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description Publicationkeyboard_double_arrow_right Review , Article , Other literature type 2021 Netherlands, IrelandPublisher:Elsevier BV Publicly fundedFunded by:EC | STAMPEC| STAMPWouters, B.; Currivan, S.A.; Abdulhussain, N.; Hankemeier, T.; Schoenmakers, P.J.;handle: 1887/3250346
Immobilized-enzyme reactors (IMERs) are flow-through devices containing enzymes that are physically confined or localized with retention of their catalytic activities. IMERs can be used repeatedly and continuously and have been applied for (bio)polymer degradation, proteomics, biomarker discovery, inhibitor screening, and detection. Online integration of IMERs with analytical instrumentation, such as high-performance liquid chromatography (HPLC) systems, reduces the time needed for multi-step workflows, reduces the need for sample handling, and enables automation. However, online integra-tion can also be challenging, as reaching its full potential requires complex instrumental setups and experienced users. This review aims to provide an assessment of recent advances and challenges in online IMER-based (analytical) LC platforms, covering publications from 2014-2021. A critical discussion of challenges often encountered in IMER fabrication, sample preparation, integration into the analytical workflow, long-term usage, and of potential ways to overcome these is provided. Finally, the obstacles preventing the proliferation of IMERs as efficient tools for high-throughput pharmacological, industrial, and biological studies are discussed. (c) 2021 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
NARCIS arrow_drop_down Leiden University Scholarly Publications RepositoryOther literature type . 2021License: CC BYData sources: Leiden University Scholarly Publications Repositoryadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.trac.2021.116419&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 23 citations 23 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert NARCIS arrow_drop_down Leiden University Scholarly Publications RepositoryOther literature type . 2021License: CC BYData sources: Leiden University Scholarly Publications Repositoryadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.trac.2021.116419&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2021 Netherlands, Ireland, LithuaniaPublisher:MDPI AG Publicly fundedAuthors: Büchler, Jan-Philipp; Brüggelambert, Gregor; de Haan-Cao, Haijing Helen; Sherlock, Roger; +1 AuthorsBüchler, Jan-Philipp; Brüggelambert, Gregor; de Haan-Cao, Haijing Helen; Sherlock, Roger; Savanevičienė, Asta;handle: 10419/275231
In the field of management science and business administration, the case method is gaining ground in research and in teaching. Case studies support on the one hand exploratory research and on the other hand problem-based teaching. However, we find that case research and case teaching remain unchained in management study programs and propose to close this gap. We identify an untapped potential of boosting the case method by integrating case-based research and teaching into a discovery and learning journey of applied science. We suggest embedding the “integrated case method” (ICM) in the ecosystem of universities, with the aim of enhancing and intensifying the knowledge transfer between business and the higher educational sector, thereby achieving better learning objectives in higher education. As a result, this approach enables the development of a high level of contextual intelligence and thus helps to avoid the fallacies of teaching based on uniform theoretical content.
