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pro vyhledávání: '"P, Freour"'
Accretion disks surrounding stellar mass black holes (BHs) have been suggested as potential locations for the nucleosynthesis of light elements, which are our primary observational discriminant of multiple stellar populations within globular clusters
Externí odkaz:
http://arxiv.org/abs/2402.10590
Autor:
Schulze, Steve, Fransson, Claes, Kozyreva, Alexandra, Chen, Ting-Wan, Yaron, Ofer, Jerkstrand, Anders, Gal-Yam, Avishay, Sollerman, Jesper, Yan, Lin, Kangas, Tuomas, Leloudas, Giorgos, Omand, Conor M. B., Smartt, Stephen J., Yang, Yi, Nicholl, Matt, Sarin, Nikhil, Yao, Yuhan, Brink, Thomas G., Sharon, Amir, Rossi, Andrea, Chen, Ping, Chen, Zhihao, Cikota, Aleksandar, De, Kishalay, Drake, Andrew J., Filippenko, Alexei V., Fremling, Christoffer, Freour, Laurane, Fynbo, Johan P. U., Ho, Anna Y. Q., Inserra, Cosimo, Irani, Ido, Kuncarayakti, Hanindyo, Lunnan, Ragnhild, Mazzali, Paolo, Ofek, Eran O., Palazzi, Eliana, Perley, Daniel A., Pursiainen, Miika, Rothberg, Barry, Shingles, Luke J., Smith, Ken, Taggart, Kirsty, Tartaglia, Leonardo, Zheng, WeiKang, Anderson, Joseph P., Cassara, Letizia, Christensen, Eric, Djorgovski, S. George, Galbany, Lluis, Gkini, Anamaria, Graham, Matthew J., Gromadzki, Mariusz, Groom, Steven L., Hiramatsu, Daichi, Howell, D. Andrew, Kasliwal, Mansi M., McCully, Curtis, Müller-Bravo, Tomas E., Paiano, Simona, Paraskeva, Emmanouela, Pessi, Priscila J., Polishook, David, Rau, Arne, Rigault, Mickael, Rusholme, Ben
Abridged - Stars with ZAMS masses between 140 and $260 M_\odot$ are thought to explode as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe can produce up to several tens of solar masses of radioactive nickel, resulting i
Externí odkaz:
http://arxiv.org/abs/2305.05796
Autor:
A. Dezellus, S. Mirallie, F. Leperlier, B. Sauterey, P.-E. Bouet, A. Dessaint, S. Duros, A.S. Gremeau, M.-A. Mouret-Reynier, L.M. Durand, L. Venat, P. De Blay, M. Robert, T. Freour, M. Campone, A. Blanc-Lapierre, V. Bordes
Publikováno v:
Breast, Vol 77, Iss , Pp 103776- (2024)
Purpose: Fertility issues are of great concern for young women undergoing treatment for breast cancer (BC). Fertility preservation (FP) protocols using controlled ovarian stimulation (COS) with letrozole have been widely used with overall good result
Externí odkaz:
https://doaj.org/article/393c7a99dbb3420d92cf58ac97c87529
We present a spectropolarimetric analysis of the hot star V352Peg. We have acquired 18 spectropolarimetric observations of the star with ESPaDOnS at the CFHT between 2018 and 2019 and completed our dataset with one archival ESPaDOnS measurement obtai
Externí odkaz:
http://arxiv.org/abs/2207.12887
An important limitation to the development of AI-based solutions for In Vitro Fertilization (IVF) is the black-box nature of most state-of-the-art models, due to the complexity of deep learning architectures, which raises potential bias and fairness
Externí odkaz:
http://arxiv.org/abs/2205.06546
Autor:
Gomez, Tristan, Feyeux, Magalie, Normand, Nicolas, David, Laurent, Paul-Gilloteaux, Perrine, Fréour, Thomas, Mouchère, Harold
An important limitation to the development of Artificial Intelligence (AI)-based solutions for In Vitro Fertilization (IVF) is the absence of a public reference benchmark to train and evaluate deep learning (DL) models. In this work, we describe a fu
Externí odkaz:
http://arxiv.org/abs/2203.00531
Due to the black-box nature of deep learning models, there is a recent development of solutions for visual explanations of CNNs. Given the high cost of user studies, metrics are necessary to compare and evaluate these different methods. In this paper
Externí odkaz:
http://arxiv.org/abs/2201.13291
Autor:
Fukui, A., Korth, J., Livingston, J. H., Twicken, J. D., Osorio, M. R. Zapatero, Jenkins, J. M., Mori, M., Murgas, F., Ogihara, M., Narita, N., Pallé, E., Stassun, K. G., Nowak, G., Ciardi, D. R., Alvarez-Hernandez, L., Béjar, V. J. S., Casasayas-Barris, N., Crouzet, N., de Leon, J. P., Esparza-Borges, E., Soto, D. Hidalgo, Isogai, K., Kawauchi, K., Klagyivik, P., Kodama, T., Kurita, S., Kusakabe, N., Luque, R., Madrigal-Aguado, A., Rodriguez, P. Montanes, Morello, G., Nishiumi, T., Orell-Miquel, J., Oshagh, M., Parviainen, H., Sánchez-Benavente, M., Stangret, M., Watanabe, N., Chen, G., Tamura, M., Bosch-Cabot, P., Bowen, M., Eastridge, K., Freour, L., Gonzales, E., Guerra, P., Jundiyeh, Y., Kim, T. K., Kroer, L. V., Levine, A. M., Morgan, E. H., Reefe, M., Tronsgaard, R., Wedderkopp, C. K., Wittrock, J., Collins, K. A., Hesse, K., Latham, D. W., Ricker, G. R., Seager, S., Vanderspek, R., Winn, J., Bachelet, E., Bowman, M., McCully, C., Daily, M., Harbeck, D., Volgenau, N. H.
Publikováno v:
Astronomical Journal, 162, 167 (2021)
We report the discovery of one super-Earth- (TOI-1749b) and two sub-Neptune-sized planets (TOI-1749c and TOI-1749d) transiting an early M dwarf at a distance of 100~pc, which were first identified as planetary candidates using data from the TESS phot
Externí odkaz:
http://arxiv.org/abs/2107.05430
The prevalence of employing attention mechanisms has brought along concerns on the interpretability of attention distributions. Although it provides insights about how a model is operating, utilizing attention as the explanation of model predictions
Externí odkaz:
http://arxiv.org/abs/2106.02566
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