Zobrazeno 1 - 10
of 1 134
pro vyhledávání: '"Gawroński, P."'
Autor:
Hewitt, Danté M., Bhardwaj, Mohit, Gordon, Alexa C., Kirichenko, Aida, Nimmo, Kenzie, Bhandari, Shivani, Cognard, Ismaël, Fong, Wen-fai, de Paz, Armando Gil, Gopinath, Akshatha, Hessels, Jason W. T., Kirsten, Franz, Marcote, Benito, Bezrukovs, Vladislavs, Blaauw, Richard, Bray, Justin D., Buttaccio, Salvatore, Cassanelli, Tomas, Chawla, Pragya, Corongiu, Alessandro, Deng, William, Didehbani, Hannah N., Dong, Yuxin, Gawroński, Marcin P., Giroletti, Marcello, Guillemot, Lucas, Huang, Jeff, Joseph, Ronniy C., Kaspi, Victoria M., Lazda, Mattias, Lindqvist, Michael, Giuseppe, Maccaferri, Mas-Ribas, Lluis, Masui, Kiyoshi W., Mckinven, Ryan, Michilli, Daniele, Nugent, Anya E., Ould-Boukattine, Omar S., Paragi, Zsolt, Pearlman, Aaron B., Pen, Ue-Li, Pleunis, Ziggy, Sand, Ketan R., Shah, Vishwangi, Shin, Kaitlyn, Snelders, Mark P., Venturi, Tiziana, Wang, Na, Williams-Baldwin, David R. A., Yang, Jun, Yuan, Jianping P.
We present the localization and host galaxy of FRB 20190208A, a repeating source of fast radio bursts (FRBs) discovered using CHIME/FRB. As part of the PRECISE repeater localization program on the EVN, we monitored FRB 20190208A for 65.6 hours at $\s
Externí odkaz:
http://arxiv.org/abs/2410.17044
Autor:
Ould-Boukattine, O. S., Chawla, P., Hessels, J. W. T., Cooper, A. J., Gawroński, M. P., Herrmann, W., Kirsten, F., Hewitt, D. M., Konijn, D. C., Nimmo, K., Pleunis, Z., Puchalska, W., Snelders, M. P.
Fast radio bursts (FRBs) are sufficiently energetic to be detectable from luminosity distances up to at least seven billion parsecs (redshift $z > 1$). Probing the maximum energies and luminosities of FRBs constrains their emission mechanism and cosm
Externí odkaz:
http://arxiv.org/abs/2410.17024
Publikováno v:
Journal of Experimental Social Psychology, 114, Article 104632 (2024)
An analysis drawing on Signal Detection Theory suggests that people may fall for misinformation because they are unable to discern true from false information (truth insensitivity) or because they tend to accept information with a particular slant re
Externí odkaz:
http://arxiv.org/abs/2406.01621
Autor:
Ibrahim, A. Y., Borghese, A., Zelati, F. Coti, Parent, E., Marino, A., Ould-Boukattine, O. S., Rea, N., Ascenzi, S., Pacholski, D. P., Mereghetti, S., Israel, G. L., Tiengo, A., Possenti, A., Burgay, M., Turolla, R., Zane, S., Esposito, P., Gotz, D., Campana, S., Kirsten, F., Gawronski, M. P., Hessels, J. W. T.
Recently, the Galactic magnetar SGR J1935+2154 has garnered attention due to its emission of an extremely luminous radio burst, reminiscent of Fast Radio Bursts (FRBs). SGR J1935+2154 is one of the most active magnetars, displaying flaring events nea
Externí odkaz:
http://arxiv.org/abs/2402.08596
Autor:
Hewitt, Danté M., Bhandari, Shivani, Marcote, Benito, Hessels, Jason W. T., Nimmo, Kenzie, Kirsten, Franz, Bach, Uwe, Bezrukovs, Vladislavs, Bhardwaj, Mohit, Blaauw, Richard, Bray, Justin D., Buttaccio, Salvatore, Corongiu, Alessandro, Gawroński, Marcin P., Giroletti, Marcello, Keimpema, Aard, Maccaferri, Giuseppe M., Paragi, Zsolt, Trudu, Matteo, Snelders, Mark P., Venturi, Tiziana, Wang, Na, Williams-Baldwin, David R. A., Wrigley, Nicholas H., Yang, Jun, Yuan, Jianping P.
We present very-long-baseline interferometry (VLBI) observations of the hyperactive repeating FRB 20220912A using the European VLBI Network (EVN) with an EVN-Lite setup. We detected 150 bursts from FRB 20220912A over two observing epochs in October 2
Externí odkaz:
http://arxiv.org/abs/2312.14490
Autor:
Kirsten, F., Ould-Boukattine, O., Herrmann, W., Gawronski, M., Hessels, J., Lu, W., Snelders, M., Chawla, P., Yang, J., Blaauw, R., Nimmo, K., Puchalska, W., Wolak, P., van Ruiten, R.
Fast radio bursts (FRBs) are extremely energetic, millisecond-duration radio flashes that reach Earth from extragalactic distances. Broadly speaking, FRBs can be classified as repeating or (apparently) non-repeating. It is still unclear, however, whe
Externí odkaz:
http://arxiv.org/abs/2306.15505
Autor:
Le, N., Karska, A., Figueira, M., Sewiło, M., Mirocha, A., Fischer, Ch., Kaźmierczak-Barthel, M., Klein, R., Gawroński, M., Koprowski, M., Kowalczyk, K., Fischer, W. J., Menten, K. M., Wyrowski, F., König, C., Kristensen, L. E.
Publikováno v:
A&A 674, A64 (2023)
(abridged) Far-infrared (FIR) line emission provides key information about the gas cooling and heating due to shocks and UV radiation associated with the early stages of star formation. Gas cooling via FIR lines might, however, depend on metallicity.
Externí odkaz:
http://arxiv.org/abs/2304.08127
Autor:
Nimmo, K., Hessels, J. W. T., Snelders, M. P., Karuppusamy, R., Hewitt, D. M., Kirsten, F., Marcote, B., Bach, U., Bansod, A., Barr, E. D., Behrend, J., Bezrukovs, V., Buttaccio, S., Feiler, R., Gawroński, M. P., Lindqvist, M., Orbidans, A., Puchalska, W., Wang, N., Winchen, T., Wolak, P., Wu, J., Yuan, J.
The repeating fast radio burst (FRB) source FRB 20200120E is exceptional because of its proximity and association with a globular cluster. Here we report $60$ bursts detected with the Effelsberg telescope at 1.4 GHz. We observe large variations in th
Externí odkaz:
http://arxiv.org/abs/2206.03759
The system of two resources $R_1$, $R_2$ and one consumer $C$ is investigated within the Rosenzweig-MacArthur model with Holling type II functional response. The rates $\beta_i$ of consumption of resources $i=1,2$ are coupled by the condition $\beta_
Externí odkaz:
http://arxiv.org/abs/2205.11910
Autor:
Karska, Agata, Koprowski, Maciej, Solarz, Aleksandra, Szczerba, Ryszard, Sewiło, Marta, Siódmiak, Natasza, Elia, Davide, Gawroński, Marcin, Grzesiak, Konrad, Yung, Bosco H. K., Fischer, William J., Kristensen, Lars E.
Publikováno v:
A&A 663, A133 (2022)
(abridged) Star formation in the outer Galaxy, i.e., outside of the Solar circle, has been lightly studied in part due to low CO brightness of molecular clouds linked with the negative metallicity gradient. Recent infrared surveys provide an overview
Externí odkaz:
http://arxiv.org/abs/2204.11687