NARCIS arrow_drop_down Administrative Sciences; KTUePubl (Repository of Kaunas University of Technology); NARCISOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 2 citations 2 popularity Top 10% influence Top 10% impulse Average Powered by BIP!more_vert NARCIS arrow_drop_down Administrative Sciences; KTUePubl (Repository of Kaunas University of Technology); NARCISOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euResearch data keyboard_double_arrow_right Dataset 2021Embargo end date: 14 Feb 2021Publisher:Mendeley Authors: Peña-Vinces, Jesús;Peña-Vinces, Jesús;Data for: Environmental knowledge, collaborative economy and responsible consumption in the context of second-hand perinatal and infant clothes in Spain
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.17632/m9f43z5h6p&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2021 France, France, France, Finland, United States, France, France, United Kingdom, Italy, Spain, Italy, Netherlands, Italy, Spain, Italy, ItalyPublisher:EDP Sciences Funded by:EC | EWC, UKRI | Exploring the Universe wi...EC| EWC ,UKRI| Exploring the Universe with radio and optical galaxy surveysM. Martinelli; Isaac Tutusaus; M. Archidiacono; Stefano Camera; V. F. Cardone; Sebastien Clesse; S. Casas; Luciano Casarini; David F. Mota; Henk Hoekstra; Carmelita Carbone; S. Ilić; Thomas D. Kitching; Valeria Pettorino; Alkistis Pourtsidou; Z. Sakr; Domenico Sapone; Natalia Auricchio; A. Balestra; A. Boucaud; Enzo Branchini; Massimo Brescia; V. Capobianco; J. Carretero; Marco Castellano; Stefano Cavuoti; Andrea Cimatti; R. Cledassou; G. Congedo; C. J. Conselice; L. Conversi; Leonardo Corcione; Anne Costille; Marian Douspis; F. Dubath; S. Dusini; Giulio Fabbian; Pablo Fosalba; M. Frailis; E. Franceschi; B. Gillis; Carlo Giocoli; F. Grupp; Luigi Guzzo; W. A. Holmes; Felix Hormuth; Knud Jahnke; S. Kermiche; Alina Kiessling; M. Kilbinger; Martin Kunz; Hannu Kurki-Suonio; Sebastiano Ligori; P. B. Lilje; I. Lloro; Elisabetta Maiorano; Ole Marggraf; K. Markovic; Richard Massey; Massimo Meneghetti; G. Meylan; B. Morin; Lauro Moscardini; S. Niemi; C. Padilla; S. Paltani; Fabio Pasian; K. Pedersen; S. Pires; G. Polenta; M. Poncet; L. Popa; F. Raison; Jason Rhodes; Mauro Roncarelli; Emanuel Rossetti; Roberto P. Saglia; Peter Schneider; A. Secroun; S. Serrano; Chiara Sirignano; G. Sirri; Jean-Luc Starck; F. Sureau; Andy Taylor; Ismael Tereno; Rafael Toledo-Moreo; Edwin A. Valentijn; Luca Valenziano; T. Vassallo; Yu Wang; N. Welikala; Andrea Zacchei; Julien Zoubian;Stefano Camera acknowledges support from the Italian Ministry of Education, University and Research (Miur) through Rita Levi Mon-talcini project ‘Prometheus – Probing and Relating Observables with Multiwavelength Experiments To Help Enlightening the Universe’s Structure’, and the ‘Departments of Excellence 2018–2022’ Grant awarded by Miur (L. 232/2016). The work of SC is supported by the Belgian Fund for Research FNRS-F.R.S. I. T. acknowledges support from the Spanish Ministry of Science, Innovation and Universities through grant ESP2017-89838-C3-1-R. I. T. and T. K. acknowledge funding from the H2020 programme of the European Commission through grant 776247. AP is a UK Research and Innovation Future Leaders Fellow, grant MR/S016066/1. The Euclid Consortium acknowledges the European Space Agency and a number of agencies and institutes that have supported the development of Euclid, in particular the Academy of Finland, the Agenzia Spaziale Italiana, the Belgian Science Policy, the Canadian Euclid Consortium, the Centre National d’Etudes Spatiales, the Deutsches Zentrum für Luft-und Raumfahrt, the Danish Space Research Institute, the Fundação para a Ciência e a Tecnolo-gia, the Ministerio de Economia y Competitividad, the National Aeronautics and Space Administration, the Netherlandse Onderzoekschool Voor Astronomie, the Norwegian Space Agency, the Romanian Space Agency, the State Secretariat for Education, Research and Innovation (SERI) at the Swiss Space Office (SSO), and the United Kingdom Space Agency. A complete and detailed list is available on the Euclid web site (http://www.euclid-ec.org). D. F. M. thanks the Research Council of Norway for their support, and the resources provided by UNINETT Sigma2 – the National Infrastructure for High