cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
As I have more than 5 files on ESM, so I have uploaded the fiels, titles and captions as a document along with my manuscript files entitled "ESM_fig._tables" from Rainwater-driven microbial fuel cells for power generation In the remote areas
Creators: name: Amen, Mohamed Taha
name: Yasin, Ahmed S.
name: Hegazy, Mohamed I.
name: Jamal, Mohammad Abu Hena Mostafa
name: Hong, Seong-Tshool
name: Barakat, Nasser A. M.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: Environmental Chemistry
subject: 90799 Environmental Engineering not elsewhere classified
subject: FOS: Environmental engineering
subject: 91305 Energy Generation, Conversion and Storage Engineering
subject: FOS: Mechanical engineering

description: The possibility of using rainwater as a sustainable anolyte in an air-cathode microbial fuel cell (MFC) is investigated in this study. The results indicate that the proposed MFC can work within a wide temperature range (from 0 to 30°C), and under aerobic or anaerobic conditions. However, the rainwater season has a distinct impact. Under anaerobic conditions, the summer rainwater achieves a promised open circuit potential (OCP) of 553 ± 2 mV without addition of nutrients at the ambient temperature, while addition of nutrients leads to increase the cell voltage to 763 ± 3 and 588 ± 2 mV at 30°C and ambient temperature, respectively. The maximum OCP for the winter rainwater (492 ± 1.5 mV) is obtained when the reactor is exposed to the air (aerobic conditions) at ambient temperature. Furthermore, the winter rainwater MFC generates a maximum power output of 7 ± 0.1 mWm−2 at a corresponding current density value of 44 ± 0.7 mAm−2 at 30°C. While, at the ambient temperature, the maximum output power is obtained with the summer rainwater (7.2 ± 0.1 mWm−2 at 26 ± 0.5 mAm−2). Moreover, investigation of the bacterial diversity indicates that Lactobacillus spp. is the dominant electroactive genus in the summer rainwater, while in the winter rainwater, Staphylococcus spp. is the main electroactive bacteria. The cyclic voltammetry analysis confirms that the electrons are delivered directly from the bacterial biofilm to the anode surface and without mediators. Overall, the study opens a new avenue for using a novel sustainable type of MFC derived by rainwater.
title: Diagnóstico prenatal de las anomalías torácicas fetales por RM
Creators: name: Recio Rodríguez, Manuel
Publisher: name: Sociedad Española de Radiología Médica
Year: 2014
Subjects: subject: Obstetrics (Pregnancy / birth / postnatal period)
subject: Thorax
subject: Foetal imaging
subject: MR

description: Objetivo docente
Revisión del tema
Conclusiones
Bibliografía
description: Objetivo docente:
Los objetivos docentes de este trabajo son: -Mostrar las diferentes secuencias de RM útiles en el estudio de las anomalías torácicas fetales. -Definir las indicaciones de la RM fetalen el estudio de las diferentes patologías congénitas...
title: ICTUS sí, pero... venoso!!!
Creators: name: Gómez Jiménez, Estibaliz
Publisher: name: Sociedad Española de Radiología Médica
Year: 2014
Subjects: subject: CT
subject: MR
subject: Neuroradiology brain

description: Objetivo docente
Revisión del tema
Conclusiones
Bibliografía
description: Objetivo docente:
Conocer la anatomía del sistema venoso cerebral. Describir las características radiologicas(TC y RM) del infarto venoso...
title: A propósito de la fibrosis estromal focal de mama: nuestra experiencia.
Creators: name: Fernández Cuadriello, Estela
Publisher: name: Sociedad Española de Radiología Médica
Year: 2014
Subjects: subject: Elastography
subject: Ultrasound
subject: Mammography
subject: Breast

description: Objetivo docente
Revisión del tema
Conclusiones
Bibliografía
description: Objetivo docente:
Nuestro objetivo es describir una entidad cada vez más frecuente en nuestro centro y de interés radiológico dada su dificultad diagnóstica dentro de la patología mamaria benigna,
tanto desde el punto de vista mamográfico como ecográfico y su...
Modeling He-rich subdwarfs through the hot-flasher scenario (brief version)
Creators: name: Bertolami, M. M. Miller
name: Althaus, L. G.
name: Unglaub, K.
name: Weiss, A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present 1D numerical simulations aimed at studying the hot-flasher scenario for the formation of He-rich subdwarf stars. Sequences were calculated for a wide range of metallicities and with the He core flash at different points of the post-RGB evolution (i.e. different remnant masses). We followed the complete evolution from the ZAMS, through the hot-flasher event, and to the subdwarf stage for all kinds of hot-flashers. This allows us to present a homogeneous set of abundances for different metallicities and all flavors of hot-flashers. We extend the scope of our work by analyzing the effects in the predicted surface abundances of some standard assumptions in convective mixing and the effects of element diffusion. We find that the hot-flasher scenario is a viable explanation for the formation of He-sdO stars. Our results also show that element diffusion may produce the transformation of (post hot-flasher) He-rich atmospheres into He-deficient ones. If this is so, then the hot-flasher scenario is able to reproduce both the observed properties and distribution of He-sdO stars.
description: Submitted to the "Proceedings of the 16th European White Dwarf Workshop" (to be published JPCS). 4 pages including 1 table and 1 figure. Brief version of the work to be published by A&A (DOI: 10.1051/0004-6361:200810373), but including some complementary information to that work
D5.3 Virtual Computing Laboratories
Creators: name: Kutuzov, Andrey
name: Razick, Sabry
name: Oepen, Stephan
name: Azab, Abdulrahman
Publisher: name: Zenodo
Year: 2021
Subjects: EOSC-Nordic

