Zobrazeno 1 - 10
of 17 992
pro vyhledávání: '"Kubiak AT"'
Autor:
Kubiak, Nikolina, Wortman, Elliot, Mustafa, Armin, Phillipson, Graeme, Jolly, Stephen, Hadfield, Simon
Existing shadow detection models struggle to differentiate dark image areas from shadows. In this paper, we tackle this issue by verifying that all detected shadows are real, i.e. they have paired shadow casters. We perform this step in a physically-
Externí odkaz:
http://arxiv.org/abs/2408.17143
Autor:
Anugu, Narsireddy, Gies, Douglas R., Roettenbacher, Rachael M., Monnier, John D., Montargés, Miguel, Mérand, Antoine, Baron, Fabien, Schaefer, Gail H., Shepard, Katherine A., Kraus, Stefan, Anderson, Matthew D., Codron, Isabelle, Gardner, Tyler, Gutierrez, Mayra, Köhler, Rainer, Kubiak, Karolina, Lanthermann, Cyprien, Majoinen, Olli, Scott, Nicholas J., Vollmann, Wolfgang
Stars with initial masses larger than 8 solar masses undergo substantial mass loss through mechanisms that remain elusive. Unraveling the origins of this mass loss is important for comprehending the evolutionary path of these stars, the type of super
Externí odkaz:
http://arxiv.org/abs/2408.11906
Autor:
Jany, Benedykt R., Madajska, Katarzyna, Butrymowicz-Kubiak, Aleksandra, Krok, Franciszek, Szymańska, Iwona B.
The development of modern metal deposition techniques like Focused Ion/Electron Beam Induced Deposition FIBID/FEBID relies heavily on the availability of metal-organic precursors of particular properties. To create a new precursor, extensive testing
Externí odkaz:
http://arxiv.org/abs/2406.10022
Interstellar Neutral Hydrogen in the Heliosphere: New Horizons Observations in the Context of Models
Autor:
Swaczyna, P., Bzowski, M., Dialynas, K., Dyke, L., Fraternale, F., Galli, A., Heerikhuisen, J., Kornbleuth, M. Z., Koutroumpa, D., Kowalska-Leszczyńska, I., Kubiak, M. A., Michael, A. T., Müller, H. -R., Opher, M., Rahmanifard, F.
Interstellar neutral (ISN) hydrogen is the most abundant species in the outer heliosheath and the very local interstellar medium (VLISM). Charge exchange collisions in the outer heliosheath result in filtration, reducing the ISN hydrogen density insi
Externí odkaz:
http://arxiv.org/abs/2406.09915
Autor:
Czyżnikiewicz, Mateusz, Bondaruk, Łukasz, Kubiak, Jakub, Wiącek, Adam, Degórski, Łukasz, Kubis, Marek, Skórzewski, Paweł
In this paper we study the impact of augmenting spoken language corpora with domain-specific synthetic samples for the purpose of training a speech recognition system. Using both a conventional neural TTS system and a zero-shot one with voice cloning
Externí odkaz:
http://arxiv.org/abs/2406.07090
In this paper we present S3R-Net, the Self-Supervised Shadow Removal Network. The two-branch WGAN model achieves self-supervision relying on the unify-and-adaptphenomenon - it unifies the style of the output data and infers its characteristics from a
Externí odkaz:
http://arxiv.org/abs/2404.12103
Enceladus is the Saturnian satellite known to have water vapor erupting from its south pole region called Tiger Stripes. Data collected by Cassini Ultraviolet Imaging Spectrograph during Enceladus transiting Saturn allow us to estimate water plume ab
Externí odkaz:
http://arxiv.org/abs/2403.15727
Autor:
Wojciechowski, L., Kubiak, K. J., Boncel, S., Marek, A., Gapinski, B., Runka, T., Jedrysiak, R., Ruczka, S., Blaszkiewicz, P., Mathia, T. G.
Publikováno v:
Tribology International, 2024, 191, 109203
Frictional losses are responsible for significant energy waste in many practical applications, and superlubricity with a coefficient of friction lower than 0.01 is the goal of tribologists. In this paper, metal-on-polymer contact was analysed and clo
Externí odkaz:
http://arxiv.org/abs/2403.08373
Direct-sampling observations of interstellar neutral gas, including hydrogen and deuterium, have been performed for more than one cycle of solar activity by IBEX. IBEX viewing is restricted to directions perpendicular to the spacecraft--Sun line, whi
Externí odkaz:
http://arxiv.org/abs/2402.09080
Direct observations of solar wind are mostly limited to the vicinity of the ecliptic plane. Retrieving the latitudinal structure of solar wind indirectly based on observations of the backscatter glow of interstellar neutral hydrogen is complex and re
Externí odkaz:
http://arxiv.org/abs/2402.08043