Performance Computing and Data Storage in Norway. M. M. has received the support of a fellowship from “la Caixa” Foundation (ID 100010434), with fellowship code LCF/BQ/PI19/11690015, and the support of the Spanish Agencia Estatal de Investigacion through the grant “IFT Centro de Excelencia Severo Ochoa SEV-2016-0597”. This paper is based upon work from the COST action CA15117 (CANTATA), supported by COST (European Cooperation in Science and Technology). M. A. acknowledges the computing Upcoming surveys will map the growth of large-scale structure with unprecented precision, improving our understanding of the dark sector of the Universe. Unfortunately, much of the cosmological information is encoded on small scales, where the clustering of dark matter and the effects of astrophysical feedback processes are not fully understood. This can bias the estimates of cosmological parameters, which we study here for a joint analysis of mock Euclid cosmic shear and Planck cosmic microwave background data. We use different implementations for the modelling of the signal on small scales and find that they result in significantly different predictions. Moreover, the different non-linear corrections lead to biased parameter estimates, especially when the analysis is extended into the highly non-linear regime, with the Hubble constant, H0, and the clustering amplitude, σ8, affected the most. Improvements in the modelling of non-linear scales will therefore be needed if we are to resolve the current tension with more and better data. For a given prescription for the non-linear power spectrum, using different corrections for baryon physics does not significantly impact the precision of Euclid, but neglecting these correction does lead to large biases in the cosmological parameters. In order to extract precise and unbiased constraints on cosmological parameters from Euclid cosmic shear data, it is therefore essential to improve the accuracy of the recipes that account for non-linear structure formation, as well as the modelling of the impact of astrophysical processes that redistribute the baryons. Martinelli, M., et al. Peer reviewed
Caltech Authors arrow_drop_down Astronomy and Astrophysics; NARCIS; Archivio della ricerca - Università degli studi di Napoli Federico IIOther literature type . Article . 2021 . 2022 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiLeiden University Scholarly Publications RepositoryOther literature type . 2021Data sources: Leiden University Scholarly Publications RepositoryRecolector de Ciencia Abierta, RECOLECTAArticle . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 29 citations 29 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 23visibility views 23 download downloads 35 Powered bymore_vert Caltech Authors arrow_drop_down Astronomy and Astrophysics; NARCIS; Archivio della ricerca - Università degli studi di Napoli Federico IIOther literature type . Article . 2021 . 2022 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiLeiden University Scholarly Publications RepositoryOther literature type . 2021Data sources: Leiden University Scholarly Publications RepositoryRecolector de Ciencia Abierta, RECOLECTAArticle . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2021 Finland, Italy, Italy, United States, Netherlands, Italy, Italy, France, Netherlands, Spain, France, France, France, Netherlands, United Kingdom, Italy, Italy, Denmark, Italy, Switzerland, ItalyPublisher:EDP Sciences Funded by:EC | ClustersXCosmoEC| ClustersXCosmoA. Fumagalli; Alexandro Saro; Stefano Borgani; Tiago Castro; M. Costanzi; Pierluigi Monaco; E. Munari; Emiliano Sefusatti; Adam Amara; Natalia Auricchio; A. Balestra; C. Bodendorf; D. Bonino; Enzo Branchini; Jarle Brinchmann; V. Capobianco; Carmelita Carbone; Marco Castellano; Stefano Cavuoti; Andrea Cimatti; R. Cledassou; Christopher J. Conselice; Leonardo Corcione; Anne Costille; Mark Cropper; H. Degaudenzi; Marian Douspis; F. Dubath; S. Dusini; A. Ealet; Pablo Fosalba; E. Franceschi; P. Franzetti; M. Fumana; B. Garilli; Carlo Giocoli; F. Grupp; Luigi Guzzo; Stein Vidar Hagfors Haugan; Henk Hoekstra; W. A. Holmes; Felix Hormuth; Knud Jahnke; Alina Kiessling; M. Kilbinger; Thomas D. Kitching; M. Kümmel; Martin Kunz; Hannu Kurki-Suonio; René J. Laureijs; P. B. Lilje; I. Lloro; Elisabetta