Zobrazeno 1 - 10
of 1 383
pro vyhledávání: '"Oliva, C."'
Autor:
Nogueira, P. H., Lazzoni, C., Zurlo, A., Bhowmik, T., Donoso-Oliva, C., Desidera, S., Milli, J., Pérez, S., Delorme, P., Fernadez, A., Langlois, M., Petrus, S., Cabrera-Vives, G., Chauvin, G.
Publikováno v:
A&A 687, A301 (2024)
$\eta$ Tel is an 18 Myr system with a 2.09 M$_{\odot}$ A-type star and an M7-M8 brown dwarf companion, $\eta$ Tel B, separated by 4.2'' (208 au). High-contrast imaging campaigns over 20 years have enabled orbital and photometric characterization. $\e
Externí odkaz:
http://arxiv.org/abs/2405.04723
Publikováno v:
A&A 670, A54 (2023)
Taking inspiration from natural language embeddings, we present ASTROMER, a transformer-based model to create representations of light curves. ASTROMER was pre-trained in a self-supervised manner, requiring no human-labeled data. We used millions of
Externí odkaz:
http://arxiv.org/abs/2205.01677
Autor:
Sánchez-Sáez, P., Lira, H., Martí, L., Sánchez-Pi, N., Arredondo, J., Bauer, F. E., Bayo, A., Cabrera-Vives, G., Donoso-Oliva, C., Estévez, P. A., Eyheramendy, S., Förster, F., Hernández-García, L., Arancibia, A. M. Muñoz, Pérez-Carrasco, M., Sepúlveda, M., Vergara, J. R.
Publikováno v:
AJ 162 206 (2021)
The classic classification scheme for Active Galactic Nuclei (AGNs) was recently challenged by the discovery of the so-called changing-state (changing-look) AGNs (CSAGNs). The physical mechanism behind this phenomenon is still a matter of open debate
Externí odkaz:
http://arxiv.org/abs/2106.07660
In the new era of very large telescopes, where data is crucial to expand scientific knowledge, we have witnessed many deep learning applications for the automatic classification of lightcurves. Recurrent neural networks (RNNs) are one of the models u
Externí odkaz:
http://arxiv.org/abs/2106.03736
Autor:
Förster, F., Cabrera-Vives, G., Castillo-Navarrete, E., Estévez, P. A., Sánchez-Sáez, P., Arredondo, J., Bauer, F. E., Carrasco-Davis, R., Catelan, M., Elorrieta, F., Eyheramendy, S., Huijse, P., Pignata, G., Reyes, E., Reyes, I., Rodríguez-Mancini, D., Ruz-Mieres, D., Valenzuela, C., Alvarez-Maldonado, I., Astorga, N., Borissova, J., Clocchiatti, A., De Cicco, D., Donoso-Oliva, C., Graham, M. J., Kurtev, R., Mahabal, A., Maureira, J. C., Molina-Ferreiro, R., Moya, A., Palma, W., Pérez-Carrasco, M., Protopapas, P., Romero, M., Sabatini-Gacitúa, L., Sánchez, A., Martín, J. San, Sepúlveda-Cobo, C., Vera, E., Vergara, J. R.
We introduce the Automatic Learning for the Rapid Classification of Events (ALeRCE) broker, an astronomical alert broker designed to provide a rapid and self--consistent classification of large etendue telescope alert streams, such as that provided b
Externí odkaz:
http://arxiv.org/abs/2008.03303
Autor:
Molina-Mateo, D., Valderrama, B.P., Zárate, R.V., Hidalgo, S., Tamayo-Leiva, J., Soto-González, A., Guerra-Ayala, S., Arriagada-Vera, V., Oliva, C., Diez, B., Campusano, J.M.
Publikováno v:
In Neuropharmacology 15 September 2023 236
Autor:
Sessa, C., Cortes, J., Conte, P., Cardoso, F., Choueiri, T., Dummer, R., Lorusso, P., Ottmann, O., Ryll, B., Mok, T., Tempero, M., Comis, S., Oliva, C., Peters, S., Tabernero, J.
Publikováno v:
In ESMO Open February 2022 7(1)
Autor:
Nogueira, P. H., Lazzoni, C., Zurlo, A., Bhowmik, T., Donoso-Oliva, C., Desidera, S., Milli, J., Pérez, S., Delorme, P., Fernadez, A., Langlois, M., Petrus, S., Cabrera-Vives, G., Chauvin, G.
Publikováno v:
Astronomy & Astrophysics / Astronomie et Astrophysique; 7/15/2024, Vol. 687, p1-13, 13p
Autor:
Allieta, M., Scavini, M., Lopresti, L., Coduri, M., Loconte, L., Cappelli, S., Oliva, C., Ghigna, P., Pattison, P., Scagnoli, V.
We present a detailed study on the charge ordering (CO) transition in GdBaCo2O5 system by combining high resolution synchrotron powder/single crystal diffraction with electron paramagnetic resonance (EPR) experiments as a function of temperature. We
Externí odkaz:
http://arxiv.org/abs/1307.2692
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.