Zobrazeno 1 - 10
of 5 025
pro vyhledávání: '"P. Van De Ven"'
In this study, we present the Graph Sub-Graph Network (GSN), a novel hybrid image classification model merging the strengths of Convolutional Neural Networks (CNNs) for feature extraction and Graph Neural Networks (GNNs) for structural modeling. GSN
Externí odkaz:
http://arxiv.org/abs/2407.14772
Autor:
Koller, M., Ziegler, B., Ciocan, B. I., Thater, S., Mendel, J. T., Wisnioski, E., Battisti, A. J., Harborne, K. E., Foster, C., Lagos, C., Croom, S. M., Grasha, K., Papaderos, P., Remus, R. S., Sharma, G., Sweet, S. M., Valenzuela, L. M., van de Ven, G., Zafar, T.
Star formation rates (SFRs), gas-phase metallicities, and stellar masses are crucial for studying galaxy evolution. The different relations resulting from these properties give insights into the complex interplay of gas inside galaxies and their evol
Externí odkaz:
http://arxiv.org/abs/2406.20017
We study the classical and quantum KMS conditions within the context of spin lattice systems. Specifically, we define a strict deformation quantization (SDQ) for a $\mathbb{S}^2$-valued spin lattice system over $\mathbb{Z}^d$ generalizing the renown
Externí odkaz:
http://arxiv.org/abs/2406.12342
Autor:
Nitschai, M. S., Neumayer, N., Häberle, M., Clontz, C., Seth, A. C., Milone, A. P., Alfaro-Cuello, M., Bellini, A., Dreizler, S., Feldmeier-Krause, A., Husser, T. -O., Kacharov, N., Kamann, S., Latour, M., Libralato, M., van de Ven, G., Voggel, K., Wang, Z.
Publikováno v:
ApJ 970, 152 (2024)
$\omega$ Centauri, the most massive globular cluster in the Milky Way, has long been suspected to be the stripped nucleus of a dwarf galaxy that fell into the Galaxy a long time ago. There is considerable evidence for this scenario including a large
Externí odkaz:
http://arxiv.org/abs/2406.01688
Autor:
Häberle, Maximilian, Neumayer, Nadine, Seth, Anil, Bellini, Andrea, Libralato, Mattia, Baumgardt, Holger, Whitaker, Matthew, Dumont, Antoine, Cuello, Mayte Alfaro, Anderson, Jay, Clontz, Callie, Kacharov, Nikolay, Kamann, Sebastian, Feldmeier-Krause, Anja, Milone, Antonino, Nitschai, Maria Selina, Pechetti, Renuka, van de Ven, Glenn
Publikováno v:
Nature 631, 285-288 (2024)
Black holes have been found over a wide range of masses, from stellar remnants with masses of 5-150 solar masses (Msun), to those found at the centers of galaxies with $M>10^5$ Msun. However, only a few debated candidate black holes exist between 150
Externí odkaz:
http://arxiv.org/abs/2405.06015
Autor:
Hemati, Hamed, Pellegrini, Lorenzo, Duan, Xiaotian, Zhao, Zixuan, Xia, Fangfang, Masana, Marc, Tscheschner, Benedikt, Veas, Eduardo, Zheng, Yuxiang, Zhao, Shiji, Li, Shao-Yuan, Huang, Sheng-Jun, Lomonaco, Vincenzo, van de Ven, Gido M.
Continual learning (CL) provides a framework for training models in ever-evolving environments. Although re-occurrence of previously seen objects or tasks is common in real-world problems, the concept of repetition in the data stream is not often con
Externí odkaz:
http://arxiv.org/abs/2405.04101
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:
Häberle, Maximilian, Neumayer, Nadine, Bellini, Andrea, Libralato, Mattia, Clontz, Callie, Seth, Anil C., Nitschai, Maria Selina, Kamann, Sebastian, Alfaro-Cuello, Mayte, Anderson, Jay, Dreizler, Stefan, Feldmeier-Krause, Anja, Kacharov, Nikolay, Latour, Marilyn, Milone, Antonino, Pechetti, Renuka, van de Ven, Glenn, Voggel, Karina
Publikováno v:
ApJ 970 192 (2024)
Omega Centauri ($\omega$ Cen) is the most massive globular cluster of the Milky Way. It is thought to be the nucleus of an accreted dwarf galaxy because of its high mass and its complex stellar populations. To decipher its formation history and study
Externí odkaz:
http://arxiv.org/abs/2404.03722
Autor:
Ding, Yuchen, Zhu, Ling, Pillepich, Annalisa, van de Ven, Glenn, Iodice, Enrichetta, Corsini, Enrico Maria, Pinna, Francesca
Publikováno v:
A&A 686, A184 (2024)
We studied the effects of cluster environments on galactic structures by using the TNG50 cosmological simulation and observed galaxies in the Fornax cluster. We focused on galaxies with stellar masses of $10^{8-12}M_{\odot}$ at z=0 that reside in For
Externí odkaz:
http://arxiv.org/abs/2404.01541
Autor:
Veršič, Tadeja, Rejkuba, Marina, Arnaboldi, Magda, Gerhard, Ortwin, Pulsoni, Claudia, Valenzuela, Lucas M., Hartke, Johanna, Watkins, Laura L., van de Ven, Glenn, Thater, Sabine
Publikováno v:
A&A 687, A80 (2024)
Within the $\Lambda$CDM cosmology, dark matter haloes are expected to deviate from spherical symmetry. Constraining the halo shapes at large galactocentric distances is challenging due to the low density of luminous tracers. The well-studied early-ty
Externí odkaz:
http://arxiv.org/abs/2403.13109