Maiorano; Ole Marggraf; K. Markovic; Richard Massey; Massimo Meneghetti; G. Meylan; Lauro Moscardini; S. M. Niemi; C. Padilla; S. Paltani; Fabio Pasian; K. Pedersen; Valeria Pettorino; Sandrine Pires; M. Poncet; L. Popa; Lucia Pozzetti; F. Raison; Jason Rhodes; Mauro Roncarelli; Emanuel Rossetti; Roberto P. Saglia; Roberto Scaramella; Peter Schneider; A. Secroun; G. Seidel; S. Serrano; Chiara Sirignano; G. Sirri; Andy Taylor; Ismael Tereno; Rafael Toledo-Moreo; Edwin A. Valentijn; Luca Valenziano; Yu Wang; Jochen Weller; G. Zamorani; Julien Zoubian; Massimo Brescia; G. Congedo; L. Conversi; Simona Mei; Michele Moresco; T. Vassallo;SB, AS and AF acknowledge financial support from the ERC-StG ‘ClustersxCosmo’ grant agreement 716762, the PRIN-MIUR 2015W7KAWC grant, the ASI-Euclid contract and the INDARK grant. TC is supported by the INFN INDARK PD51 grant and by the PRIN-MIUR 2015W7KAWC grant. Our analyses have been carried out at: CINECA, with the projects INA17_C5B32 and IsC82_CosmGC; the computing center of INAF-Osservatorio Astronomico di Trieste, under the coordination of the CHIPP project (Bertocco et al. 2019; Taffoni et al. 2020). The Euclid Consortium acknowledges the European Space Agency and a number of agencies and institutes that have supported the development of Euclid, in particular the Academy of Finland, the Agenzia Spaziale Italiana, the Belgian Science Policy, the Canadian Euclid Consortium, the Centre National d’Etudes Spatiales, the Deutsches Zentrum für Luft- und Raumfahrt, the Danish Space Research Institute, the Fundação para a Ciência e a Tecnologia, the Ministerio de Economia y Competitividad, the National Aeronautics and Space Administration, the Netherlandse Onderzoekschool Voor Astronomie, the Norwegian Space Agency, the Romanian Space Agency, the State Secretariat for Education, Research and Innovation (SERI) at the Swiss Space Office (SSO), and the United Kingdom Space Agency. A complete and detailed list is available on the Euclid website (http://www.euclid-ec.org). [Methods] By analysing 1000 Euclid-like light cones, produced with the PINOCCHIO approximate method, we validated the analytical model of Hu & Kravtsov (2003, ApJ, 584, 702) for the covariance matrix, which takes into account both sources of statistical error. Then, we used such a covariance to define the likelihood function that is better equipped to extract cosmological information from cluster number counts at the level of precision that will be reached by the future Euclid photometric catalogs of galaxy clusters. We also studied the impact of the cosmology dependence of the covariance matrix on the parameter constraints. [Results] The analytical covariance matrix reproduces the variance measured from simulations within the 10 percent; such a difference has no sizeable effect on the error of cosmological parameter constraints at this level of statistics. Also, we find that the Gaussian likelihood with full covariance is the only model that provides an unbiased inference of cosmological parameters without underestimating the errors, and that the cosmology-dependence of the covariance must be taken into account. [Aims] We investigate the contribution of shot-noise and sample variance to uncertainties in the cosmological parameter constraints inferred from cluster number counts, in the context of the Euclid survey. Fumagalli, A. et al. Euclid Consortium Peer reviewed
Archivio della ricer... arrow_drop_down Durham Research Online; Astronomy and Astrophysics; Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; NARCISArticle . 2021 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationsHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2021Data sources: OA@INAF - Istituto Nazionale di AstrofisicaAstronomy and AstrophysicsArticle . 2021add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 3 citations 3 popularity Top 10% influence Average impulse Average Powered by BIP!visibility 21visibility views 21 download downloads 22 Powered bymore_vert Archivio della ricer... arrow_drop_down Durham Research Online; Astronomy and Astrophysics; Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; NARCISArticle . 2021 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationsHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2021Data sources: OA@INAF - Istituto Nazionale di AstrofisicaAstronomy and AstrophysicsArticle . 2021add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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description Publicationkeyboard_double_arrow_right Review , Article , Other literature type 2021 Netherlands, IrelandPublisher:Elsevier BV Publicly fundedFunded by:EC | STAMPEC| STAMPWouters, B.; Currivan, S.A.; Abdulhussain, N.; Hankemeier, T.; Schoenmakers, P.J.;handle: 1887/3250346
