O. Peles
4 Papers
2 Citations
O. Peles is an academic researcher. The author has contributed to research in topics: Terrestrial planet & Planetary system. The author has an hindex of 1, co-authored 2 publications.
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Papers
Post-operative glioblastoma multiforme segmentation with uncertainty estimation
TL;DR: In this paper , an ensemble of segmentation networks and the Kullback-Leibler divergence agreement score in the objective function is used to estimate the prediction label uncertainty and cope with noisy labels and inter-observer variability.
Stability of Terrestrial Planets in the Habitable Zone of Gl 777 A, HD 72659, Gl 614, 47 Uma and HD 4208
N. Asghari,C. Broeg,L. Carone,Rigoberto A. Casas-Miranda,J. C. Castro Palacio,I. Csillik,Rudolf Dvorak,F. Freistetter,G. Hadjivantsides,Hauke Hussmann,A. Khramova,M. Khristoforova,I. Khromova,I. Kitiashivilli,S. Kozlowski,T. Laakso,T. Laczkowski,D. Lytvinenko,O. Miloni,Ryuji Morishima,Amaya Moro-Martin,V. Paksyutov,A. Pal,Vinod Patidar,B. Pecnik,O. Peles,J. Pyo,Thomas R. Quinn,Adrián Rodríguez,C. Romano,Eeshankur Saikia,Joachim Stadel,Marco Thiel,N. Todorovic,Dimitri Veras,E. Vieira Neto,Jozef Vilagi,W. von Bloh,R. Zechner,E. Zhuchkova +39 more
TL;DR: In this article, the authors investigated the mean motion resonances between fictitious terrestrial planets and the existing gas giants in these five extrasolar systems, and then a fine grid of initial conditions for a potential terrestrial planet within the HZ was chosen for each system, from which the stability of orbits was then assessed by direct integrations over a time interval of 1 million years.
Estimating the lowest latitude of baroclinic growth
O. Peles,Orli Lachmy +1 more
TL;DR: In this article , a new estimate for the lowest latitude of baroclinic growth was proposed, based on the assumption that barocliic growth is limited by the vertical scale of eddy fluxes.
Stability of terrestrial planets in the habitable zone of Gl 777 A, HD 72659, Gl 614, 47 Uma and HD 4208
N. Asghari,C. Broeg,L. Carone,Rigoberto A. Casas-Miranda,J. C. Castro Palacio,I. Csillik,Rudolf Dvorak,F. Freistetter,G. Hadjivantsides,Hauke Hussmann,A. Khramova,M. Khristoforova,I. Khromova,I. Kitiashivilli,S. Kozlowski,T. Laakso,T. Laczkowski,D. Lytvinenko,O. Miloni,Ryuji Morishima,Amaya Moro-Martin,V. Paksyutov,A. Pal,Vinod Patidar,B. Pecnik,O. Peles,J. Pyo,Thomas R. Quinn,Adrián Rodríguez,C. Romano,Eeshankur Saikia,Joachim Stadel,Marco Thiel,N. Todorovic,Dimitri Veras,E. Vieira Neto,Jozef Vilagi,W. von Bloh,R. Zechner,E. Zhuchkova +39 more
TL;DR: In this paper, the authors performed a thorough dynamical investigation of five extrasolar planetary systems using extensive numerical experiments on the supercomputer of the Max Planck Institute for Gravitational Physics (Albert Einstein Institute).