Zobrazeno 1 - 10
of 27 203
pro vyhledávání: '"A, Fumagalli"'
While the orbital eccentricity is a key feature of the gravitational two-body problem, providing an unambiguous definition in General Relativity poses significant challenges. Despite such foundational issue, the eccentricity of binary black holes has
Externí odkaz:
http://arxiv.org/abs/2411.00098
Autor:
Hui, Tong, Fumagalli, Matteo
As aerial robots gain traction in industrial applications, there is growing interest in enhancing their physical interaction capabilities. Pushing tasks performed by aerial manipulators have been successfully demonstrated in contact-based inspections
Externí odkaz:
http://arxiv.org/abs/2410.22816
Autor:
Berra, Andrea, Sankaranarayanan, Viswa Narayanan, Seisa, Achilleas Santi, Mellet, Julien, Gamage, Udayanga G. W. K. N., Satpute, Sumeet Gajanan, Ruggiero, Fabio, Lippiello, Vincenzo, Tolu, Silvia, Fumagalli, Matteo, Nikolakopoulos, George, Soto, Miguel Ángel Trujillo, Heredia, Guillermo
Publikováno v:
2024 International Conference on Unmanned Aircraft Systems (ICUAS)
The paper introduces a novel framework for safe and autonomous aerial physical interaction in industrial settings. It comprises two main components: a neural network-based target detection system enhanced with edge computing for reduced onboard compu
Externí odkaz:
http://arxiv.org/abs/2410.15802
We consider a mixed formulation of parametrized elasticity problems in terms of stress, displacement, and rotation. The latter two variables act as Lagrange multipliers to enforce conservation of linear and angular momentum. Due to the saddle-point s
Externí odkaz:
http://arxiv.org/abs/2410.06975
Autor:
Pensabene, A., Galbiati, M., Fumagalli, M., Fossati, M., Smail, I., Rafelski, M., Revalski, M., Arrigoni-Battaia, F., Beckett, A., Cantalupo, S., Dutta, R., Lusso, E., Lazeyras, T., Quadri, G., Tornotti, D.
We present new ALMA continuum and spectral observations of the MUSE Ultra Deep Field (MUDF), a $2\times 2$ arcmin$^2$ region with ultradeep multiwavelength imaging and spectroscopy hosting two bright $z\approx 3.22$ quasars used to study intervening
Externí odkaz:
http://arxiv.org/abs/2410.06249
Autor:
Galbiati, M., Cantalupo, S., Steidel, C., Pensabene, A., Travascio, A., Wang, W., Fossati, M., Fumagalli, M., Rudie, G., Fresco, A., Lazeyras, T., Ledos, N., Quadri, G.
A direct link between large-scale environment and galaxy properties is very well established in the local universe. However, very little is known about the role of the environment for galaxy growth before the peak of the cosmic star formation history
Externí odkaz:
http://arxiv.org/abs/2410.03822
We search for the galaxies associated with the intervening MgII absorbers over a redshift range of $0.4 \le z \le 1.0$ using imaging data from DESI Legacy Imaging Surveys and measure the redshift based on direct detection of nebular emission in the b
Externí odkaz:
http://arxiv.org/abs/2410.03824
Autor:
Travascio, A., Cantalupo, S., Tozzi, P., Vito, F., Paggi, A., Pezzulli, G., Elvis, M., Fabbiano, G., Fiore, F., Fossati, M., Fresco, A., Fumagalli, M., Galbiati, M., Lazeyras, T., Ledos, N., Pannella, M., Pensabene, A., Quadri, G., Wang, W.
Exploring SMBH population in protoclusters offers valuable insights into how environment affects SMBH growth. However, research on AGN within these areas is still limited by the small number of protoclusters known at high redshift and by the availabi
Externí odkaz:
http://arxiv.org/abs/2410.03933
Autor:
Muschalik, Maximilian, Baniecki, Hubert, Fumagalli, Fabian, Kolpaczki, Patrick, Hammer, Barbara, Hüllermeier, Eyke
Originally rooted in game theory, the Shapley Value (SV) has recently become an important tool in machine learning research. Perhaps most notably, it is used for feature attribution and data valuation in explainable artificial intelligence. Shapley I
Externí odkaz:
http://arxiv.org/abs/2410.01649
Autor:
Wang, Weichen, Cantalupo, Sebastiano, Pensabene, Antonio, Galbiati, Marta, Travascio, Andrea, Steidel, Charles C., Maseda, Michael V., Pezzulli, Gabriele, de Beer, Stephanie, Fossati, Matteo, Fumagalli, Michele, Gallego, Sofia G., Lazeyras, Titouan, Mackenzie, Ruari, Matthee, Jorryt, Nanayakkara, Themiya, Quadri, Giada
Observational studies showed that galaxy disks are already in place in the first few billion years of the universe. The early disks detected so far, with typical half-light radii of 3 kiloparsecs at stellar masses around 10^11 M_sun for redshift z~3,
Externí odkaz:
http://arxiv.org/abs/2409.17956