Immobilized-enzyme reactors (IMERs) are flow-through devices containing enzymes that are physically confined or localized with retention of their catalytic activities. IMERs can be used repeatedly and continuously and have been applied for (bio)polymer degradation, proteomics, biomarker discovery, inhibitor screening, and detection. Online integration of IMERs with analytical instrumentation, such as high-performance liquid chromatography (HPLC) systems, reduces the time needed for multi-step workflows, reduces the need for sample handling, and enables automation. However, online integra-tion can also be challenging, as reaching its full potential requires complex instrumental setups and experienced users. This review aims to provide an assessment of recent advances and challenges in online IMER-based (analytical) LC platforms, covering publications from 2014-2021. A critical discussion of challenges often encountered in IMER fabrication, sample preparation, integration into the analytical workflow, long-term usage, and of potential ways to overcome these is provided. Finally, the obstacles preventing the proliferation of IMERs as efficient tools for high-throughput pharmacological, industrial, and biological studies are discussed. (c) 2021 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
NARCIS arrow_drop_down Leiden University Scholarly Publications RepositoryOther literature type . 2021License: CC BYData sources: Leiden University Scholarly Publications Repositoryadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.trac.2021.116419&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 23 citations 23 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert NARCIS arrow_drop_down Leiden University Scholarly Publications RepositoryOther literature type . 2021License: CC BYData sources: Leiden University Scholarly Publications Repositoryadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.trac.2021.116419&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2021 Netherlands, Ireland, LithuaniaPublisher:MDPI AG Publicly fundedAuthors: Büchler, Jan-Philipp; Brüggelambert, Gregor; de Haan-Cao, Haijing Helen; Sherlock, Roger; +1 AuthorsBüchler, Jan-Philipp; Brüggelambert, Gregor; de Haan-Cao, Haijing Helen; Sherlock, Roger; Savanevičienė, Asta;handle: 10419/275231
In the field of management science and business administration, the case method is gaining ground in research and in teaching. Case studies support on the one hand exploratory research and on the other hand problem-based teaching. However, we find that case research and case teaching remain unchained in management study programs and propose to close this gap. We identify an untapped potential of boosting the case method by integrating case-based research and teaching into a discovery and learning journey of applied science. We suggest embedding the “integrated case method” (ICM) in the ecosystem of universities, with the aim of enhancing and intensifying the knowledge transfer between business and the higher educational sector, thereby achieving better learning objectives in higher education. As a result, this approach enables the development of a high level of contextual intelligence and thus helps to avoid the fallacies of teaching based on uniform theoretical content.
NARCIS arrow_drop_down Administrative Sciences; KTUePubl (Repository of Kaunas University of Technology); NARCISOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 2 citations 2 popularity Top 10% influence Top 10% impulse Average Powered by BIP!more_vert NARCIS arrow_drop_down Administrative Sciences; KTUePubl (Repository of Kaunas University of Technology); NARCISOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euResearch data keyboard_double_arrow_right Dataset 2021Embargo end date: 14 Feb 2021Publisher:Mendeley Authors: Peña-Vinces, Jesús;Peña-Vinces, Jesús;Data for: Environmental knowledge, collaborative economy and responsible consumption in the context of second-hand perinatal and infant clothes in Spain