description: This deliverable presents a method to provide the researchers with a consistent software environment across multiple computing facilities. The consistency is achieved by constructing a set of build scripts that will install the software tools with the same configurations and versions with the same set of dependencies. EasyBuild was selected as the framework to install and configure the software from source code, optimised for the underlying system and expose them as software-modules with uniform naming across systems. This way the researchers can bring their analysis pipelines and run on any of the systems just by loading the same set of modules.
description: This deliverable is approved by the EC on 2nd March 2023. The EOSC-Nordic project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 857652.
Period Change Rates in Large Magellanic Cloud Cepheids Revisited
Creators: name: Rodríguez-Segovia, N.
name: Hajdu, G.
name: Catelan, M.
name: Espinoza-Arancibia, F.
name: Boggiano, G.
name: Cenzano, C.
name: H., E. Garcés
name: Joachimi, K.
name: Muñoz-López, C.
name: Ordenes-Huanca, C.
name: Orquera-Rojas, C.
name: Torres, P.
name: Valenzuela-Navarro, Á.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The period-change rate (PCR) of pulsating variable stars is a useful probe of changes in their interior structure, and thus of their evolutionary stages. So far, the PCRs of Classical Cepheids in the Large Magellanic Cloud (LMC) have been explored in a limited sample of the total population of these variables. Here we use a template-based method to build observed minus computed (O-C) period diagrams, from which we can derive PCRs for these stars by taking advantage of the long time baseline afforded by the Digital Access to a Sky Century @ Harvard (DASCH) light curves, combined with additional data from the Optical Gravitational Lensing Experiment (OGLE), the MAssive Compact Halo Object (MACHO) project, Gaia's Data Release 2, and in some cases the All-Sky Automated Survey (ASAS). From an initial sample of 2315 sources, our method provides an unprecedented sample of 1303 LMC Classical Cepheids with accurate PCRs, the largest for any single galaxy, including the Milky Way. The derived PCRs are largely compatible with theoretically expected values, as computed by our team using the Modules for Experiments in Stellar Astrophysics (MESA) code, as well as with similar previous computations available in the literature. Additionally, five long-period (P>50 d) sources display a cyclic behavior in their O-C diagrams, which is clearly incompatible with evolutionary changes. Finally, on the basis of their large positive PCR values, two first-crossing Cepheid candidates are identified.
description: 11 pages, 6 figures. Accepted by MNRAS
Formation and kinetics of transient metastable states in mixtures under coupled phase ordering and chemical demixing
Creators: name: Soulé, Ezequiel R.
name: Rey, Alejandro D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present theory and simulation of simultaneous chemical demixing and phase ordering in a polymer-liquid crystal mixture in conditions where isotropic- isotropic phase separation is metastable with respect to isotropic-nematic phase transition. It is found that mesophase formation proceeds by a transient metastable phase that surround the ordered phase, and whose lifetime is a function of the ratio of diffusional to orientational mobilities. It is shown that kinetic phase ordering in polymer-mesogen mixtures is analogous to kinetic crystallization in polymer solutions.
description: 17 pages, 5 figures accepted for publication in EPL
Appendexies
Creators: name: Abusaada, Hisham
name: Elshater, Abeer
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 390107
subject: Humanities and social sciences curriculum and pedagogy (excl. economics, business and management)
classificationCode: 461102
subject: Context learning

