Zobrazeno 1 - 10
of 14 273
pro vyhledávání: '"de Lorenzo, A."'
Autor:
Andersen, Trond I., Astrakhantsev, Nikita, Karamlou, Amir, Berndtsson, Julia, Motruk, Johannes, Szasz, Aaron, Gross, Jonathan A., Westerhout, Tom, Zhang, Yaxing, Forati, Ebrahim, Rossi, Dario, Kobrin, Bryce, Di Paolo, Agustin, Klots, Andrey R., Drozdov, Ilya, Kurilovich, Vladislav D., Petukhov, Andre, Ioffe, Lev B., Elben, Andreas, Rath, Aniket, Vitale, Vittorio, Vermersch, Benoit, Acharya, Rajeev, Beni, Laleh Aghababaie, Anderson, Kyle, Ansmann, Markus, Arute, Frank, Arya, Kunal, Asfaw, Abraham, Atalaya, Juan, Ballard, Brian, Bardin, Joseph C., Bengtsson, Andreas, Bilmes, Alexander, Bortoli, Gina, Bourassa, Alexandre, Bovaird, Jenna, Brill, Leon, Broughton, Michael, Browne, David A., Buchea, Brett, Buckley, Bob B., Buell, David A., Burger, Tim, Burkett, Brian, Bushnell, Nicholas, Cabrera, Anthony, Campero, Juan, Chang, Hung-Shen, Chen, Zijun, Chiaro, Ben, Claes, Jahan, Cleland, Agnetta Y., Cogan, Josh, Collins, Roberto, Conner, Paul, Courtney, William, Crook, Alexander L., Das, Sayan, Debroy, Dripto M., De Lorenzo, Laura, Barba, Alexander Del Toro, Demura, Sean, Devoret, Michel, Donohoe, Paul, Dunsworth, Andrew, Earle, Clint, Eickbusch, Alec, Elbag, Aviv Moshe, Elzouka, Mahmoud, Erickson, Catherine, Faoro, Lara, Fatemi, Reza, Ferreira, Vinicius S., Burgos, Leslie Flores, Fowler, Austin G., Foxen, Brooks, Ganjam, Suhas, Gasca, Robert, Giang, William, Gidney, Craig, Gilboa, Dar, Giustina, Marissa, Gosula, Raja, Dau, Alejandro Grajales, Graumann, Dietrich, Greene, Alex, Habegger, Steve, Hamilton, Michael C., Hansen, Monica, Harrigan, Matthew P., Harrington, Sean D., Heslin, Stephen, Heu, Paula, Hill, Gordon, Hoffmann, Markus R., Huang, Hsin-Yuan, Huang, Trent, Huff, Ashley, Huggins, William J., Isakov, Sergei V., Jeffrey, Evan, Jiang, Zhang, Jones, Cody, Jordan, Stephen, Joshi, Chaitali, Juhas, Pavol, Kafri, Dvir, Kang, Hui, Kechedzhi, Kostyantyn, Khaire, Trupti, Khattar, Tanuj, Khezri, Mostafa, Kieferová, Mária, Kim, Seon, Kitaev, Alexei, Klimov, Paul V., Korotkov, Alexander N., Kostritsa, Fedor, Kreikebaum, John Mark, Landhuis, David, Langley, Brandon W., Laptev, Pavel, Lau, Kim-Ming, Guevel, Loïck Le, Ledford, Justin, Lee, Joonho, Lee, Kenny, Lensky, Yuri D., Lester, Brian J., Li, Wing Yan, Lill, Alexander T., Liu, Wayne, Livingston, William P., Locharla, Aditya, Lundahl, Daniel, Lunt, Aaron, Madhuk, Sid, Maloney, Ashley, Mandrà, Salvatore, Martin, Leigh S., Martin, Orion, Martin, Steven, Maxfield, Cameron, McClean, Jarrod R., McEwen, Matt, Meeks, Seneca, Miao, Kevin C., Mieszala, Amanda, Molina, Sebastian, Montazeri, Shirin, Morvan, Alexis, Movassagh, Ramis, Neill, Charles, Nersisyan, Ani, Newman, Michael, Nguyen, Anthony, Nguyen, Murray, Ni, Chia-Hung, Niu, Murphy Yuezhen, Oliver, William