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu0 citations 0 popularity Average influence Average impulse Average Powered by BIP!more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2021 France, France, France, Finland, United States, France, France, United Kingdom, Italy, Spain, Italy, Netherlands, Italy, Spain, Italy, ItalyPublisher:EDP Sciences Funded by:EC | EWC, UKRI | Exploring the Universe wi...EC| EWC ,UKRI| Exploring the Universe with radio and optical galaxy surveysM. Martinelli; Isaac Tutusaus; M. Archidiacono; Stefano Camera; V. F. Cardone; Sebastien Clesse; S. Casas; Luciano Casarini; David F. Mota; Henk Hoekstra; Carmelita Carbone; S. Ilić; Thomas D. Kitching; Valeria Pettorino; Alkistis Pourtsidou; Z. Sakr; Domenico Sapone; Natalia Auricchio; A. Balestra; A. Boucaud; Enzo Branchini; Massimo Brescia; V. Capobianco; J. Carretero; Marco Castellano; Stefano Cavuoti; Andrea Cimatti; R. Cledassou; G. Congedo; C. J. Conselice; L. Conversi; Leonardo Corcione; Anne Costille; Marian Douspis; F. Dubath; S. Dusini; Giulio Fabbian; Pablo Fosalba; M. Frailis; E. Franceschi; B. Gillis; Carlo Giocoli; F. Grupp; Luigi Guzzo; W. A. Holmes; Felix Hormuth; Knud Jahnke; S. Kermiche; Alina Kiessling; M. Kilbinger; Martin Kunz; Hannu Kurki-Suonio; Sebastiano Ligori; P. B. Lilje; I. Lloro; Elisabetta Maiorano; Ole Marggraf; K. Markovic; Richard Massey; Massimo Meneghetti; G. Meylan; B. Morin; Lauro Moscardini; S. Niemi; C. Padilla; S. Paltani; Fabio Pasian; K. Pedersen; S. Pires; G. Polenta; M. Poncet; L. Popa; F. Raison; Jason Rhodes; Mauro Roncarelli; Emanuel Rossetti; Roberto P. Saglia; Peter Schneider; A. Secroun; S. Serrano; Chiara Sirignano; G. Sirri; Jean-Luc Starck; F. Sureau; Andy Taylor; Ismael Tereno; Rafael Toledo-Moreo; Edwin A. Valentijn; Luca Valenziano; T. Vassallo; Yu Wang; N. Welikala; Andrea Zacchei; Julien Zoubian;Stefano Camera acknowledges support from the Italian Ministry of Education, University and Research (Miur) through Rita Levi Mon-talcini project ‘Prometheus – Probing and Relating Observables with Multiwavelength Experiments To Help Enlightening the Universe’s Structure’, and the ‘Departments of Excellence 2018–2022’ Grant awarded by Miur (L. 232/2016). The work of SC is supported by the Belgian Fund for Research FNRS-F.R.S. I. T. acknowledges support from the Spanish Ministry of Science, Innovation and Universities through grant ESP2017-89838-C3-1-R. I. T. and T. K. acknowledge funding from the H2020 programme of the European Commission through grant 776247. AP is a UK Research and Innovation Future Leaders Fellow, grant MR/S016066/1. The Euclid Consortium acknowledges the European Space Agency and a number of agencies and institutes that have supported the development of Euclid, in particular the Academy of Finland, the Agenzia Spaziale Italiana, the Belgian Science Policy, the Canadian Euclid Consortium, the Centre National d’Etudes Spatiales, the Deutsches Zentrum für Luft-und Raumfahrt, the Danish Space Research Institute, the Fundação para a Ciência e a Tecnolo-gia, the Ministerio de Economia y Competitividad, the National Aeronautics and Space Administration, the Netherlandse Onderzoekschool Voor Astronomie, the Norwegian Space Agency, the Romanian Space Agency, the State Secretariat for Education, Research and Innovation (SERI) at the Swiss Space Office (SSO), and the United Kingdom Space Agency. A complete and detailed list is available on the Euclid web site (http://www.euclid-ec.org). D. F. M. thanks the Research Council of Norway for their support, and the resources provided by UNINETT Sigma2 – the National Infrastructure for High Performance Computing and Data Storage in Norway. M. M. has received the support of a fellowship from “la Caixa” Foundation (ID 100010434), with fellowship code LCF/BQ/PI19/11690015, and the support of the Spanish Agencia Estatal de Investigacion through the grant “IFT Centro de Excelencia Severo Ochoa SEV-2016-0597”. This paper is based upon work from the COST action CA15117 (CANTATA), supported by COST (European