description: This review introduces the Contextual Critical Historical Inquiry and Analysis (CCHIA) Framework, which integrates context and text to enhance the literature review section in academic urban studies literature.
Deep-Learning Based Linear Precoding for MIMO Channels with Finite-Alphabet Signaling
Creators: name: Girnyk, Maksym A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Information Theory (cs.IT)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: This paper studies the problem of linear precoding for multiple-input multiple-output (MIMO) communication channels employing finite-alphabet signaling. Existing solutions typically suffer from high computational complexity due to costly computations of the constellation-constrained mutual information. In contrast to existing works, this paper takes a different path of tackling the MIMO precoding problem. Namely, a data-driven approach, based on deep learning, is proposed. In the offline training phase, a deep neural network learns the optimal solution on a set of MIMO channel matrices. This allows the reduction of the computational complexity of the precoder optimization in the online inference phase. Numerical results demonstrate the efficiency of the proposed solution vis-à-vis existing precoding algorithms in terms of significantly reduced complexity and close-to-optimal performance.
description: Published in Physical Communication, 4 pages, 1 figure, 1 table
Phenotypic and in silico studies for a series of synthetic thiosemicarbazones as New Delhi metallo-beta-lactamase carbapenemase inhibitors
Creators: name: Moreira, Jonatham Souza
name: Galvão, Danilo Santana
name: Xavier, Carolina Ferreira Cavalcanti
name: Cunha, Silvio
name: da Rocha Pita, Samuel Silva
name: Reis, Joice Neves
name: de Freitas, Humberto Fonseca
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: The past two decades have been marked by a global spread of bacterial resistance to β-lactam drugs and carbapenems derivatives are the ultimate treatment against multidrug-resistant bacteria. β-lactamase expression is related to resistance which demands the development of bacterial resistance blockers. Drug inhibitor combinations of serine-β-lactamase and β-lactam were successful employed in therapy despite their inactivity against New Delhi metallo-beta-lactamase (NDM). Until now, few compounds are active against NDM-producing bacteria and no specific inhibitors are available yet. The rational strategy for NDM inhibitors development starts with in vitro assays aiming to seek compounds that could act synergistically with β-lactam antibiotics. Thus, eight thiosemicarbazone derivatives were synthesized and investigated for their ability to reverse the resistant phenotype in NDM in Enterobacter cloacae. Phenotypic screening indicated that four isatin-beta-thiosemicarbazones showed Fractional Inhibitory Concentration (FIC) ≤ 250 µM in the presence of meropenem (4 µg/mL). The most promising compound (FIC= 31.25 µM) also presented synergistic effect (FICI = 0.34). Docking and molecular dynamics studies on NDM-thiosemicarbazone complex suggested that 2,3-dihydro-1H-indol-2-one subunit interacts with catalytic zinc and interacted through hydrogen bonds with Asp124 acting like a carboxylic acid bioisostere. Additionally, thiosemicarbazone tautomer with oxidized sulfur (thione) seems to act as a spacer rather than zinc chelator, and the aromatic moieties are stabilized by pi–pi and cation–pi interactions with His189 and Lys221 residues. Our results addressed some thiosemicarbazone structural changes to increase its biological activity against NDM and highlight its scaffold as promising alternatives to treat bacterial resistance. Communicated by Ramaswamy H. Sarma
Technology and costs in international competitiveness: from countries and sectors to firms
Creators: name: Dosi, Giovanni
name: Grazzi, Marco
name: Moschella, Daniele
Publisher: name: Alma Mater Studiorum - Università di Bologna
Year: 2014
Subjects: SECS-P/01 Economia politica

description: This paper examines the determinants of international competitiveness at the level of sectors and firms. First, we address the relation between cost-related and technological competition in a sample of fifteen OECD countries. Results suggest that the countries’ sectoral market shares are indeed mainly shaped by technological factors (proxied by investment intensity and patents) while cost advantages/disadvantages do not seem to play any significant role. Next, we attempt to identify the underlying dynamics at the firm level. We do that for a single country, Italy, using a large panel of Italian firms, over nearly two decades. Results show that also at micro level in most sectors investments and patents correlate positively both with the probability of being an exporter and with the capacity to acquire and to increase export market shares. The evidence on costs is more mixed. A simple measure like total labour compensation is positively correlated with the probability of being an exporter, while unit labour costs show a negative correlation only in some manufacturing sectors.
Multi-omics research on common allergens during the ripening of pollen and poplar flocs of Populus deltoides
Creators: name: Guo, Wei
Publisher: name: figshare
Year: 2023
Subjects: Plant biochemistry

description: Raw data about Multi-omics research on common allergens during the ripening of pollen and poplar flocs of Populus deltoides
Produzione e circolazione delle anfore greco italiche in area Adriatica
Creators: name: Esquilini, Elisa <1978>
Publisher: name: Alma Mater Studiorum - Università di Bologna
Year: 2011
Subjects: GEO/09 Georisorse minerarie e applicazioni mineralogico- petrografiche per l'ambiente ed i beni culturali

description: The present study, being part of a wide research program carried by the University of Bologna (Dipartimento di Scienze della Terra e Geo-Ambientali and Dipartimento di Archeologia) together with the Soprintendenze of Emilia-Romagna and Veneto, is aimed at examining the manufacturing and circulation of Greek Italic amphorae in the Adriatic area. This represents an essential step for the historical and archaeological reconstructions and in particular for: 

- the identification of local manufacturing though the archaeometric comparisons between ceramic samples and raw materials 

- the reconstruction of the ancient routes connecting different areas of the Roman world 

The examined archaeologic sites are representative of the main manufacturing areas in the Adriatic region both along the Italian and Albanian coasts: Adria, Cattolica, Rimini, Spina , Suasa and Phoinike. Notably, the Adriatic region not only represents the manufacturing area, but also coincides with the source area where the raw materials were collected. 
Archaeometric analyses of representative samples from the different areas of interests, were performed adapting the analytical tecniques used in mineralogy, petrography and geochemistry, to the study of ancient archaeological finds. These data were combined with the ones obtained from the analysis of clays, aimed at characterizing the nature of the raw materials. 
As a whole, an integration of these data with the available archaeologic observations led to significant advances in the scientific knowledge about of the main types of amphoric manufacturing and distribution in the Adriatic region. 
In particular, a local manufacturing is suggested for all the archaeological finds from Cattolica and for the main part of the archaeological finds from Suasa. Moreover, the occurrence of commercial routes between the sites of Rimini and Suasa and between Adria, Spina and Suasa is evidenced. On the contrary, for the amphorae from Phoinike a provenance from the examined sites is very unlikely.
Erosioni dentali nei bambini affetti da GERD
Creators: name: Caputo, Antonella <1978>
Publisher: name: Alma Mater Studiorum - Università di Bologna
Year: 2011
Subjects: MED/28 Malattie odontostomatologiche

