy, Germany, United Kingdom, Portugal, United Kingdom, France, Brazil, United Kingdom, Germany, United Kingdom, United Kingdom, Australia, United Kingdom, United Kingdom, Brazil, France, United KingdomPublisher:Wiley Publicly fundedFunded by:UKRI | Global modelling of local..., FCT | LA 1, UKRI | RootDetect: Remote Detect... +1 projectsUKRI| Global modelling of local biodiversity responses to human impacts ,FCT| LA 1 ,UKRI| RootDetect: Remote Detection and Precision Management of Root Health ,UKRI| Doctoral Training GrantLionel Hernández; Jodi L. Sedlock; Matthew J. Struebig; Vânia Proença; Eike Lena Neuschulz; Åke Berg; Martin Jung; Carolina L. Morales; Biagio D'Aniello; Kristoffer Hylander; Tom M. Fayle; Tom M. Fayle; Tom M. Fayle; Masahiro Ishitani; Carolina A. Robles; Vassiliki Kati; Virginia Aguilar-Barquero; Pedro Beja; Norbertas Noreika; Alexis Cerezo; Juan Paritsis; Szabolcs Sáfián; Nina Farwig; Steven J. Presley; Jörg Brunet; Oliver Schweiger; Thibault Lachat; T. Keith Philips; Igor Lysenko; Nick A. Littlewood; Stephen J. Rossiter; William Oduro; Kiril Vassilev; Michelle L K Harrison; Robert M. Ewers; Loreta Rosselli; Ulrika Samnegård; Felix Herzog; Alvin J. Helden; James I. Watling; Niall O'Dea; Olivia Norfolk; Víctor H. Luja; Carlos A. Peres; Eliana Martínez; Michael R. Willig; Jimmy Cabra-García; Douglas Sheil; Douglas Sheil; J. Leighton Reid; Tim Diekötter; Tim Diekötter; Nicolás Pelegrin; Antonio Felicioli; Lauchlan H. Fraser; Hollie Booth; Hollie Booth; Gilbert B. Adum; Grzegorz Mikusiński; Victoria Lantschner; Paola J. Isaacs-Cubides; Nor Rasidah Hashim; Annika M. Felton; Lawrence N. Hudson; Tibor Magura; Susan G. Letcher; Akihiro Nakamura; Anelena L Carvalho; Birgit Jauker; Béla Tóthmérész; Neil Aldrin D. Mallari; Neil Aldrin D. Mallari; Marco Silva Gottschalk; Eleanor M. Slade; Andrey S. Zaitsev; Shoji Naoe; Carsten F. Dormann; Mats Jonsell; Diego Higuera-Diaz; Lars Edenius; Péter Batáry; Violette Le Féon; Ben Darvill; Alain Dejean; Alain Dejean; Erin M. Bayne; Carlos H. Vergara; Luz Piedad Romero-Duque; Mick E. Hanley; Christopher D. Williams; Christian Hébert; Isabel Brito; Rolando Cerda; Yana T. Reis; Gretchen LeBuhn; Erika Buscardo; Erika Buscardo; Bertrand Dumont; James R. Miller; Jenni G. Garden; Lucinda Kirkpatrick; Allan H. Smith-Pardo; Allan H. Smith-Pardo; Dario Furlani; John-André Henden; Jochen H. Bihn; Yik Hei Sung; James Grogan; Manuel Esteban Lucas-Borja; John C. Z. Woinarski; Ádám Kőrösi; Ádám Kőrösi; Kaoru Maeto; Gábor L. Lövei; Stefan Abrahamczyk; Paolo Giordani; Lander Baeten; Morgan Garon; Argyrios Choimes; Argyrios Choimes; Danilo Bandini Ribeiro; Inge Armbrecht; Laurent Rousseau; Theodora Petanidou; Helena Castro; Mary N Muchane; Nicole M. Nöske; Nicholas J. Berry; Fernando A. B. Silva; Guiomar Nates-Parra; Pedro Giovâni da Silva; Muchai Muchane; Hannah J. White; Mats Dynesius; Bruno K. C. Filgueiras; Eric Katovai; Jörg U. Ganzhorn; Mounir Louhaichi; Christof Schüepp; Jort Verhulst; Stuart Connop; Matthieu Chauvat; Vena Kapoor; Katja Poveda; Marcelo A. Aizen; Eva Knop; Jörn P. W. Scharlemann; Jörn P. W. Scharlemann; Caragh G. Threlfall; Aaron D. Gove; Aaron D. Gove; Jonathan P. Sadler; Job Aben; Daniel F. R. Cleary; Erika Marin-Spiotta; Caleb Ofori-Boateng; Caleb Ofori-Boateng; Victoria Kemp; Dario A Navarrete Gutierrez; Francis Q. Brearley; Yanping Wang; David L P Correia; Jean-Philippe Légaré; Marino Quaranta; Gentile Francesco Ficetola; Adam J. Vanbergen; Zoltán Elek; Sydney A. Cameron; Jane C. Stout; Chris O. Oke; Ben Collen; Jorge Ari Noriega; Jörg Römbke; Ramón A. Sosa; Simon G. Dures; Simon G. Dures; Alejandro A. Castro-Luna; Joseph E. Hawes; Joseph E. Hawes; Adriana De Palma; Adriana De Palma; Steven J. Fonte; Hans Verboven; Marc Ancrenaz; Andy Purvis; Andy Purvis; Helen Phillips; Helen Phillips; Barbara A. Richardson; Daisuke Fukuda; Carlos A. López-Quintero; Yuan Pan; Badrul Azhar; Katrin Böhning-Gaese; Alejandro Parra-H; Alejandro Parra-H; Ben Phalan; Rebecca A. Senior; Navjot S. Sodhi; Jos Barlow;doi: 10.17863/cam.36177
