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Institution

International School for Advanced Studies

EducationTrieste, Friuli-Venezia Giulia, Italy
About: International School for Advanced Studies is a education organization based out in Trieste, Friuli-Venezia Giulia, Italy. It is known for research contribution in the topics: Galaxy & Dark matter. The organization has 3751 authors who have published 13433 publications receiving 588454 citations. The organization is also known as: SISSA & Scuola Internazionale Superiore di Studi Avanzati.


Papers
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Journal ArticleDOI
TL;DR: It is demonstrated that the neurodegeneration induced by the expression of anti-NGF antibodies in AD11 mice can be largely reversed by NGF delivery through an olfactory route.
Abstract: Phenotypic knockout of nerve growth factor (NGF) activity in transgenic anti-NGF mice (AD11 mice) results in a progressive neurodegenerative phenotype resembling Alzheimer's disease. In this article, we examine whether and how the progressive neurodegenerative phenotype of AD11 mice could be prevented or ameliorated by pharmacological treatments with NGF or the cholinergic agonist galantamine, at a relatively early phase of Alzheimer's disease-like neurodegeneration. We demonstrate that the neurodegeneration induced by the expression of anti-NGF antibodies in AD11 mice can be largely reversed by NGF delivery through an olfactory route.

209 citations

Journal ArticleDOI
TL;DR: Microglia-derived MVs are identified as a novel mechanism by which microglia participate in AD degeneration, and new therapeutic strategies for the treatment of the disease are suggested.
Abstract: Alzheimer's disease (AD) is characterized by extracellular amyloid-β (Aβ) deposition, which activates microglia, induces neuroinflammation and drives neurodegeneration. Recent evidence indicates that soluble pre-fibrillar Aβ species, rather than insoluble fibrils, are the most toxic forms of Aβ. Preventing soluble Aβ formation represents, therefore, a major goal in AD. We investigated whether microvesicles (MVs) released extracellularly by reactive microglia may contribute to AD degeneration. We found that production of myeloid MVs, likely of microglial origin, is strikingly high in AD patients and in subjects with mild cognitive impairment and that AD MVs are toxic for cultured neurons. The mechanism responsible for MV neurotoxicity was defined in vitro using MVs produced by primary microglia. We demonstrated that neurotoxicity of MVs results from (i) the capability of MV lipids to promote formation of soluble Aβ species from extracellular insoluble aggregates and (ii) from the presence of neurotoxic Aβ forms trafficked to MVs after Aβ internalization into microglia. MV neurotoxicity was neutralized by the Aβ-interacting protein PrP and anti-Aβ antibodies, which prevented binding to neurons of neurotoxic soluble Aβ species. This study identifies microglia-derived MVs as a novel mechanism by which microglia participate in AD degeneration, and suggest new therapeutic strategies for the treatment of the disease.

208 citations

Journal ArticleDOI
TL;DR: In this article, the authors present a counting of microstates of a class of dyonic BPS black holes in AdS4 which precisely reproduces their Bekenstein-Hawking entropy.

208 citations

Journal ArticleDOI
TL;DR: In this paper, the authors demonstrate how this technique might also become useful for the spectroscopy of surfaces, and in particular of surface electronic states, by direct calculation of the tunneling current flowing into, or out of, a graphite surface, as a function of an applied voltage V, illustrating the direct relationship between the current J(V) and the surface electronic structure at energy E-EF=V.
Abstract: Scanning Tunneling Microscopy is now well established as a powerful technique for surface structural studies(1). Our aim is to demonstrate how this technique might also become useful for the spectroscopy of surfaces, and in particular of surface electronic states. We do this by direct calculation of the tunneling current flowing into, or out of, a graphite surface, as a function of an applied voltage V, illustrating the direct relationship between the current J(V) and the surface electronic structure at energy E-EF=V. Graphite has been chosen because it is an important surface, with perfectly known atomic structure, and a simple and well-known electronic structure, where localized σ and π states coexist with fairly delocalized interlayer bulk states(2), and with recently discovered empty surface states(3,4). Most of these interesting features lie several eV away from the Fermi energy. We do not concern ourselves here the the technical difficulties of achieving such a high tunneling voltage on a semimetallic surface. Our calculation, however, shows that the outcome would be very worthwhile, in terms of information on the surface electronic structure.

207 citations

Journal ArticleDOI
Peter A. R. Ade1, Nabila Aghanim2, M. Arnaud3, M. Ashdown4  +255 moreInstitutions (58)
TL;DR: In this paper, the authors constructed spectra for two known AME regions: the Perseus and ρ Ophiuchi molecular clouds using Planck maps and multi-frequency ancillary data.
Abstract: Anomalous microwave emission (AME) has been observed by numerous experiments in the frequency range ~10–60 GHz. Using Planck maps and multi-frequency ancillary data, we have constructed spectra for two known AME regions: the Perseus and ρ Ophiuchi molecular clouds. The spectra are well fitted by a combination of free-free radiation, cosmic microwave background, thermal dust, and electric dipole radiation from small spinning dust grains. The spinning dust spectra are the most precisely measured to date, and show the high frequency side clearly for the first time. The spectra have a peak in the range 20–40 GHz and are detected at high significances of 17.1σ for Perseus and 8.4σ for ρ Ophiuchi. In Perseus, spinning dust in the dense molecular gas can account for most of the AME; the low density atomic gas appears to play a minor role. In ρ Ophiuchi, the ~30 GHz peak is dominated by dense molecular gas, but there is an indication of an extended tail at frequencies 50–100 GHz, which can be accounted for by irradiated low density atomic gas. The dust parameters are consistent with those derived from other measurements. We have also searched the Planck map at 28.5 GHz for candidate AME regions, by subtracting a simple model of the synchrotron, free-free, and thermal dust. We present spectra for two of the candidates; S140 and S235 are bright Hii regions that show evidence for AME, and are well fitted by spinning dust models.

206 citations


Authors

Showing all 3802 results

NameH-indexPapersCitations
Sabino Matarrese155775123278
G. de Zotti154718121249
J. González-Nuevo144500108318
Matt J. Jarvis144106485559
Carlo Baccigalupi137518104722
L. Toffolatti13637695529
Michele Parrinello13363794674
Marzio Nessi129104678641
Luigi Danese12839492073
Lidia Smirnova12794475865
Michele Pinamonti12684669328
David M. Alexander12565260686
Davide Maino12441088117
Dipak Munshi12436584322
Peter Onyisi11469460392
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
202322
202279
2021658
2020714
2019712
2018622