description: L’erosione dentale è definita come una perdita progressiva e irreversibile dei tessuti duri del dente, a causa di un processo chimico che non coinvolge i batteri.
La sua prevalenza è accresciuta negli ultimi anni nella popolazione generale, particolarmente nei bambini e negli adolescenti e rappresenta attualmente un’enorme sfida per la cura della salute orale.
L'eziologia delle erosioni è difficile da diagnosticare perché può essere il risultato di una varietà di fattori e si può manifestare in maniera differente in base alla causa che l’ha determinata. L’eziologia può essere intrinseca, cioè derivante dal contenuto acido dello stomaco associato a disordini alimentari come l’anoressia, la bulimia nervosa, il reflusso gastro-esofageo e il regurgito, o estrinseca, derivante dal contenuto acido proveniente dall’ambiente esterno (cibi dietetici, bevande analcoliche, succhi di frutta, ecc). 
L’erosione è particolarmente frequente nei bambini e poiché i soggetti che presentano erosioni in dentizione decidua hanno un rischio aumentato di manifestare erosioni in dentizione permanente, una diagnosi precoce e una prevenzione attuata in tenera età, aiuterà a prevenire il danno a carico dei denti permanenti. Inoltre se l’erosione dentale non è controllata e stabilizzata, il bambino potrebbe soffrire di severe perdite di superfici dentali, sensibilità dentale, malocclusione, inestetismi o anche ascessi dentali dei denti affetti.
Lo studio caso-controllo è stato condotto dalla Sezione di Odontostomatologia del Dipartimento Testa - Collo, in collaborazione con l’Unità Operativa Complessa di Gastroenterologia Pediatrica dell’Azienda Ospedaliera-Univesitaria di Parma.
Il gruppo di studio comprende 60 pazienti di età compresa tra i 4 e i 13 anni.
Dei 60 bambini arruolati, 30 presentano sintomi e storia clinica di GERD, mentre gli altri 30 sono bambini sani senza alcun sintomo di GERD o di altri disturbi gastrointestinali.
Il gruppo campione A include anche soggetti affetti, oltre che dal reflusso gastro-esofageo, da varie forme di disabilità, in alcune delle quali il GERD sembra essere parte del quadro sindromico.
I risultati ottenuti dallo studio hanno dimostrato una prevalenza maggiore di erosioni dentali nel gruppo di bambini affetti da GERD, rispetto ai bambini sani, in accordo con quanto riportato dalla letteratura.
Snapshot Ptychography on Array cameras
Creators: name: Wang, Chengyu
name: Hu, Minghao
name: Takashima, Yuzuru
name: Schulz, Timothy J.
name: Brady, David J.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Image and Video Processing (eess.IV)
subject: Optics (physics.optics)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Physical sciences

description: We use convolutional neural networks to recover images optically down-sampled by $6.7\times$ using coherent aperture synthesis over a 16 camera array. Where conventional ptychography relies on scanning and oversampling, here we apply decompressive neural estimation to recover full resolution image from a single snapshot, although as shown in simulation multiple snapshots can be used to improve SNR. In place training on experimental measurements eliminates the need to directly calibrate the measurement system. We also present simulations of diverse array camera sampling strategies to explore how snapshot compressive systems might be optimized.
Axisymmetric viscous gravity currents flowing over a porous medium
Creators: name: Spannuth, Melissa J.
name: Neufeld, Jerome A.
name: Wettlaufer, J. S.
name: Worster, M. Grae
Publisher: name: arXiv
Year: 2009
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We study the axisymmetric propagation of a viscous gravity current over a deep porous medium into which it also drains. A model for the propagation and drainage of the current is developed and solved numerically in the case of constant input from a point source. In this case, a steady state is possible in which drainage balances the input, and we present analytical expressions for the resulting steady profile and radial extent. We demonstrate good agreement between our experiments, which use a bed of vertically aligned tubes as the porous medium, and the theoretically predicted evolution and steady state. However, analogous experiments using glass beads as the porous medium exhibit a variety of unexpected behaviours, including overshoot of the steady-state radius and subsequent retreat, thus highlighting the importance of the porous medium geometry and permeability structure in these systems.
description: 11 pages, 6 figures, 1 table
Northwest coast kerfed containers : a formal study
Creators: name: Patterson, Margaret Jean
Publisher: name: University of British Columbia
Year: 2010

description: This study examines a large collection of artifacts, Northwest Coast kerfed containers. A terminology is developed with which to describe the physical traits of these artifacts. These data are analysed using numerical taxonomy, and clustered according to their affinities. The typology thereby produced strongly reflects pre-existing intuitive typologies. As well, the newly discovered ability formally to describe construction traits opens new possibilities for determining the provenance of these containers.
title: CSIC: overview of DIGITALCSIC activities related to EOSC
title: DIGITAL.CSIC and EOSC
titleType: AlternativeTitle
Creators: name: Bernal, Isabel
name: Oficina T??Cnica De DIGITAL.CSIC
name: EOSC-SYNERGY
Publisher: name: CSIC - Unidad de Recursos de Informaci??n Cient??fica para la Investigaci??n (URICI)
Year: 2021
Subjects: Research data management
Gesti??n de datos de investigaci??n
Institutional data repository
Repositorio institucional de datos
DIGITAL.CSIC Policies
Pol??ticas de DIGITAL.CSIC
European Plate Observing System EPOS
EOSC-SYNERGY
IPERION HS
FAIRsFAIR Roadshow - Spain