pmc: PMC4278822
Biodiversity continues to decline in the face of increasing anthropogenic pressures such as habitat destruction, exploitation, pollution and introduction of alien species. Existing global databases of species' threat status or population time series are dominated by charismatic species. The collation of datasets with broad taxonomic and biogeographic extents, and that support computation of a range of biodiversity indicators, is necessary to enable better understanding of historical declines and to project - and avert - future declines. We describe and assess a new database of more than 1.6 million samples from 78 countries representing over 28,000 species, collated from existing spatial comparisons of local-scale biodiversity exposed to different intensities and types of anthropogenic pressures, from terrestrial sites around the world. The database contains measurements taken in 208 (of 814) ecoregions, 13 (of 14) biomes, 25 (of 35) biodiversity hotspots and 16 (of 17) megadiverse countries. The database contains more than 1% of the total number of all species described, and more than 1% of the described species within many taxonomic groups - including flowering plants, gymnosperms, birds, mammals, reptiles, amphibians, beetles, lepidopterans and hymenopterans. The dataset, which is still being added to, is therefore already considerably larger and more representative than those used by previous quantitative models of biodiversity trends and responses. The database is being assembled as part of the PREDICTS project (Projecting Responses of Ecological Diversity In Changing Terrestrial Systems - http://www.predicts.org.uk). We make site-level summary data available alongside this article. The full database will be publicly available in 2015.
CORE arrow_drop_down Repositório do INPAArticle . 2014License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)James Cook University, Australia: ResearchOnline@JCUArticle . 2014Full-Text: http://dx.doi.org/10.1002/ece3.1303Data sources: Bielefeld Academic Search Engine (BASE)Imperial College London: SpiralArticle . 2015License: CC BYFull-Text: http://hdl.handle.net/10044/1/23623Data sources: Bielefeld Academic Search Engine (BASE)Queen Mary University of London: Queen Mary Research Online (QMRO)Article . 2017License: CC BYData sources: Bielefeld Academic Search Engine (BASE)CGIAR CGSpace (Consultative Group on International Agricultural Research)Article . 2015License: CC BYFull-Text: https://hdl.handle.net/10568/68192Data sources: Bielefeld Academic Search Engine (BASE)The University of Melbourne: Digital RepositoryArticle . 2014License: CC BYFull-Text: http://hdl.handle.net/11343/263351Data sources: Bielefeld Academic Search Engine (BASE)Publikationenserver der Georg-August-Universität GöttingenArticle . 2014 . Peer-reviewedLicense: CC BYRepositório Institucional da Universidade de AveiroArticle . 2014Data sources: Repositório Institucional da Universidade de AveiroHochschulschriftenserver - Universität Frankfurt am MainArticle . 2017Data sources: Hochschulschriftenserver - Universität Frankfurt am MainMunin - Open Research ArchiveArticle . 2014 . Peer-reviewedData sources: Munin - Open Research ArchiveQueen's University Belfast Research PortalArticle . 2014Data sources: Bielefeld Academic Search Engine (BASE)Publication Server of Goethe University Frankfurt am MainArticle . 2017License: CC BYData sources: Bielefeld Academic Search Engine (BASE)University of East Anglia: UEA Digital RepositoryArticle . 2014Data sources: Bielefeld Academic Search Engine (BASE)All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.17863/cam.36177&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 155 citations 155 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!