D., Ottosson, Kristoffer, Pizzuto, Alex, Potter, Rebecca, Pritchard, Orion, Pryadko, Leonid P., Quintana, Chris, Reagor, Matthew J., Rhodes, David M., Roberts, Gabrielle, Rocque, Charles, Rosenberg, Eliott, Rubin, Nicholas C., Saei, Negar, Sankaragomathi, Kannan, Satzinger, Kevin J., Schurkus, Henry F., Schuster, Christopher, Shearn, Michael J., Shorter, Aaron, Shutty, Noah, Shvarts, Vladimir, Sivak, Volodymyr, Skruzny, Jindra, Small, Spencer, Smith, W. Clarke, Springer, Sofia, Sterling, George, Suchard, Jordan, Szalay, Marco, Sztein, Alex, Thor, Douglas, Torres, Alfredo, Torunbalci, M. Mert, Vaishnav, Abeer, Vdovichev, Sergey, Villalonga, Benjamin, Heidweiller, Catherine Vollgraff, Waltman, Steven, Wang, Shannon X., White, Theodore, Wong, Kristi, Woo, Bryan W., Xing, Cheng, Yao, Z. Jamie, Yeh, Ping, Ying, Bicheng, Yoo, Juhwan, Yosri, Noureldin, Young, Grayson, Zalcman, Adam, Zhu, Ningfeng, Zobrist, Nicholas, Neven, Hartmut, Babbush, Ryan, Boixo, Sergio, Hilton, Jeremy, Lucero, Erik, Megrant, Anthony, Kelly, Julian, Chen, Yu, Smelyanskiy, Vadim, Vidal, Guifre, Roushan, Pedram, Lauchli, Andreas M., Abanin, Dmitry A., Mi, Xiao
Understanding how interacting particles approach thermal equilibrium is a major challenge of quantum simulators. Unlocking the full potential of such systems toward this goal requires flexible initial state preparation, precise time evolution, and ex
Externí odkaz:
http://arxiv.org/abs/2405.17385
Autor:
Kim, Taehyun, Gadotti, Dimitri A., Querejeta, Miguel, Pérez, Isabel, Zurita, Almudena, Neumann, Justus, van de Ven, Glenn, Méndez-Abreu, Jairo, de Lorenzo-Cáceres, Adriana, Sánchez-Blázquez, Patricia, Fragkoudi, Francesca, Martins, Lucimara P., Silva-Lima, Luiz A., Kim, Woong-Tae, Park, Myeong-gu
Bars drive gas inflow. As the gas flows inwards, shocks and shear occur along the bar dust lanes. Such shocks and shear can affect the star formation and change the gas properties. For four barred galaxies, we present H{\alpha} velocity gradient maps
Externí odkaz:
http://arxiv.org/abs/2405.00107
Autor:
Prieto-Fernández, Natalia, Fernández-Blanco, Sergio, Fernández-Blanco, Álvaro, Benítez-Andrades, José Alberto, Carro-De-Lorenzo, Francisco, Benavides, Carmen
Publikováno v:
IEEE Transactions on Instrumentation and Measurement, Volume 72, June 2023, 8504110
One of the main challenges in simultaneous localization and mapping (SLAM) is real-time processing. High-computational loads linked to data acquisition and processing complicate this task. This article presents an efficient feature extraction approac
Externí odkaz:
http://arxiv.org/abs/2402.03376
Autor:
Cuomo, V., Morelli, L., Aguerri, J. A. L., Corsini, E. M., Debattista, V. P., Coccato, L., Pizzella, A., Boselli, A., Buttitta, C., de Lorenzo-Cáceres, A., Ferrarese, L., Gasparri, D., Lee, Y. H., Mendez-Abreu, J., Roediger, J., Zarattini, S.