description: [ES] El 23 de junio FAIRsFAIR en colaboraci??n con la Unidad de Recursos de Informaci??n Cient??fica para la Investigaci??n (URICI) del Consejo Superior de Investigaciones Cient??ficas (CSIC) organizan un evento online abierto a toda la comunidad espa??ola sobre la Nube Europea de Ciencia Abierta (EOSC) y la participaci??n de los repositorios. El evento tiene como t??tulo "Green Data Market for Research & the Role of Repositories" y abordar??, a trav??s de intervenciones de integrantes del proyecto FAIRsFAIR, as?? como de diferentes iniciativas espa??olas y europeas, aspectos relativos a buenas pr??cticas en las pol??ticas y gesti??n de repositorios de datos de investigaci??n para su adhesi??n a los Principios FAIR y su inclusi??n en EOSC. El evento tendr?? un formato bilingue y dar?? una panor??mica de recomendaciones, servicios, recursos y formaci??n para los repositorios de datos a trav??s de experiencias del propio proyecto FAIRsFAIR como del Ministerio de Ciencia e Innovaci??n de Espa??a, Science Europe, EOSC SYNERGY, IBERGRID y el CSIC. [EN] On June 23, FAIRsFAIR in collaboration with the Scientific Information Resources Unit for Research (URICI) of the Higher Council for Scientific Research (CSIC) organizes an online event open to the entire Spanish community on the European Open Science Cloud (EOSC) and the participation of data repositories. The event is entitled "Green Data Market for Research & the Role of Repositories" and will address, through interventions by members of the FAIRsFAIR project, as well as different Spanish and European initiatives, aspects related to good practices in the policies and management of research data repositories for adherence to the FAIR Principles and inclusion in EOSC. The event will have a bilingual format and will provide an overview of recommendations, services, resources and training for data repositories through experiences from the FAIRsFAIR project itself as well as from the Ministry of Science and Innovation of Spain, Science Europe, EOSC SYNERGY, IBERGRID and the CSIC.
Data tables and plots to support the data presented in the main manuscript from Consumer trait responses track change in resource supply along with replicated thermal gradients
Creators: name: Moffett, E. R.
name: Fryxell, D. C.
name: Lee, F.
name: Palkovacs, E. P.
name: Simon, K. S.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: Ecology
subject: FOS: Biological sciences

description: Rising temperatures may alter consumer diets through increased metabolic demand and altered resource availability. However, current theories assessing dietary shifts with warming do not account for a change in resource availability. It is unknown whether consumers will increase consumption rates or consume different resources to meet increased energy requirements and whether the dietary change will lead to associated variation in morphology and nutrient utilization. Here, we used populations of Gambusia affinis across parallel thermal gradients in New Zealand (NZ) and California (CA) to understand the influence of temperature on diets, morphology and stoichiometric phenotypes. Our results show that with increasing temperature in NZ, mosquitofish consumed more plant material, whereas, in CA, mosquitofish shifted towards increased consumption of invertebrate prey. In both regions, populations with plant-based diets had fuller guts, longer relative gut lengths, more superior orientated mouths and reduced body elemental %C and N/P. Together, our results show multiple pathways by which consumers may alter their feeding patterns with rising temperatures, and they suggest that warming-induced changes to resource availability may be the principal determinant of which pathway is taken.
Science Europe DMP rubric- alignment with EC DMPs policy
Creators: name: Borrell-Dami??N, Lidia
Publisher: name: CSIC - Unidad de Recursos de Informaci??n Cient??fica para la Investigaci??n (URICI)
Year: 2021
Subjects: FAIRsFAIR Roadshow - Spain