visibility 87visibility views 87 download downloads 186 Powered bymore_vert CORE arrow_drop_down Repositório do INPAArticle . 2014License: CC BY NC NDData sources: Bielefeld Academic Search Engine (BASE)James Cook University, Australia: ResearchOnline@JCUArticle . 2014Full-Text: http://dx.doi.org/10.1002/ece3.1303Data sources: Bielefeld Academic Search Engine (BASE)Imperial College London: SpiralArticle . 2015License: CC BYFull-Text: http://hdl.handle.net/10044/1/23623Data sources: Bielefeld Academic Search Engine (BASE)Queen Mary University of London: Queen Mary Research Online (QMRO)Article . 2017License: CC BYData sources: Bielefeld Academic Search Engine (BASE)CGIAR CGSpace (Consultative Group on International Agricultural Research)Article . 2015License: CC BYFull-Text: https://hdl.handle.net/10568/68192Data sources: Bielefeld Academic Search Engine (BASE)The University of Melbourne: Digital RepositoryArticle . 2014License: CC BYFull-Text: http://hdl.handle.net/11343/263351Data sources: Bielefeld Academic Search Engine (BASE)Publikationenserver der Georg-August-Universität GöttingenArticle . 2014 . Peer-reviewedLicense: CC BYRepositório Institucional da Universidade de AveiroArticle . 2014Data sources: Repositório Institucional da Universidade de AveiroHochschulschriftenserver - Universität Frankfurt am MainArticle . 2017Data sources: Hochschulschriftenserver - Universität Frankfurt am MainMunin - Open Research ArchiveArticle . 2014 . Peer-reviewedData sources: Munin - Open Research ArchiveQueen's University Belfast Research PortalArticle . 2014Data sources: Bielefeld Academic Search Engine (BASE)Publication Server of Goethe University Frankfurt am MainArticle . 2017License: CC BYData sources: Bielefeld Academic Search Engine (BASE)University of East Anglia: UEA Digital RepositoryArticle . 2014Data sources: Bielefeld Academic Search Engine (BASE)All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.17863/cam.36177&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Journal 2002 ItalyPublisher:Kluwer Academic, Boston , Paesi Bassi Neil L. Rose; Roland Psenner; Andrea Lami; Anna Agusti-Panareda; Peter G. Appleby; Øyvind A. Schnell; Richard Tessadri; Roy Thompson; Karin A. Koinig; Karin A. Koinig; Christian Kamenik; Roland Schmidt; Miroslava Prazakova;Changes in microfossils (diatoms, chrysophytes, chironomids and cladocera remains), geochemistry and deposition of atmospheric pollutants have been investigated in the sediment records of the alpine lake Gossenkollesee ( Tyrol, Austria) spanning the last two centuries. The sediment records were compared with seasonal and annual air temperature trends calculated for the elevation (2417 m a. s. l.) and the geographical position (47degrees13'46"N, 11degrees00'51"E) of the lake, and with precipitation records available since 1866 from Innsbruck. Temperature trends followed a 20 30 year oscillation between cold and warm periods. Regarding long-term changes, temperature trends showed a U-shaped trend between 1780 and 1950, followed by a steep increase since 1975.