Zobrazeno 1 - 10
of 15 443
pro vyhledávání: '"A. Parmentier"'
Autor:
D. Recchiuti, G. D’Angelo, E. Papini, P. Diego, A. Cicone, A. Parmentier, P. Ubertini, R. Battiston, M. Piersanti
Publikováno v:
Frontiers in Earth Science, Vol 11 (2023)
Ionospheric disturbances (such as electromagnetic emissions) in connection to strong earthquakes have been reported in literature for over two decades. In order to be reliable, the identification of such disturbances requires a preliminary robust def
Externí odkaz:
https://doaj.org/article/0505dcffeac241dca3f75b0c5b854865
Autor:
M. Martucci, R. Ammendola, D. Badoni, S. Bartocci, R. Battiston, S. Beolè, W. J. Burger, D. Campana, G. Castellini, P. Cipollone, S. Coli, L. Conti, A. Contin, M. Cristoforetti, G. D’Angelo, C. De Donato, C. De Santis, A. Di Luca, F. M. Follega, G. Gebbia, R. Iuppa, A. Lega, M. Lolli, N. Marcelli, G. Masciantonio, M. Mergè, M. Mese, C. Neubüser, F. Nozzoli, A. Oliva, G. Osteria, L. Pacini, F. Palma, F. Palmonari, B. Panico, A. Parmentier, S. Perciballi, F. Perfetto, P. Picozza, M. Pozzato, G. M. Rebustini, E. Ricci, M. Ricci, S. B. Ricciarini, U. Savino, Z. Sahnoun, V. Scotti, A. Sotgiu, R. Sparvoli, P. Ubertini, V. Vilona, V. Vitale, S. Zoffoli, P. Zuccon, O. P. M. Aslam, M. D. Ngobeni, M. S. Potgieter
Publikováno v:
The Astrophysical Journal Letters, Vol 945, Iss 2, p L39 (2023)
Time-dependent energy spectra of galactic cosmic rays (GCRs) carry crucial information regarding their origin and propagation throughout the interstellar environment. When observed at the Earth, after traversing the interplanetary medium, such spectr
Externí odkaz:
https://doaj.org/article/b8ea916360bd4c22af329ed2f2b52bff
Autor:
R. Battiston, C. Neubüser, F. M. Follega, R. Iuppa, V. Vitale, R. Ammendola, D. Badoni, S. Bartocci, A. Bazzano, S. Beolè, I. Bertello, W. J. Burger, D. Campana, A. Cicone, P. Cipollone, S. Coli, L. Conti, A. Contin, M. Cristoforetti, G. D’Angelo, F. De Angelis, C. De Donato, C. De Santis, P. Diego, A. Di Luca, E. Fiorenza, G. Gebbia, A. Lega, M. Lolli, B. Martino, M. Martucci, G. Masciantonio, M. Mergè, M. Mese, A. Morbidini, F. Nuccilli, F. Nozzoli, A. Oliva, G. Osteria, E. Papini, F. Palma, F. Palmonari, A. Parmentier, B. Panico, S. Perciballi, F. Perfetto, A. Perinelli, P. Picozza, M. Piersanti, M. Pozzato, G. Rebustini, D. Recchiuti, E. Ricci, M. Ricci, J. Rodi, A. Russi, S. B. Ricciarini, Z. Sahnoun, U. Savino, V. Scotti, X. Shen, A. Sotgiu, R. Sparvoli, S. Tofani, P. Ubertini, N. Vertolli, V. Vilona, U. Zannoni, Z. Zeren, S. Zoffoli, P. Zuccon
Publikováno v:
The Astrophysical Journal Letters, Vol 946, Iss 1, p L29 (2023)
High-energy, long gamma-ray bursts (GRBs) can be generated by the core collapse of massive stars at the end of their lives. When they happen in the close-by universe they can be exceptionally bright, as seen from the Earth in the case of the recent,
Externí odkaz:
https://doaj.org/article/a26169c0241b4e06b6ea8fcba4266db4
Autor:
Parmentier, Geneviève
Galactic globular clusters contain two main groups of stars, the pristine or 1P stars, and the polluted or 2P stars. The pristine-star fraction in clusters, $F_{1P}$, is a decreasing function of the cluster present-day mass, $m_{prst}$. Paper~I has i
Externí odkaz:
http://arxiv.org/abs/2410.11950
Autor:
Ohno, Kazumasa, Schlawin, Everett, Bell, Taylor J., Murphy, Matthew M., Beatty, Thomas G., Welbanks, Luis, Greene, Thomas P., Fortney, Jonathan J., Parmentier, Vivien, Edelman, Isaac R., Mehta, Nishil, Rieke, Marcia J.
GJ1214b is the archetype sub-Neptune for which thick aerosols have prevented us from constraining its atmospheric properties for over a decade. In this study, we leverage the panchromatic transmission spectrum of GJ1214b established by HST and JWST t
Externí odkaz:
http://arxiv.org/abs/2410.10186
Autor:
Schlawin, Everett, Ohno, Kazumasa, Bell, Taylor J., Murphy, Matthew M., Welbanks, Luis, Beatty, Thomas G., Greene, Thomas P., Fortney, Jonathan J., Parmentier, Vivien, Edelman, Isaac R., Gill, Samuel, Anderson, David R., Wheatley, Peter J., Henry, Gregory W., Mehta, Nishil, Kreidberg, Laura, Rieke, Marcia J.
Sub-Neptune planets with radii smaller than Neptune (3.9 Re) are the most common type of planet known to exist in The Milky Way, even though they are absent in the Solar System. These planets can potentially have a large diversity of compositions as
Externí odkaz:
http://arxiv.org/abs/2410.10183
Autor:
Jacobs, Bob, Désert, Jean-Michel, Lewis, Nikole, Challener, Ryan C., Mayorga, L. C., de Beurs, Zoë, Parmentier, Vivien, Stevenson, Kevin B., de Wit, Julien, Barat, Saugata, Fortney, Jonathan, Kataria, Tiffany, Line, Michael
The extreme environments of transiting close-in exoplanets in highly-eccentric orbits are ideal for testing exo-climate physics. Spectroscopically resolved phase curves not only allow for the characterization of their thermal response to irradiation
Externí odkaz:
http://arxiv.org/abs/2410.11643
When optimizing transportation systems, anticipating traffic flows is a central element. Yet, computing such traffic equilibria remains computationally expensive. Against this background, we introduce a novel combinatorial optimization augmented neur
Externí odkaz:
http://arxiv.org/abs/2410.06656
Autor:
Fisher, Chloe, Taylor, Jake, Parmentier, Vivien, Kitzmann, Daniel, Birkby, Jayne L., Radica, Michael, Barstow, Joanna, Yang, Jingxuan, Morello, Giuseppe
The Hubble Space Telescope has been a pioneering instrument for studying the atmospheres of exoplanets, specifically its WFC3 and STIS instruments. With the launch of JWST, we are able to observe larger spectral ranges at higher precision. NIRISS/SOS
Externí odkaz:
http://arxiv.org/abs/2409.17042
Autor:
Delagrange, Raphaëlle, Garg, Manjari, Breton, Gaëlle Le, Zhang, Aifei, Dong, Quan, Jin, Yong, Watanabe, Kenji, Taniguchi, Takashi, Roulleau, Preden, Maillet, Olivier, Roche, Patrice, Parmentier, François D.
Under high perpendicular magnetic field and at low temperatures, graphene develops an insulating state at the charge neutrality point. This state, dubbed $\nu=0$, is due to the interplay between electronic interactions and the four-fold spin and vall
Externí odkaz:
http://arxiv.org/abs/2409.08878