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of 373
pro vyhledávání: '"E Ambrosi"'
Publikováno v:
BMC Nursing, Vol 21, Iss 1, Pp 1-9 (2022)
Abstract Background During the COVID-19 pandemic, the care of hip fracture patients remains a clinical priority. To date, there is limited empirical knowledge about the impact of pandemic on the care of patients surgically treated for hip fracture, a
Externí odkaz:
https://doaj.org/article/5868ae2b605a4934b3c2866ce4c8532e
Autor:
A Del Casale, S Ferracuti, G D Kotzalidis, C Rapinesi, D Serata, E Ambrosi, A Simonetti, V Savoja, M Pompili, G Angeletti, R Tatarelli, P Girardi
Publikováno v:
South African Journal of Psychiatry, Vol 17, Iss 1 (2011)
The perception of fear and subsequent appropriate behavioral responding are crucial for the adaptation of species to their living environment. Functional neuroimaging studies of the neural basis of fear during the last few decades in humans contribut
Externí odkaz:
https://doaj.org/article/9c1017d407fa4fe3b5754a80f3fed52f
Autor:
P. C. Chang, P. J. Liao, C. H. Wu, Y. C. Chang, D. H. Hou, E. Ambrosi, H. Y. Lee, J. H. Lee, X. Y. Bao Taiwan
Publikováno v:
2023 IEEE International Reliability Physics Symposium (IRPS).
Autor:
A Robba, C Pinto, F Pintore, G Rodriguez, E Ambrosi, F Barra, G Cusumano, A D’Aì, M Del Santo, P Kosec, A Marino, M Middleton, T Roberts, C Salvaggio, R Soria, A Wolter, D Walton
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2022, Vol.515(4), pp.4669-4674 [Peer Reviewed Journal]
Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 10$^{39}$ erg s$^{-1}$. The average number of ULXs per galaxy is still not well constrained, especially given the uncertainty on the fraction of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::963c70cfd2e6882318bd70d00e74b242
http://arxiv.org/abs/2207.09447
http://arxiv.org/abs/2207.09447
Akademický článek
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Autor:
Chiara Salvaggio, A Wolter, F Pintore, C Pinto, E Ambrosi, G L Israel, A Marino, R Salvaterra, L Zampieri, A Belfiore
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 512:1814-1828
Variability is a powerful tool to investigate properties of X-ray binaries (XRB), in particular for Ultraluminous X-ray sources (ULXs) that are mainly detected in the X-ray band. For most ULXs the nature of the accretor is unknown, although a few ULX
Autor:
R Sathyaprakash, T P Roberts, F Grisé, P Kaaret, E Ambrosi, C Done, J C Gladstone, J J E Kajava, R Soria, L Zampieri
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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Monthly Notices of the Royal Astronomical Society, 2022, Vol.511(4), pp.5346-5362 [Peer Reviewed Journal]
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Monthly Notices of the Royal Astronomical Society, 2022, Vol.511(4), pp.5346-5362 [Peer Reviewed Journal]
NGC 1313 X-2 is one of the few known pulsating ultraluminous X-ray sources (PULXs), and so is thought to contain a neutron star that accretes at highly super-Eddington rates. However, the physics of this accretion remains to be determined. Here, we r
Autor:
E. Ambrosi, C. H. Wu, H. Y. Lee, C. F. Hsu, C. M. Lee, S. Vaziri, I. M. Datye, Y. Y. Chen, D. H. Hou, P. C. Chang, D. W. Heh, P. J. Liao, T. Y. Lee, M. F. Chang, H.-S. P. Wong, X. Y. Bao
Publikováno v:
2022 International Electron Devices Meeting (IEDM).
Autor:
Fabio Pintore, M. Del Santo, A. Robba, P. Kosec, E. Ambrosi, Erin Kara, Antonino D'Ai, Dom Walton, Ciro Pinto, A. C. Fabian, G. Rodriguez-Castillo, Matthew J. Middleton, F. Fürst, Timothy P.L. Roberts, Didier Barret, Roberto Soria, W. N. Alston
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 507 (4), pp.5567-5579. ⟨10.1093/mnras/stab2427⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 507 (4), pp.5567-5579. ⟨10.1093/mnras/stab2427⟩
Monthly Notices of the Royal Astronomical Society, 2021, Vol.507(4), pp.5567-5579 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 2021, 507 (4), pp.5567-5579. ⟨10.1093/mnras/stab2427⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 507 (4), pp.5567-5579. ⟨10.1093/mnras/stab2427⟩
Monthly Notices of the Royal Astronomical Society, 2021, Vol.507(4), pp.5567-5579 [Peer Reviewed Journal]
Soft Ultra-Luminous X-ray (ULXs) sources are a subclass of the ULXs that can switch from a supersoft spectral state, where most of the luminosity is emitted below 1 keV, to a soft spectral state with significant emission above 1 keV. In a few systems
Akademický článek
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