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Institution

Spanish National Research Council

GovernmentMadrid, Spain
About: Spanish National Research Council is a government organization based out in Madrid, Spain. It is known for research contribution in the topics: Population & Galaxy. The organization has 79563 authors who have published 220470 publications receiving 7698991 citations. The organization is also known as: CSIC & Consejo Superior de Investigaciones Científicas.
Topics: Population, Galaxy, Catalysis, Stars, Star formation


Papers
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Journal ArticleDOI
Stephen J. Smartt1, Ting-Wan Chen2, Anders Jerkstrand2, Michael W. Coughlin3, Erkki Kankare1, Stuart A. Sim1, Morgan Fraser4, Cosimo Inserra5, Kate Maguire1, K. C. Chambers6, M. E. Huber6, Thomas Krühler2, Giorgos Leloudas7, M. R. Magee1, Luke J. Shingles1, K. W. Smith1, David Young1, John L. Tonry6, Rubina Kotak1, Avishay Gal-Yam8, J. D. Lyman9, D. Homan10, C. Agliozzo11, C. Agliozzo12, Joseph P. Anderson13, C. Angus5, Chris Ashall14, Cristina Barbarino15, Franz E. Bauer16, Franz E. Bauer12, Franz E. Bauer17, Marco Berton18, Marco Berton19, M. T. Botticella19, Mattia Bulla15, J. Bulger6, Giacomo Cannizzaro20, Giacomo Cannizzaro21, Zach Cano22, Régis Cartier5, Aleksandar Cikota13, P. Clark1, A. De Cia13, M. Della Valle19, Larry Denneau6, M. Dennefeld23, Luc Dessart24, Georgios Dimitriadis5, Nancy Elias-Rosa, R. E. Firth5, H. Flewelling6, A. Flörs2, A. Franckowiak, C. Frohmaier25, Lluís Galbany26, Santiago González-Gaitán27, Jochen Greiner2, Mariusz Gromadzki28, A. Nicuesa Guelbenzu, Claudia P. Gutiérrez5, A. Hamanowicz28, A. Hamanowicz13, Lorraine Hanlon4, Jussi Harmanen29, Kasper E. Heintz7, Kasper E. Heintz30, A. Heinze6, M.-S. Hernandez31, Simon Hodgkin32, Isobel Hook33, Luca Izzo22, Phil A. James14, Peter G. Jonker21, Peter G. Jonker20, Wolfgang Kerzendorf13, S. Klose, Z. Kostrzewa-Rutkowska21, Z. Kostrzewa-Rutkowska20, Marek Kowalski34, Markus Kromer35, Markus Kromer36, Hanindyo Kuncarayakti29, Andy Lawrence10, T. Lowe6, Eugene A. Magnier6, Ilan Manulis8, Antonio Martin-Carrillo4, Seppo Mattila29, O. McBrien1, André Müller2, Jakob Nordin34, D. O'Neill1, F. Onori20, F. Onori21, J. Palmerio37, Andrea Pastorello19, Ferdinando Patat13, G. Pignata12, G. Pignata11, Ph. Podsiadlowski38, Maria Letizia Pumo39, Maria Letizia Pumo19, S. J. Prentice14, Arne Rau2, A. Razza13, A. Razza24, A. Rest40, A. Rest41, T. M. Reynolds29, Rupak Roy42, Rupak Roy15, Ashley J. Ruiter43, Ashley J. Ruiter44, Krzysztof A. Rybicki28, Lána Salmon4, Patricia Schady2, A. S. B. Schultz6, T. Schweyer2, Ivo R. Seitenzahl44, Ivo R. Seitenzahl43, M. Smith5, Jesper Sollerman15, B. Stalder, Christopher W. Stubbs45, Mark Sullivan5, Helene Szegedi46, Francesco Taddia15, Stefan Taubenberger2, Giacomo Terreran47, Giacomo Terreran19, B. van Soelen46, J. Vos31, Richard J. Wainscoat6, Nicholas A. Walton32, Christopher Waters6, H. Weiland6, Mark Willman6, P. Wiseman2, Darryl Wright48, Łukasz Wyrzykowski28, O. Yaron8 
02 Nov 2017-Nature
TL;DR: Observations and physical modelling of a rapidly fading electromagnetic transient in the galaxy NGC 4993, which is spatially coincident with GW170817, indicate that neutron-star mergers produce gravitational waves and radioactively powered kilonovae, and are a nucleosynthetic source of the r-process elements.
Abstract: Gravitational waves were discovered with the detection of binary black-hole mergers and they should also be detectable from lower-mass neutron-star mergers. These are predicted to eject material rich in heavy radioactive isotopes that can power an electromagnetic signal. This signal is luminous at optical and infrared wavelengths and is called a kilonova. The gravitational-wave source GW170817 arose from a binary neutron-star merger in the nearby Universe with a relatively well confined sky position and distance estimate. Here we report observations and physical modelling of a rapidly fading electromagnetic transient in the galaxy NGC 4993, which is spatially coincident with GW170817 and with a weak, short γ-ray burst. The transient has physical parameters that broadly match the theoretical predictions of blue kilonovae from neutron-star mergers. The emitted electromagnetic radiation can be explained with an ejected mass of 0.04 ± 0.01 solar masses, with an opacity of less than 0.5 square centimetres per gram, at a velocity of 0.2 ± 0.1 times light speed. The power source is constrained to have a power-law slope of -1.2 ± 0.3, consistent with radioactive powering from r-process nuclides. (The r-process is a series of neutron capture reactions that synthesise many of the elements heavier than iron.) We identify line features in the spectra that are consistent with light r-process elements (atomic masses of 90-140). As it fades, the transient rapidly becomes red, and a higher-opacity, lanthanide-rich ejecta component may contribute to the emission. This indicates that neutron-star mergers produce gravitational waves and radioactively powered kilonovae, and are a nucleosynthetic source of the r-process elements.