description: [ES] El 23 de junio FAIRsFAIR en colaboraci??n con la Unidad de Recursos de Informaci??n Cient??fica para la Investigaci??n (URICI) del Consejo Superior de Investigaciones Cient??ficas (CSIC) organizan un evento online abierto a toda la comunidad espa??ola sobre la Nube Europea de Ciencia Abierta (EOSC) y la participaci??n de los repositorios. El evento tiene como t??tulo "Green Data Market for Research & the Role of Repositories" y abordar??, a trav??s de intervenciones de integrantes del proyecto FAIRsFAIR, as?? como de diferentes iniciativas espa??olas y europeas, aspectos relativos a buenas pr??cticas en las pol??ticas y gesti??n de repositorios de datos de investigaci??n para su adhesi??n a los Principios FAIR y su inclusi??n en EOSC. El evento tendr?? un formato bilingue y dar?? una panor??mica de recomendaciones, servicios, recursos y formaci??n para los repositorios de datos a trav??s de experiencias del propio proyecto FAIRsFAIR como del Ministerio de Ciencia e Innovaci??n de Espa??a, Science Europe, EOSC SYNERGY, IBERGRID y el CSIC. [EN] On June 23, FAIRsFAIR in collaboration with the Scientific Information Resources Unit for Research (URICI) of the Higher Council for Scientific Research (CSIC) organizes an online event open to the entire Spanish community on the European Open Science Cloud (EOSC) and the participation of data repositories. The event is entitled "Green Data Market for Research & the Role of Repositories" and will address, through interventions by members of the FAIRsFAIR project, as well as different Spanish and European initiatives, aspects related to good practices in the policies and management of research data repositories for adherence to the FAIR Principles and inclusion in EOSC. The event will have a bilingual format and will provide an overview of recommendations, services, resources and training for data repositories through experiences from the FAIRsFAIR project itself as well as from the Ministry of Science and Innovation of Spain, Science Europe, EOSC SYNERGY, IBERGRID and the CSIC.
Modelling the evolution of planets in disks
Creators: name: Kley, Willy
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: To explain important properties of extrasolar planetary systems (eg. close-in hot Jupiters, resonant planets) an evolutionary scenario which allows for radial migration of planets in disks is required. During their formation protoplanets undergo a phase in which they are embedded in the disk and interact gravitationally with it. This planet-disk interaction results in torques (through gravitational forces) acting on the planet that will change its angular momentum and result in a radial migration of the planet through the disk. To determine the outcome of this very important process for planet formation, dedicated high resolution numerical modeling is required. This contribution focusses on some important aspects of the numerical approach that we found essential for obtaining successful results. We specifically mention the treatment of Coriolis forces, Cartesian grids, and the FARGO method.
description: Talk given at JENAM meeting, Vienna 2008
A Fresh Look at AGB stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial-Final Mass Relation
Creators: name: Marigo, Paola
name: Bossini, Diego
name: Trabucchi, Michele
name: Addari, Francesco
name: Girardi, Léo
name: Cummings, Jeffrey
name: Pastorelli, Giada
name: Tio, Piero Dal
name: Costa, Guglielmo
name: Bressan, Alessandro
Publisher: name: arXiv
Year: 2021
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Benefiting from the GAIA second and early third releases of photometric and astrometric data we examine the population of asymptotic giant branch (AGB) stars that appear in the fields of intermediate-age and young open star clusters. We identify 49 AGB star candidates, brighter than the tip of the red giant branch, with a good-to-high cluster membership probability. Among them we find 19 TP-AGB stars with known spectral type: 4 M stars, 3 MS/S stars and 12 C stars. By combining observations, stellar models, and radiative transfer calculations that include the effect of circumstellar dust, we characterize each star in terms of initial mass, luminosity, mass-loss rate, core mass, period and mode of pulsation. The information collected helps us shed light on the TP-AGB evolution at solar-like metallicity, placing constraints on the third dredge-up process, the initial masses of carbon stars, stellar winds, and the initial-final mass relation (IFMR). In particular, we find that two bright carbon stars, MSB 75 and BM IV 90, members of the clusters NGC 7789 and NGC 2660 (with similar ages of $\simeq 1.2-1.6$ Gyr and initial masses $ 2.1 \ge M_{\rm i}/M_{\odot} \ge 1.9$), have unusually high core masses, $M_{\rm c} \approx 0.67-0.7\,M_{\odot}$. These results support the findings of a recent work (Marigo et al. 2020) that identified a kink in the IFMR, which interrupts its monotonic trend just at the same initial masses. Finally, we investigate two competing scenarios to explain the $M_{\rm c}$ data: the role of stellar winds in single-star evolution, and binary interactions through the blue-straggler channel.
description: Article accepted for publication in ApJS (46 pages, 11 figures, 10 tables)
Self-limited self-assembly of chiral filaments
Creators: name: Yang, Yasheng
name: Meyer, Robert B.
name: Hagan, Michael F.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The assembly of filamentous bundles with controlled diameters is common in biological systems and desirable for the development of nanomaterials. We discuss dynamical simulations and free energy calculations on patchy spheres with chiral pair interactions that spontaneously assemble into filamentous bundles. The chirality frustrates long-range crystal order by introducing twist between interacting subunits. For some ranges of system parameters this constraint leads to bundles with a finite diameter as the equilibrium state, and in other cases frustration is relieved by the formation of defects. While some self-limited structures can be modeled as twisted filaments arranged with local hexagonal symmetry, other structures are surprising in their complexity.
description: 5 pages, 5 figures
High energy factorization in nucleus-nucleus collisions III. Long range rapidity correlations
Creators: name: Gelis, F.
name: Lappi, T.
name: Venugopalan, R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We obtain a novel result in QCD for long range rapidity correlations between gluons produced in the collision of saturated high energy hadrons or nuclei. This result, obtained in a high energy factorization framework, provides strong justification for the Glasma flux tube picture of coherent strong color fields. Our formalism can be applied to "near side ridge" events at RHIC and in future studies of long range rapidity correlations at the LHC.
description: 14 pages, 4 postscript figure, final version to appear in PRD
Chirped Biphotons and Their Compression in Optical Fibres
Creators: name: Chekhova, M. V.
name: Kitaeva, G. Kh.
name: Shumilkina, O. A.
name: Degiovanni, I. P.
name: Genovese, M.
name: Meda, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We show that broadband biphoton wavepackets produced via Spontaneous Parametric Down-Conversion (SPDC) in crystals with linearly aperiodic poling can be easily compressed in time using the effect of group-velocity dispersion in optical fibres. This result could foster important developments in quantum metrology and lithography.
description: 4 pages, 5 figures
title: RM de la articulación temporo-mandibular:Técnica,anatomía y análisis de la disfunción articular.
Creators: name: Montes Pérez, Esther
Publisher: name: Sociedad Española de Radiología Médica
Year: 2014
Subjects: subject: MR
subject: Head and neck

