Zobrazeno 1 - 10
of 2 387
pro vyhledávání: '"P. d'Orio"'
Autor:
S. Parmigiani, E. Mikulan, S. Russo, S. Sarasso, F.M. Zauli, A. Rubino, A. Cattani, M. Fecchio, D. Giampiccolo, J. Lanzone, P. D'Orio, M. Del Vecchio, P. Avanzini, L. Nobili, I. Sartori, M. Massimini, A. Pigorini
Publikováno v:
Brain Stimulation, Vol 15, Iss 3, Pp 664-675 (2022)
Background: Cortico-cortical evoked potentials (CCEPs) recorded by stereo-electroencephalography (SEEG) are a valuable tool to investigate brain reactivity and effective connectivity. However, invasive recordings are spatially sparse since they depen
Externí odkaz:
https://doaj.org/article/c65af508edf644429cd66c5bf6465c3a
Autor:
Orio, M., Melicherčík, M., Ciroi, S., Canton, V., Aydi, E., Buckley, D. A. H., Dobrotka, A., Luna, G. J. M., Ness, J.
We present X-ray and optical observations of nova V407 Lup (Nova Lup 2016), previously well monitored in outburst, as it returned to quiescent accretion. The X-ray light curve in 2020 February revealed a clear flux modulation with a stable period of
Externí odkaz:
http://arxiv.org/abs/2408.03779
Autor:
Mitrani, Sharon, Behar, Ehud, Drake, Jeremy J., Orio, Marina, Page, Kim, Canton, Valentina, Ness, Jan-Uwe, Sokolovsky, Kirill
The origin of bright X-ray emission lines that appear late in a nova eruption remains largely a puzzle. We present two high-resolution X-ray grating spectra of the classical nova YZ Ret, observed 77 and 115 days post-eruption, using XMM-Newton and Ch
Externí odkaz:
http://arxiv.org/abs/2405.09219
Autor:
S. Russo, A. Pigorini, E. Mikulan, S. Sarasso, A. Rubino, F.M. Zauli, S. Parmigiani, P. d'Orio, A. Cattani, S. Francione, L. Tassi, C.L.A. Bassetti, G. Lo Russo, L. Nobili, I. Sartori, M. Massimini
Publikováno v:
NeuroImage, Vol 234, Iss , Pp 117964- (2021)
Focal cortical lesions are known to result in large-scale functional alterations involving distant areas; however, little is known about the electrophysiological mechanisms underlying these network effects. Here, we addressed this issue by analysing
Externí odkaz:
https://doaj.org/article/27e1b9c185044d3e915cbe25bf302d42
The old nova and intermediate polar (IP) GK Persei underwent one of its recurrent dwarf nova (DN) outbursts in 2018. We proposed monitoring it in UV and X-rays with the Neil Gehrels Swift Observatory, starting less than six days after the eruption, u
Externí odkaz:
http://arxiv.org/abs/2403.05328
Autor:
Bhargava, Yash, Dewangan, Gulab Chand, Anupama, G. C., Kamath, U. S., Sonith, L. S., Singh, Kulinder Pal, Drake, J. J., Beardmore, A., Luna, G. J. M., Orio, M., Page, K. L.
Nova Her 2021 or V1674 Her was one of the fastest novae to be observed so far. We report here the results from our timing and spectral studies of the source observed at multiple epochs with AstroSat. We report the detection of a periodicity in the so
Externí odkaz:
http://arxiv.org/abs/2312.10291
Nova Her 2021 was observed with TESS 12.62 days after its most recent outburst in June 12.537 2021. This cataclysmic variable belongs to the intermediate polar class, with an spin period of $\sim$501 s and orbital period of 0.1529 days. During TESS o
Externí odkaz:
http://arxiv.org/abs/2310.02220
Autor:
Strong, Giles C., Lagrange, Maxime, Orio, Aitor, Bordignon, Anna, Bury, Florian, Dorigo, Tommaso, Giammanco, Andrea, Heikal, Mariam, Kieseler, Jan, Lamparth, Max, del Árbol, Pablo Martínez Ruíz, Nardi, Federico, Vischia, Pietro, Zaraket, Haitham
We describe a software package, TomOpt, developed to optimise the geometrical layout and specifications of detectors designed for tomography by scattering of cosmic-ray muons. The software exploits differentiable programming for the modeling of muon
Externí odkaz:
http://arxiv.org/abs/2309.14027
Autor:
Aydi, E., Chomiuk, L., Strader, J., Sokolovsky, K. V., Williams, R. E., Buckley, D. A. H., Ederoclite, A., Izzo, L., Kyer, R., Linford, J. D., Kniazev, A., Metzger, B. D., Mikolajewska, J., Molaro, P., Mollina, I., Mukai, K., Munari, U., Orio, M., Panurach, T., Shappee, B. J., Shen, K. J., Sokoloski, J. L., Urquhart, R., Walter, F. M.
The optical spectra of novae are characterized by emission lines from the hydrogen Balmer series and either Fe II or He/N, leading to their traditional classification into two spectral classes: "Fe II" and "He/N". For decades, the origins of these sp
Externí odkaz:
http://arxiv.org/abs/2309.07097
Autor:
J. Schusser, H. Orio, M. Ünzelmann, J. Heßdörfer, M. P. T. Masilamani, F. Diekmann, K. Rossnagel, F. Reinert
Publikováno v:
Communications Physics, Vol 7, Iss 1, Pp 1-6 (2024)
Abstract Dichroic techniques are highly relevant in the field of topological materials, layered systems, and spin-polarized electronic states. Dichroism in angle-resolved photoemission is per se a matrix element effect, which depends on the initial a
Externí odkaz:
https://doaj.org/article/26a29a95689d4cf6b39fc5d4f476b871