Cooperation in Science and Technology). M. A. acknowledges the computing Upcoming surveys will map the growth of large-scale structure with unprecented precision, improving our understanding of the dark sector of the Universe. Unfortunately, much of the cosmological information is encoded on small scales, where the clustering of dark matter and the effects of astrophysical feedback processes are not fully understood. This can bias the estimates of cosmological parameters, which we study here for a joint analysis of mock Euclid cosmic shear and Planck cosmic microwave background data. We use different implementations for the modelling of the signal on small scales and find that they result in significantly different predictions. Moreover, the different non-linear corrections lead to biased parameter estimates, especially when the analysis is extended into the highly non-linear regime, with the Hubble constant, H0, and the clustering amplitude, σ8, affected the most. Improvements in the modelling of non-linear scales will therefore be needed if we are to resolve the current tension with more and better data. For a given prescription for the non-linear power spectrum, using different corrections for baryon physics does not significantly impact the precision of Euclid, but neglecting these correction does lead to large biases in the cosmological parameters. In order to extract precise and unbiased constraints on cosmological parameters from Euclid cosmic shear data, it is therefore essential to improve the accuracy of the recipes that account for non-linear structure formation, as well as the modelling of the impact of astrophysical processes that redistribute the baryons. Martinelli, M., et al. Peer reviewed
Caltech Authors arrow_drop_down Astronomy and Astrophysics; NARCIS; Archivio della ricerca - Università degli studi di Napoli Federico IIOther literature type . Article . 2021 . 2022 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiLeiden University Scholarly Publications RepositoryOther literature type . 2021Data sources: Leiden University Scholarly Publications RepositoryRecolector de Ciencia Abierta, RECOLECTAArticle . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 29 citations 29 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 23visibility views 23 download downloads 35 Powered bymore_vert Caltech Authors arrow_drop_down Astronomy and Astrophysics; NARCIS; Archivio della ricerca - Università degli studi di Napoli Federico IIOther literature type . Article . 2021 . 2022 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiLeiden University Scholarly Publications RepositoryOther literature type . 2021Data sources: Leiden University Scholarly Publications RepositoryRecolector de Ciencia Abierta, RECOLECTAArticle . 2021Data sources: Recolector de Ciencia Abierta, RECOLECTAadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2021 Finland, Italy, Italy, United States, Netherlands, Italy, Italy, France, Netherlands, Spain, France, France, France, Netherlands, United Kingdom, Italy, Italy, Denmark, Italy, Switzerland, ItalyPublisher:EDP Sciences Funded by:EC | ClustersXCosmoEC| ClustersXCosmoA. Fumagalli; Alexandro Saro; Stefano Borgani; Tiago Castro; M. Costanzi; Pierluigi Monaco; E. Munari; Emiliano Sefusatti; Adam Amara; Natalia Auricchio; A. Balestra; C. Bodendorf; D. Bonino; Enzo Branchini; Jarle Brinchmann; V. Capobianco; Carmelita Carbone; Marco Castellano; Stefano Cavuoti; Andrea Cimatti; R. Cledassou; Christopher J. Conselice; Leonardo Corcione; Anne Costille; Mark Cropper; H. Degaudenzi; Marian Douspis; F. Dubath; S. Dusini; A. Ealet; Pablo Fosalba; E. Franceschi; P. Franzetti; M. Fumana; B. Garilli; Carlo Giocoli; F. Grupp; Luigi Guzzo; Stein Vidar Hagfors Haugan; Henk Hoekstra; W. A. Holmes; Felix Hormuth; Knud Jahnke; Alina Kiessling; M. Kilbinger; Thomas D. Kitching; M. Kümmel; Martin Kunz; Hannu Kurki-Suonio; René J. Laureijs; P. B. Lilje; I. Lloro; Elisabetta Maiorano; Ole Marggraf; K. Markovic; Richard Massey; Massimo Meneghetti; G. Meylan; Lauro Moscardini; S. M. Niemi; C. Padilla; S. Paltani; Fabio Pasian; K. Pedersen; Valeria Pettorino; Sandrine Pires; M. Poncet; L. Popa; Lucia Pozzetti; F. Raison; Jason Rhodes; Mauro Roncarelli; Emanuel Rossetti; Roberto P. Saglia; Roberto Scaramella; Peter