description: Objetivo docente
Revisión del tema
Conclusiones
Bibliografía
description: Objetivo docente:
1.
Exponer las características técnicas y el protocolo de estudio empleado para la valoración de la articulación temporo-mandibular mediante RM. 2.
Repasar la anatomía de la articulación temporo-mandibular mediante imágenes de RM. 3.
Valorar...
title: Lo esencial de la comunicación entre pacientes y radiólogos. Gestión emocional y desafío profesional
Creators: name: Guzmán Revuelta, Jesús
Publisher: name: Sociedad Española de Radiología Médica
Year: 2014
Subjects: subject: Health policy and practice
subject: Ethics
subject: Education
subject: Teleradiology
subject: eHealth
subject: Professional issues

description: Objetivos
Material y método
Resultados
Conclusiones
Bibliografía
description: Objetivos:
Revisar la evolución comunicacional con nuestros pacientes y sus expectativas. Concienciar sobre los beneficios de un trato directo (Radiología centrada en el paciente). Ofrecer pautas-guías de aprendizaje comunicacional y gestión emocional....
D2.7: Open Science in the Nordics: Recommendations on Legal Issues
Creators: name: Fisher, Lars
name: Hammargren, Per-Olov
name: Iozzi, Maria Fancesca
name: Kontkanen, Pirjo
name: Sarti, Jarmo
name: Gunnarsdóttir, Birna
Publisher: name: Zenodo
Year: 2021
Subjects: EOSC-Nordic
Open Science policy

description: The success of EOSC largely depends on its capability to enable cross-border research.
 Cross-border research poses challenges not only regarding the technical solutions but also regarding the legal frameworks under which cross-border research sharing is to happen. This deliverable is a follow-up to the deliverable 2.3 Open Science in the Nordics: Legal Insights. In deliverable 2.3, use cases were selected and used to study the types of legal issues hindering cross-border research collaboration, in particular cross-border data sharing. In this deliverable, the legal constraints, as found in deliverable 2.3, have been further studied. In particular, the legal issues reported by researchers in D2.3 have been investigated from the research institution's perspective, supporting research collaborations. Based on the findings in deliverable 2.3 further interviews have been conducted with institution legal experts and other administrative personnel.
description: This deliverable is approved by the EC on 2nd March 2023. The EOSC-Nordic project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 857652.
Second-generation dust in planetary systems: The case of HD 163296
Creators: name: D'Angelo, Gennaro
name: Marzari, Francesco
Publisher: name: arXiv
Year: 2021
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Observations indicate that large, dust-laden protoplanetary discs are common. Some features, like gaps, rings and spirals, suggest they may host young planets, which can excite the orbits of nearby leftover planetesimals. Energetic collisions among these bodies can lead to the production of second-generation dust. Grains produced by collisions may have a dynamical behaviour different from that of first-generation, primordial dust out of which planetesimals and planets formed. We aim to study these differences for the HD 163296 system and determine whether dynamical signatures in the mixture of the two dust populations can help separate their contributions. We use three-dimensional (3-D) hydrodynamic models to describe the gaseous disc with three, Saturn- to Jupiter-mass, embedded planets. Dust grains, of sizes 1um-1mm, are treated as Lagrangean particles with resolved thermodynamics and mass loss. Initial disc and planet configurations are derived from observation-based work, which indicates low gas viscosity. The 3-D approach also allows us to detect the formation of vortices induced by Rossby waves, where dust becomes concentrated and may contribute to planetesimal formation. We find that the main differences in the dynamical behaviour of first- and second-generation dust occur in the vertical distribution. The two populations have similar distributions around the disc mid-plane, although second-generation dust shows longer residence times close to the radial locations of the planets' gas gaps. Sedimentation rates of um-size grains are comparable to or lower than the production rates by planetesimals' collisions, making this population potentially observable. These outcomes can be extended to similar systems harbouring giant planets.
description: 13 pages, 1 table, 13 figures. Accepted for publication in Monthly Notices of the Royal Astronomical Society Main Journal
The effect of network topology on the stability of discrete state models of genetic control
Creators: name: Pomerance, Andrew
name: Ott, Edward
name: Girvan, Michelle
name: Losert, Wolfgang
Publisher: name: arXiv
Year: 2009
Subjects: subject: Molecular Networks (q-bio.MN)
subject: FOS: Biological sciences

