Zobrazeno 1 - 10
of 4 396
pro vyhledávání: '"Sokolowski P"'
With the low Earth orbit environment becoming increasingly populated with artificial satellites, rockets, and debris, it is important to understand the effects they have on radio astronomy. In this work, we undertake a multi-frequency, multi-epoch su
Externí odkaz:
http://arxiv.org/abs/2412.14483
Autor:
Rox, Hannes, Ränke, Fabian, Mädler, Jonathan, Marzec, Mateusz M., Sokolowski, Krystian, Baumann, Robert, Hamedi, Homa, Yang, Xuegeng, Mutschke, Gerd, Urbas, Leon, Lasagni, Andrés Fabián, Eckert, Kerstin
Laser-structuring techniques like Direct Laser Interference Patterning show great potential for optimizing electrodes for water electrolysis. Therefore, a systematic experimental study based on statistical design of experiments is performed to analyz
Externí odkaz:
http://arxiv.org/abs/2411.03373
The Vela pulsar (J0835-4510) is known to exhibit variations in Faraday rotation and dispersion on multi-decade timescales due to the changing sightline through the surrounding Vela supernova remnant and the Gum Nebula. Until now, variations in Farada
Externí odkaz:
http://arxiv.org/abs/2411.00602
Autor:
Palai, Swaroop Kumar, Dyksik, Mateusz, Sokolowski, Nikodem, Ciorga, Mariusz, Viso, Estrella Sánchez, Xie, Yong, Schubert, Alina, Taniguchi, Takashi, Watanabe, Kenji, Maude, Duncan K., Surrente, Alessandro, Baranowski, Michał, Castellanos-Gomez, Andres, Munuera, Carmen, Plochocka, Paulina
Stacking monolayers of transition metal dichalcogenides (TMDs) has led to the discovery of a plethora of new exotic phenomena, resulting from moir\'e pattern formation. Due to the atomic thickness and high surface-to-volume ratio of heterostructures,
Externí odkaz:
http://arxiv.org/abs/2410.12472
Autor:
Chekan, Vera, Geniet, Colin, Hatzel, Meike, Pilipczuk, Michał, Sokołowski, Marek, Seweryn, Michał T., Witkowski, Marcin
For a group $\Gamma$, a $\Gamma$-labelled graph is an undirected graph $G$ where every orientation of an edge is assigned an element of $\Gamma$ so that opposite orientations of the same edge are assigned inverse elements. A path in $G$ is non-null i
Externí odkaz:
http://arxiv.org/abs/2408.16344
Publikováno v:
Publ. Astron. Soc. Aust. 41 (2024) e045
Traditional pulsar surveys have primarily employed time-domain periodicity searches. However, these methods are susceptible to effects like scattering, eclipses and orbital motion. At lower radio frequencies (<= 300 MHz), factors such as dispersion m
Externí odkaz:
http://arxiv.org/abs/2407.13282
Autor:
Sun, Yanwen, Chen, Chaobo, Albert, Thies J., Li, Haoyuan, Arefev, Mikhail I., Chen, Ying, Dunne, Mike, Glownia, James M., Hoffmann, Matthias, Hurley, Matthew J., Mo, Mianzhen, Nguyen, Quynh L., Sato, Takahiro, Song, Sanghoon, Sun, Peihao, Sutton, Mark, Teitelbaum, Samuel, Valavanis, Antonios S., Wang, Nan, Zhu, Diling, Zhigilei, Leonid V., Sokolowski-Tinten, Klaus
Femtosecond laser ablation is a process that bears both fundamental physics interest and has wide industrial applications. For decades, the lack of probes on the relevant time and length scales has prevented access to the highly nonequilibrium phase
Externí odkaz:
http://arxiv.org/abs/2407.10505
Model parameter inference is a universal problem across science. This challenge is particularly pronounced in developmental biology, where faithful mechanistic descriptions require spatial-stochastic models with numerous parameters, yet quantitative
Externí odkaz:
http://arxiv.org/abs/2407.10938
Autor:
Sokolowski, M., Aniruddha, G., Di Pietrantonio, C., Harris, C., Price, D. C., McSweeney, S., Wayth, R. B., Bhat, N. D. R.
Fast Radio Bursts (FRBs) are millisecond dispersed radio pulses of predominately extra-galactic origin. Although originally discovered at GHz frequencies, most FRBs have been detected between 400 to 800 MHz. Nevertheless, only a handful of FRBs were
Externí odkaz:
http://arxiv.org/abs/2405.13478
Autor:
Luo, R., Ekers, R. D., Hobbs, G., Dunning, A., James, C. W., Lower, M. E., Gupta, V., Zic, A., Sokolowski, M., Phillips, C., Deller, A. T., Staveley-Smith, L.
Fast Radio Bursts (FRBs) are short-duration radio transients that occur at random times in host galaxies distributed all over the sky. Large field of view instruments can play a critical role in the blind search for rare FRBs. We present a concept fo
Externí odkaz:
http://arxiv.org/abs/2405.07439