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Other literature type 2023Publisher:OpenAlex Lewis G. Halsey; Vincent Careau; Philip N. Ainslie; Heliodoro Alemán-Mateo; Lene Frost Andersen; Liam Anderson; Lenore Arab; Issad Baddou; Linda G. Bandini; Kweku Bedu-Addo; Ellen E. Blaak; Stéphane Blanc; A. Bonomi; Carlijn V. C. Bouten; Pascal Bovet; Søren Brage; Maciej S. Buchowski; Nancy F. Butte; Stefan Gerardus Camps; Regina C. Casper; Graeme L. Close; Lisa H. Colbert; Jamie A. Cooper; Richard Cooper; Prasangi Dabare; Sai Krupa Das; Peter S. W. Davies; Sanjoy Deb; Christine Delisle Nyström; William H. Dietz; Lara R. Dugas; Simon Eaton; Ulf Ekelund; Asmaa El Hamdouchi; Sonja Entringer; Terrence Forrester; Barry W. Fudge; Melanie B. Gillingham; Annelies H. C. Goris; Michael Gurven; Hinke Haisma; Catherine Hambly; Daniel Hoffman; Marije B. Hoos; Sumei Hu; Noorjehan Joonas; Annemiek Joosen; Peter T. Katzmarzyk; Kitty P. Kempen; Misaka Kimura; William E. Kraus; Wantanee Kriengsinyos; Rebecca Kuriyan; Robert F. Kushner; Estelle V. Lambert; Pulani Lanerolle; Christel Larsson; Nader Lessan; Marie Löf; Corby K. Martin; Eric Matsiko; G.A.L. Meijer; James C. Morehen; James P. Morton; Aviva Must; Marian L. Neuhouser; Theresa A. Nicklas; Robert Ojiambo; Kirsi H. Pietiläinen; Yannis Pitsiladis; Jacob Plange‐Rhule; Guy Plasqui; Ross L. Prentice; Roberto Rabinovich; Susan B. Racette; David A Raichen; Éric Ravussin; Leanne M. Redman; John J. Reilly; Rebecca M. Reynolds; Susan B. Roberts; Dulani Samaranayake; Luís B. Sardinha; Albertine J. Schuit; Analiza M. Silva; Srishti Sinha; Anders Sjödin; Eric Stice; Albert J. Stunkard; Samuel S. Urlacher; Mauro E. Valencia; Giulio Valenti; Ludo M. Van Etten; Edgar A. Van Mil; Jeanine A. Verbunt; Jonathan C. K. Wells; George Wilson; Brian M. Wood; Tsukasa Yoshida; Xueying Zhang;Il existe une variation considérablement plus importante des taux métaboliques entre les hommes qu'entre les femmes, en termes de dépense énergétique (EE) basale, d'activité et totale (quotidienne). Une explication possible est que l'EE est associée à des caractéristiques sexuelles masculines (qui sont connues pour varier plus que d'autres traits) telles que la musculature et la capacité athlétique. De tels traits pourraient être prédits pour être les plus importants pendant les périodes de l'adolescence et du début de l'âge adulte, lorsque le comportement sexuel se développe et culmine. Nous avons testé cette hypothèse sur un grand ensemble de données en comparant la quantité de variation masculine et la variation féminine de l'EE totale, de l'EE d'activité et de l'EE basale, à différents stades de la vie, ainsi que plusieurs traits morphologiques : hauteur, masse sans graisse et masse grasse. L'EE totale, et dans une certaine mesure aussi l'activité EE, présentent une variation masculine (GMV) considérablement plus importante chez les jeunes adultes, puis une diminution du degré de GMV chez les individus de plus en plus âgés. On peut soutenir que l'EE basale, ainsi que la morphométrie, ne présentent pas ce motif. Ces résultats suggèrent que les caractéristiques sexuelles masculines uniques peuvent ne pas présenter de pic de GMV chez les jeunes adultes, mais l'activité totale et peut-être aussi l'activité EE, associées à de nombreux traits morphologiques et physiologiques combinés, présentent le GMV le plus en évidence au cours des étapes de la vie reproductive. Existe una variación considerablemente mayor en las tasas metabólicas entre los hombres que entre las mujeres, en términos de gasto energético (EE) basal, de actividad y total (diario). Una posible explicación es que la EE se asocia con características sexuales masculinas (que se sabe que varían más que otros rasgos) como la musculatura y la capacidad atlética. Se podría predecir que tales rasgos son más prominentes durante los períodos de adolescencia y adultez temprana, cuando el comportamiento sexual se desarrolla y alcanza su punto máximo. Probamos esta hipótesis en un gran