description: Boolean networks have been proposed as potentially useful models for genetic control. An important aspect of these networks is the stability of their dynamics in response to small perturbations. Previous approaches to stability have assumed uncorrelated random network structure. Real gene networks typically have nontrivial topology significantly different from the random network paradigm. In order to address such situations, we present a general method for determining the stability of large Boolean networks of any specified network topology and predicting their steady-state behavior in response to small perturbations. Additionally, we generalize to the case where individual genes have a distribution of `expression biases,' and we consider non-synchronous update, as well as extension of our method to non-Boolean models in which there are more than two possible gene states. We find that stability is governed by the maximum eigenvalue of a modified adjacency matrix, and we test this result by comparison with numerical simulations. We also discuss the possible application of our work to experimentally inferred gene networks.
description: 25 pages, 4 figures; added supplementary information, fixed typos and figure, reformatted
title: Validez diagnóstica del índice de resistencia en pacientes trasplantados renales con disfunción del injerto.
Creators: name: Garcia Barquin, Paula
Publisher: name: Sociedad Española de Radiología Médica
Year: 2014
Subjects: subject: Transplantation
subject: Pathology
subject: Biopsy
subject: Ultrasound-Spectral Doppler
subject: Ultrasound-Colour Doppler
subject: Ultrasound
subject: Kidney
subject: Abdomen

description: Objetivos
Material y método
Resultados
Conclusiones
Bibliografía
description: Objetivos:
El objetivo de nuestro estudio fue estimar la validez diagnóstica del índice de resistencia (IR) en pacientes trasplantados renales con disfunción del injerto,
empleando como gold estándar los hallazgos histopatológicos de las biopsias renales....
title: TEP y Embarazo: un diagnóstico complicado.
Creators: name: Caldera de Canepari, Adriana Carolina
Publisher: name: Sociedad Española de Radiología Médica
Year: 2014
Subjects: subject: Drugs / Reactions
subject: Acute
subject: Contrast agent-intravenous
subject: Ultrasound-Colour Doppler
subject: CT-Angiography
subject: MR
subject: Vascular
subject: Thorax

description: Objetivo docente
Revisión del tema
Conclusiones
Bibliografía
description: Objetivo docente:
Describir las técnicas de imagen actualmente disponibles para el diagnóstico de TEP en el embarazo,
con sus ventajas,
desventajas e implicaciones clínicas. Describir las estimaciones aceptadas de dosis de radiación en la madre y el feto,
las...
The ACS LCID Project. I. Short-Period Variables in the Isolated Dwarf Spheroidal Galaxies Cetus & Tucana
Creators: name: Bernard, Edouard J.
name: Monelli, Matteo
name: Gallart, Carme
name: Drozdovsky, Igor
name: Stetson, Peter B.
name: Aparicio, Antonio
name: Cassisi, Santi
name: Mayer, Lucio
name: Cole, Andrew A.
name: Hidalgo, Sebastian L.
name: Skillman, Evan D.
name: Tolstoy, Eline
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: (abridged) We present the first study of the variable star populations in the isolated dwarf spheroidal galaxies (dSph) Cetus and Tucana. Based on Hubble Space Telescope images obtained with the Advanced Camera for Surveys in the F475W and F814W bands, we identified 180 and 371 variables in Cetus and Tucana, respectively. The vast majority are RR Lyrae stars. In Cetus we also found three anomalous Cepheids, four candidate binaries and one candidate long-period variable (LPV), while six anomalous Cepheids and seven LPV candidates were found in Tucana. Of the RR Lyrae stars, 147 were identified as fundamental mode (RRab) and only eight as first-overtone mode (RRc) in Cetus, with mean periods of 0.614 and 0.363 day, respectively. In Tucana we found 216 RRab and 82 RRc giving mean periods of 0.604 and 0.353 day. These values place both galaxies in the so-called Oosterhoff Gap, as is generally the case for dSph. We calculated the distance modulus to both galaxies using different approaches based on the properties of RRab and RRc, namely the luminosity-metallicity and period-luminosity-metallicity relations, and found values in excellent agreement with previous estimates using independent methods: (m-M)_{0,Cet}=24.46+-0.12 and (m-M)_{0,Tuc}=24.74+-0.12, corresponding to 780+-40 kpc and 890+-50 kpc. We also found numerous RR Lyrae variables pulsating in both modes simultaneously (RRd): 17 in Cetus and 60 in Tucana. Tucana is, after Fornax, the second dSph in which such a large fraction of RRd (~17%) has been observed. We provide the photometry and pulsation parameters for all the variables, and compare the latter with values from the literature for well-studied dSph of the Local Group and Galactic globular clusters.
description: 26 pages, 24 figures, in emulateapj format. To be published in ApJ. Some figures heavily degraded; See http://www.iac.es/project/LCID/?p=publications for a version with full resolution figures
The supernova rate: a critical ingredient and an important tool
Creators: name: Mannucci, F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In this review I summarize the role of supernova rate as a critical ingredient of modern astrophysics, and as an important tool to understand SN explosions. Many years of active observations and theoretical modeling have produced several important results. In particular, linking SN rates with parent stellar populations has proved to be an important strategy. Despite these advances, the situation is far from clear, in particular for the SNe Ia.
description: 9 pages; "Probing Stellar Populations out to the Distant Universe", Cefalu' (Italy), September 2008, AIP Conf. Proc. Series; Invited review