Zobrazeno 1 - 10
of 5 122
pro vyhledávání: '"Simon A.-C."'
Autor:
Yang, Tsung-Ching, Hashimoto, Tetsuya, Hsu, Tzu-Yin, Goto, Tomotsugu, Ling, Chih-Teng, Ho, Simon C. -C., Chen, Amos Y. -A., Kilerci, Ece
Measuring the Hubble constant (H$_0$) is one of the most important missions in astronomy. Nevertheless, recent studies exhibit differences between the employed methods. Fast radio bursts (FRBs) are coherent radio transients with large dispersion meas
Externí odkaz:
http://arxiv.org/abs/2411.02249
The wolensing Python package offers a solution for gravitational wave lensing computations within the full wave-optics regime. This tool is primarily designed to calculate the gravitational lensing amplification factor including diffractive effects,
Externí odkaz:
http://arxiv.org/abs/2410.19804
Autor:
Lin, Leah Ya-Ling, Hashimoto, Tetsuya, Goto, Tomotsugu, Raquel, Bjorn Jasper, Ho, Simon C. -C., Chen, Bo-Han, Kim, Seong Jin, Ling, Chih-Teng
Fast radio bursts (FRBs) are millisecond-duration radio waves from the Universe. Even though more than 50 physical models have been proposed, the origin and physical mechanism of FRB emissions are still unknown. The classification of FRBs is one of t
Externí odkaz:
http://arxiv.org/abs/2410.00576
Autor:
Amsler, Claude, Breuker, Horst, Bumbar, Marcus, Cerwenka, Matti, Costantini, Giovanni, Ferragut, Rafael, Fleck, Markus, Giammarchi, Marco, Gligorova, Angela, Gosta, Giulia, Hunter, Eric David, Killian, Carina, Kolbinger, Bernadette, Kraxberger, Viktoria, Kuroda, Naofumi, Lackner, Moritz, Leali, Marco, Maero, Giancarlo, Mascagna, Valerio, Matsuda, Yasuyuki, Migliorati, Stefano, Murtagh, Daniel James, Nanda, Amit, Nowak, Lilian, Rheinfrank, Simon, Romé, Massimiliano, Simon, Martin C., Tajima, Minori, Toso, Valerio, Ulmer, Stefan, van Beuzekom, Martin, Venturelli, Luca, Weiser, Alina, Widmann, Eberhard, Yamazaki, Yasunori, Zmeskal, Johann
The mechanism of antiproton-nucleus annihilation at rest is not fully understood, despite substantial previous experimental and theoretical work. In this study we used slow extracted antiprotons from the ASACUSA apparatus at CERN to measure the charg
Externí odkaz:
http://arxiv.org/abs/2407.06721
Autor:
Chien, Tom C. -C., Ling, Chih-Teng, Goto, Tomotsugu, Wu, Cossas K. -W., Kim, Seong Jin, Hashimoto, Tetsuya, Lin, Yu-Wei, Kilerci, Ece, Ho, Simon C. -C., Wang, Po-Ya, Raquel, Bjorn Jasper R.
The nature of the interaction between active galactic nuclei (AGNs) and their host galaxies remains an unsolved question. Therefore, conducting an AGN census is valuable to AGN research. Nevertheless, a significant fraction of AGNs are obscured by th
Externí odkaz:
http://arxiv.org/abs/2406.14888
Autor:
Nowak, Lilian, Malbrunot, Chloe, Simon, Martin C., Amsler, Claude, Cuendis, Sergio Arguedas, Lahs, Sebastian, Lanz, Andreas, Nanda, Amit, Wiesinger, Markus, Wolz, Tim, Widmann, Eberhard
Publikováno v:
Physics Letters B, Volume 858, 139012 (2024)
We present a Rabi-type measurement of two ground-state hydrogen hyperfine transitions performed in two opposite external magnetic field directions. This puts first constraints at the level of 2.3 10^-21 GeV on a set of coefficients of the Standard Mo
Externí odkaz:
http://arxiv.org/abs/2403.17763
Autor:
Amsler, C., Breuker, H., Bumbar, M., Chesnevskaya, S., Costantini, G., Ferragut, R., Giammarchi, M., Gligorova, A., Gosta, G., Higaki, H., Hori, M., Hunter, E. D., Killian, C., Kraxberger, V., Kuroda, N., Lanz, A., Leali, M., Maero, G., Malbrunot, C., Mascagna, V., Matsuda, Y., Maeckel, V., Migliorati, S., Murtagh, D. J., Nagata, Y., Nanda, A., Nowak, L., Rome, M., Simon, M. C., Tajima, M., Toso, V., Ulmer, S., Venturelli, L., Weiser, A., Widmann, E., Yamazaki, Y.
The Antiproton Decelerator (AD) at CERN provides antiproton bunches with a kinetic energy of 5.3 MeV. The Extra-Low ENergy Antiproton ring at CERN, commissioned at the AD in 2018, now supplies a bunch of electron-cooled antiprotons at a fixed energy
Externí odkaz:
http://arxiv.org/abs/2403.09268
Autor:
Ling, Chih-Teng, Goto, Tomotsugu, Kim, Seong Jin, Wu, Cossas K. -W., Hashimoto, Tetsuya, Chien, Tom C. -C., Lin, Yu-Wei, Ho, Simon C. -C., Kilerci, Ece
Mid-infrared (MIR) light from galaxies is sensitive to dust-obscured star-formation activities because it traces the characteristic emission of dust heated by young, massive stars. By constructing the MIR luminosity functions (LFs), we are able to qu
Externí odkaz:
http://arxiv.org/abs/2402.05386
Autor:
Lin, Yu-Wei, Wu, Cossas K. -W., Ling, Chih-Teng, Goto, Tomotsugu, Kim, Seong Jin, Kilerci, Ece, Hashimoto, Tetsuya, Wang, Po-Ya, Ho, Simon C. -C., Hsiao, Tiger Yu-Yang, Raquel, Bjorn Jasper R., Uno, Yuri
It has been an unanswered question how many dusty galaxies have been undetected from the state-of-the-art observational surveys. JWST enables us to detect faint IR galaxies that have prominent polycyclic aromatic hydrocarbon (PAH) features in the mid
Externí odkaz:
http://arxiv.org/abs/2401.01043
Autor:
Kim, Seong Jin, Goto, Tomotsugu, Ling, Chih-Teng, Wu, Cossas K. -W., Hashimoto, Tetsuya, Kilerci, Ece, Ho, Simon C. -C., Uno, Yuri, Wang, Po-Ya, Lin, Yu-Wei
With the advent of the James Webb Space Telescope (JWST), extra-galactic source count studies were conducted down to sub-microJy in the mid-infrared (MIR), which is several tens of times fainter than what the previous-generation infrared (IR) telesco
Externí odkaz:
http://arxiv.org/abs/2312.02090