conjunto de datos comparando la cantidad de variación masculina y la variación femenina en EE total, EE de actividad y EE basal, en diferentes etapas de la vida, junto con varios rasgos morfológicos: altura, masa libre de grasa y masa grasa. La EE total, y hasta cierto punto también la EE de actividad, exhiben una variación masculina (GMV) considerablemente mayor en adultos jóvenes, y luego una disminución en el grado de GMV en individuos progresivamente mayores. Podría decirse que el EE basal, y también la morfometría, no exhiben este patrón. Estos hallazgos sugieren que las características sexuales masculinas individuales pueden no exhibir un GMV máximo en la edad adulta joven, sin embargo, el EE total y quizás también la actividad, asociada con muchos rasgos morfológicos y fisiológicos combinados, exhiben el GMV de manera más prominente durante las etapas de la vida reproductiva. There is considerably greater variation in metabolic rates between men than between women, in terms of basal, activity and total (daily) energy expenditure (EE). One possible explanation is that EE is associated with male sexual characteristics (which are known to vary more than other traits) such as musculature and athletic capacity. Such traits might be predicted to be most prominent during periods of adolescence and young adulthood, when sexual behaviour develops and peaks. We tested this hypothesis on a large dataset by comparing the amount of male variation and female variation in total EE, activity EE and basal EE, at different life stages, along with several morphological traits: height, fat free mass and fat mass. Total EE, and to some degree also activity EE, exhibit considerable greater male variation (GMV) in young adults, and then a decrease in the degree of GMV in progressively older individuals. Arguably, basal EE, and also morphometrics, do not exhibit this pattern. These findings suggest that single male sexual characteristics may not exhibit peak GMV in young adulthood, however total and perhaps also activity EE, associated with many morphological and physiological traits combined, do exhibit GMV most prominently during the reproductive life stages. هناك تباين أكبر بكثير في معدلات التمثيل الغذائي بين الرجال منه بين النساء، من حيث الإنفاق الأساسي والنشاط وإجمالي الطاقة (اليومية). أحد التفسيرات المحتملة هو أن EE يرتبط بالخصائص الجنسية للذكور (والتي من المعروف أنها تختلف أكثر من السمات الأخرى) مثل العضلات والقدرة الرياضية. قد يُتوقع أن تكون هذه السمات أكثر بروزًا خلال فترات المراهقة ومرحلة الشباب، عندما يتطور السلوك الجنسي ويصل إلى ذروته. اختبرنا هذه الفرضية على مجموعة بيانات كبيرة من خلال مقارنة كمية تباين الذكور وتباين الإناث في إجمالي الطاقة الكهربائية والنشاط والطاقة الكهربائية القاعدية، في مراحل الحياة المختلفة، إلى جانب العديد من السمات المورفولوجية: الطول والكتلة الخالية من الدهون وكتلة الدهون. يُظهر إجمالي التقييم البيئي، وإلى حد ما أيضًا نشاط التقييم البيئي، تباينًا أكبر بكثير بين الذكور (GMV) لدى الشباب، ثم انخفاضًا في درجة التقييم الطبي العام لدى الأفراد الأكبر سنًا بشكل تدريجي. يمكن القول إن EE القاعدية، وكذلك القياسات الشكلية، لا تظهر هذا النمط. تشير هذه النتائج إلى أن الخصائص الجنسية للذكور العازبين قد لا تظهر ذروة GMV في مرحلة الشباب، ولكن إجمالي وربما أيضًا النشاط EE، المرتبط بالعديد من السمات المورفولوجية والفسيولوجية مجتمعة، يظهر GMV بشكل بارز خلال مراحل الحياة الإنجابية.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen 0 citations 0 popularity Average influence Average impulse Average Powered by BIP!
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