Zobrazeno 1 - 10
of 24 962
pro vyhledávání: '"A Galvan"'
Gamma-ray bursts (GRBs) are intense pulses of high-energy emission associated with massive stars' death or compact objects' coalescence. Their multi-wavelength observations help verify the reliability of the standard fireball model. We analyze 14 GRB
Externí odkaz:
http://arxiv.org/abs/2411.10736
Autor:
Law, Charles J., Zhang, Qizhou, Frommer, Arielle C., Öberg, Karin I., Galván-Madrid, Roberto, Keto, Eric, Liu, Hauyu Baobab, Ho, Paul T. P., Izquierdo, Andrés F., Cleeves, L. Ilsedore
Massive star-forming regions exhibit a rich chemistry with complex gas distributions, especially on small scales. While surveys have yielded constraints on typical gas conditions, they often have coarse spatial resolution and limited bandwidths. Thus
Externí odkaz:
http://arxiv.org/abs/2411.00941
Autor:
Sandoval-Garrido, N. A., Stutz, A. M., Álvarez-Gutiérrez, R. H., Galván-Madrid, R., Motte, F., Ginsburg, A., Cunningham, N., Reyes-Reyes, S., Redaelli, E., Bonfand, M., Salinas, J., Koley, A., Braine, J., Bronfman, L., Busquet, G., Csengeri, T., Di Francesco, J., Fernández-López, M., Garcia, P., Gusdorf, A., Liu, H. -L., Sanhueza, P.
ALMA-IMF observed 15 massive protoclusters capturing multiple spectral lines and the continuum emission. We focus on the G351.77 protocluster ($\sim$ 2500 M$_{\odot}$, estimated from single-dish continuum observations) located at 2 kpc. We trace the
Externí odkaz:
http://arxiv.org/abs/2410.09843
Autor:
Galvan, Bruno
Cournot's principle states that a typical event (i.e., an event with probability very close to $1$) occurs nearly certainly in a single trial of an experiment. This principle has been considered by various authors as the only connection between mathe
Externí odkaz:
http://arxiv.org/abs/2410.05228
Autor:
Betancur-Ocampo, Yonatan, García, Santiago Galván y, Nuñez, Samuel Tehuacanero, Reyes-Gasga, José, Stegmann, Thomas, Sánchez-Ochoa, Francisco
The deposition of a two-dimensional material on the surface of a three-dimensional crystal can generate superlattices with electronic properties modified through the proximity spin-orbit effect. In this study, we found that Kekul\'e graphene superlat
Externí odkaz:
http://arxiv.org/abs/2409.18322
Autor:
Fraija, Nissim, Veres, P., Kamenetskaia, B. Betancourt, Galvan-Gamez, A., Dainotti, M. G., Dichiara, Simone, Becerra, R. L.
Energetic GeV photons expected from the closest and the most energetic Gamma-ray bursts (GRBs) provide an unique opportunity to study the very-high-energy emission as well as the possible correlations with lower energy bands in realistic GRB afterglo
Externí odkaz:
http://arxiv.org/abs/2409.12166
Music streaming services often leverage sequential recommender systems to predict the best music to showcase to users based on past sequences of listening sessions. Nonetheless, most sequential recommendation methods ignore or insufficiently account
Externí odkaz:
http://arxiv.org/abs/2408.16578
Autor:
Matrosova, Kristina, Marey, Lilian, Salha-Galvan, Guillaume, Louail, Thomas, Bodini, Olivier, Moussallam, Manuel
This paper examines the influence of recommender systems on local music representation, discussing prior findings from an empirical study on the LFM-2b public dataset. This prior study argued that different recommender systems exhibit algorithmic bia
Externí odkaz:
http://arxiv.org/abs/2408.16430
Flow-guided localization using in-body nanodevices in the bloodstream is expected to be beneficial for early disease detection, continuous monitoring of biological conditions, and targeted treatment. The nanodevices face size and power constraints th
Externí odkaz:
http://arxiv.org/abs/2408.01239
Autor:
Louvet, F., Sanhueza, P., Stutz, A., Men'shchikov, A., Motte, F., Galván-Madrid, R., Bontemps, S., Pouteau, Y., Ginsburg, A., Csengeri, T., Di Francesco, J., Dell'Ova, P., González, M., Didelon, P., Braine, J., Cunningham, N., Thomasson, B., Lesaffre, P., Hennebelle, P., Bonfand, M., Gusdorf, A., Álverez-Gutiérrez, R. H., Nony, T., Busquet, G., Olguin, F., Bronfman, L., Salinas, J., Fernandez-Lopez, M., Moraux, E., Liu, H. L., Lu, X., Huei-Ru, V., Towner, A., Valeille-Manet, M., Brouillet, N., Herpin, F., Lefloch, B., Baug, T., Maud, L., Lopez-Sepulcre, A., Svodoba, B.
Publikováno v:
A&A 690, A33 (2024)
The stellar initial mass function (IMF) is critical to our understanding of star formation and the effects of young stars on their environment. On large scales, it enables us to use tracers such as UV or Halpha emission to estimate the star formation
Externí odkaz:
http://arxiv.org/abs/2407.18719