Dwarf barred galaxies are the perfect candidates for hosting slowly-rotating bars. They are common in dense environments and they have a relatively shallow potential well, making them prone to heating by interactions. When an interaction induces bar
Externí odkaz:
http://arxiv.org/abs/2312.14017
Autor:
Martín-Navarro, Ignacio, de Lorenzo-Cáceres, Adriana, Gadotti, Dimitri A., Méndez-Abreu, Jairo, Falcón-Barroso, Jesús, Sánchez-Blázquez, Patricia, Coelho, Paula, Neumann, Justus, van de Ven, Glenn, Pérez, Isabel
The debate about the universality of the stellar initial mass function (IMF) revolves around two competing lines of evidence. While measurements in the Milky Way, an archetypal spiral galaxy, seem to support an invariant IMF, the observed properties
Externí odkaz:
http://arxiv.org/abs/2312.13355
Autor:
Tahmasebzadeh, Behzad, Zhu, Ling, Shen, Juntai, Gadotti, Dimitri A., Valluri, Monica, Thater, Sabine, van de Ven, Glenn, Jin, Yunpeng, Gerhard, Ortwin, Erwin, Peter, Jethwa, Prashin, Zocchi, Alice, Lilley, Edward J., Fragkoudi, Francesca, de Lorenzo-Cáceres, Adriana, Méndez-Abreu, Jairo, Neumann, Justus, Guo, Rui
We apply the barred Schwarzschild method developed by Tahmasebzadeh et al. (2022) to a barred S0 galaxy, NGC 4371, observed by IFU instruments from the TIMER and ATLAS3D projects. We construct the gravitational potential by combining a fixed black ho
Externí odkaz:
http://arxiv.org/abs/2310.00497
Double bars make up a significant fraction of barred galaxies. We propose a new formation scenario for double bars that involves tidal interactions. We demonstrate the viability of this scenario using two examples of simulated galaxies from run TNG50
Externí odkaz:
http://arxiv.org/abs/2309.17180
Autor:
Nogueras-Lara, F., Feldmeier-Krause, A., Schödel, R., Sormani, M. C., de Lorenzo-Cáceres, A., Mastrobuono-Battisti, A., Schultheis, M., Neumayer, N., Rich, R. M., Nieuwmunster, N.
Publikováno v:
A&A 680, A75 (2023)
The innermost regions of most galaxies are characterised by the presence of extremely dense nuclear star clusters. Nevertheless, these clusters are not the only stellar component present in galactic nuclei, where larger stellar structures known as nu
Externí odkaz:
http://arxiv.org/abs/2309.07219
Autor:
de Sá-Freitas, Camila, Gadotti, Dimitri A., Fragkoudi, Francesca, Coccato, Lodovico, Coelho, Paula, de Lorenzo-Cáceres, Adriana, Falcón-Barroso, Jesús, Kolcu, Tutku, Martín-Navarro, Ignacio, Mendez-Abreu, Jairo, Neumann, Justus, Blazquez, Patricia Sanchez, Querejeta, Miguel, van de Ven, Glenn
Publikováno v:
A&A 678, A202 (2023)
When galactic discs settle and become massive enough, they are able to form stellar bars. These non-axisymmetric structures induce shocks in the gas, causing it to flow to the centre where nuclear structures, such as nuclear discs and rings, are form
Externí odkaz:
http://arxiv.org/abs/2308.04482
Autor:
Ashok, Aishwarya, Seth, Anil, Erwin, Peter, Debattista, Victor P., de Lorenzo-Cáceres, Adriana, Gadotti, Dmitri A., Méndez-Abreu, Jairo, Beckman, John E., Bender, Ralf, Drory, Niv, Fisher, Deanne, Hopp, Ulrich, Kluge, Matthias, Kolcu, Tutku, Maciejewski, Witold, Mehrgan, Kianusch, Parikh, Taniya, Saglia, Roberto, Seidel, Marja, Thomas, Jens
We present photometric and morphological analyses of nuclear star clusters (NSCs) -- very dense, massive star clusters present in the central regions of most galaxies -- in a sample of 33 massive disk galaxies within 20 Mpc, part of the "Composite Bu
Externí odkaz:
http://arxiv.org/abs/2308.03913