695 citations

Journal ArticleDOI
TL;DR: Results obtained suggest that in the cellular toxicity of NaCl in pea plants, superoxide- and H 2 O 2 -mediated oxidative damage in chloroplasts may play an important role.

694 citations

Journal ArticleDOI
TL;DR: In this paper, the authors used Monte Carlo and iterative methods considering dipolar and higher-order multipole effects to calculate the hysteresis loops of two-dimensional arrays of magnetic nanowires.
Abstract: Hysteresis loops of two-dimensional arrays of magnetic nanowires have been micromagnetically modelled. The calculations focus on magnetostatic interactions in addition to Zeeman and magnetic anisotropy energy terms. Starting from an ideally ordered hexagonal array, the generation of local disorder is first modelled and subsequently, hysteresis loops are calculated by Monte Carlo and iterative methods considering dipolar and higher-order multipole effects. The main conclusions of the modelling are: (i) distortion of the hexagonal ordering results in an increasing effective field to reach magnetic saturation while roughly maintaining coercivity, and (ii) an increase of the average distributed coercivity of individual nanowires gives rise to enhanced coercivity and anisotropy field. The results of these simulations are analysed in view of experimental loops of arrays of Ni nanowires filling nanoporous alumina membranes with different degrees of 2D-polycrystalline arrangement. After a careful analysis by image processing, it is concluded that fluctuations in the diameter and cross-section of individual nanowires play an important role in a deep correlation between modelled and experimental hysteresis loops.

693 citations

Journal ArticleDOI
15 Nov 2006-Talanta
TL;DR: The developed analytical method was successfully applied to the analysis of pharmaceutical residues in WWTP influents and effluents, as well as in river water, and justifying the selection of internal standard calibration as the most suitable approach for this study.

693 citations

Journal ArticleDOI
17 Apr 2020-Science
TL;DR: How engineering hormone signaling in specific cells and cellular domains can facilitate improved plant responses to drought is discussed and current knowledge and future questions central to the quest to produce high-yield, drought-resistant crops are explored.
Abstract: Drought alone causes more annual loss in crop yield than all pathogens combined. To adapt to moisture gradients in soil, plants alter their physiology, modify root growth and architecture, and close stomata on their aboveground segments. These tissue-specific responses modify the flux of cellular signals, resulting in early flowering or stunted growth and, often, reduced yield. Physiological and molecular analyses of the model plant Arabidopsis thaliana have identified phytohormone signaling as key for regulating the response to drought or water insufficiency. Here we discuss how engineering hormone signaling in specific cells and cellular domains can facilitate improved plant responses to drought. We explore current knowledge and future questions central to the quest to produce high-yield, drought-resistant crops.

693 citations


Authors

Showing all 79686 results

NameH-indexPapersCitations
Guido Kroemer2361404246571
George Efstathiou187637156228
Peidong Yang183562144351
H. S. Chen1792401178529
David R. Williams1782034138789
Andrea Bocci1722402176461
Adrian L. Harris1701084120365
Gang Chen1673372149819
Gregory J. Hannon165421140456
Alvaro Pascual-Leone16596998251
Jorge E. Cortes1632784124154
Dongyuan Zhao160872106451
John B. Goodenough1511064113741
David D'Enterria1501592116210
A. Gomes1501862113951
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20241
202371
2022463
202111,933
202012,584
201911,596