Schneider; A. Secroun; G. Seidel; S. Serrano; Chiara Sirignano; G. Sirri; Andy Taylor; Ismael Tereno; Rafael Toledo-Moreo; Edwin A. Valentijn; Luca Valenziano; Yu Wang; Jochen Weller; G. Zamorani; Julien Zoubian; Massimo Brescia; G. Congedo; L. Conversi; Simona Mei; Michele Moresco; T. Vassallo;SB, AS and AF acknowledge financial support from the ERC-StG ‘ClustersxCosmo’ grant agreement 716762, the PRIN-MIUR 2015W7KAWC grant, the ASI-Euclid contract and the INDARK grant. TC is supported by the INFN INDARK PD51 grant and by the PRIN-MIUR 2015W7KAWC grant. Our analyses have been carried out at: CINECA, with the projects INA17_C5B32 and IsC82_CosmGC; the computing center of INAF-Osservatorio Astronomico di Trieste, under the coordination of the CHIPP project (Bertocco et al. 2019; Taffoni et al. 2020). The Euclid Consortium acknowledges the European Space Agency and a number of agencies and institutes that have supported the development of Euclid, in particular the Academy of Finland, the Agenzia Spaziale Italiana, the Belgian Science Policy, the Canadian Euclid Consortium, the Centre National d’Etudes Spatiales, the Deutsches Zentrum für Luft- und Raumfahrt, the Danish Space Research Institute, the Fundação para a Ciência e a Tecnologia, the Ministerio de Economia y Competitividad, the National Aeronautics and Space Administration, the Netherlandse Onderzoekschool Voor Astronomie, the Norwegian Space Agency, the Romanian Space Agency, the State Secretariat for Education, Research and Innovation (SERI) at the Swiss Space Office (SSO), and the United Kingdom Space Agency. A complete and detailed list is available on the Euclid website (http://www.euclid-ec.org). [Methods] By analysing 1000 Euclid-like light cones, produced with the PINOCCHIO approximate method, we validated the analytical model of Hu & Kravtsov (2003, ApJ, 584, 702) for the covariance matrix, which takes into account both sources of statistical error. Then, we used such a covariance to define the likelihood function that is better equipped to extract cosmological information from cluster number counts at the level of precision that will be reached by the future Euclid photometric catalogs of galaxy clusters. We also studied the impact of the cosmology dependence of the covariance matrix on the parameter constraints. [Results] The analytical covariance matrix reproduces the variance measured from simulations within the 10 percent; such a difference has no sizeable effect on the error of cosmological parameter constraints at this level of statistics. Also, we find that the Gaussian likelihood with full covariance is the only model that provides an unbiased inference of cosmological parameters without underestimating the errors, and that the cosmology-dependence of the covariance must be taken into account. [Aims] We investigate the contribution of shot-noise and sample variance to uncertainties in the cosmological parameter constraints inferred from cluster number counts, in the context of the Euclid survey. Fumagalli, A. et al. Euclid Consortium Peer reviewed
Archivio della ricer... arrow_drop_down Durham Research Online; Astronomy and Astrophysics; Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; NARCISArticle . 2021 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationsHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2021Data sources: OA@INAF - Istituto Nazionale di AstrofisicaAstronomy and AstrophysicsArticle . 2021add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 3 citations 3 popularity Top 10% influence Average impulse Average Powered by BIP!visibility 21visibility views 21 download downloads 22 Powered bymore_vert Archivio della ricer... arrow_drop_down Durham Research Online; Astronomy and Astrophysics; Archivio Istituzionale della Ricerca dell'Università degli Studi di Milano; NARCISArticle . 2021 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedInfoscience - EPFL scientific publicationsOther literature typeData sources: Infoscience - EPFL scientific publicationsHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2021Data sources: OA@INAF - Istituto Nazionale di AstrofisicaAstronomy and AstrophysicsArticle . 2021add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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