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pro vyhledávání: '"Faure AS"'
H2CO is a ubiquitous molecule in the ISM and in the gas phase of prestellar cores, and is likely present in ice mantles, but its main desorption mechanism is unknown. In this paper our aim is to quantify the desorption efficiency of H2CO upon cosmic-
Externí odkaz:
http://arxiv.org/abs/2409.01700
Autor:
Faure, Gueter Josmy, Yeh, Jia-Fong, Chen, Min-Hung, Su, Hung-Ting, Hsu, Winston H., Lai, Shang-Hong
While existing research often treats long-form videos as extended short videos, we propose a novel approach that more accurately reflects human cognition. This paper introduces BREASE: BRidging Episodes And SEmantics for Long-Form Video Understanding
Externí odkaz:
http://arxiv.org/abs/2408.17443
Autor:
Monzac, Joséphine, Smartsev, Slava, Huijts, Julius, Rovige, Lucas, Andriyash, Igor A., Vernier, Aline, Tomkus, Vidmantas, Girdauskas, Valdas, Raciukaitis, Gediminas, Mackevičiūtė, Miglė, Stankevic, Valdemar, Cavagna, Antoine, Kaur, Jaismeen, Kalouguine, André, Lopez-Martens, Rodrigo, Faure, Jérôme
We present significant advances in Laser Wakefield Acceleration (LWFA) operating at a 1 kHz repetition rate, employing a sub-TW, few-femtosecond laser and a continuously flowing hydrogen gas target. We conducted the first comprehensive study assessin
Externí odkaz:
http://arxiv.org/abs/2406.17426
Autor:
Belcaid, Mohammed, Bonnafous, Eric, Crison, Louis, Faure, Christophe, Jenn, Eric, Pagetti, Claire
Publikováno v:
12th European Congress on Embedded Real Time Software and Systems, Jun 2024, Toulouse, France
In this paper, we present a development process of a drone detection system involving a machine learning object detection component. The purpose is to reach acceptable performance objectives and provide sufficient evidences, required by the recommend
Externí odkaz:
http://arxiv.org/abs/2406.12362
Autor:
Motapon, O., Pop, N., Argoubi, F., Mezei, J. Zs., Epée, M. D. Epée, Faure, A., Telmini, M., Tennyson, J., Schneider, I. F.
Publikováno v:
Physical Review A 90, 012706 (2014)
A series of Multichannel Quantum Defect Theory-based computations have been performed, in order to produce the cross sections of rotational transitions (excitations $N_{i}^{+}-2 \rightarrow$ $N_{i}^{+}$, de-excitations $N_{i}^{+}$ $\rightarrow$ $N_{i
Externí odkaz:
http://arxiv.org/abs/2405.06504
Autor:
Chakrabarti, K., Mezei, J. Zs, Motapon, O., Faure, A., Dulieu, O., Hassouni, K., Schneider, I. F.
Publikováno v:
J. Phys. B: At. Mol. Opt. Phys. 51 (2018) 104002 (8pp)
The reactive collisions of the CH$^+$ molecular ion with electrons is studied in the framework of the multichannel quantum defect theory, taking into account the contribution of the core-excited Rydberg states. In addition to the $X^1\Sigma^+$ ground
Externí odkaz:
http://arxiv.org/abs/2404.19302
Autor:
Xue, Ci, Remijan, Anthony, Faure, Alexandre, Momjian, Emmanuel, Hunter, Todd R., Loomis, Ryan A., Herbst, Eric, McGuire, Brett
At centimeter wavelengths, single-dish observations have suggested that the Sagittarius (Sgr) B2 molecular cloud at the Galactic Center hosts weak maser emission from several organic molecules, including CH$_2$NH, HNCNH, and HCOOCH$_3$. However, the
Externí odkaz:
http://arxiv.org/abs/2404.12622
Autor:
Faure, Q., Toschi, A., Soh, J. R., Lhotel, E., Detlefs, B., Prabhakaran, D., McMorrow, D. F., Sahle, C. J.
We report a resonant inelastic X-ray scattering study on a single crystal of a non-stoichiometric pyrochlore iridate Tb$_{2+x}$Ir$_{2-x}$O$_{7-y}$ ($x \simeq 0.25$) that magnetically orders at $T_{\rm{N}}\simeq 50$ K. We find that the strength of the
Externí odkaz:
http://arxiv.org/abs/2404.03829
The hydrogen and water molecules respond very differently to the collisional-radiative processes taking place in planetary atmospheres. Naturally, the question arises whether H2O-rich atmospheres are more (or less) resilient to long-term mass loss th
Externí odkaz:
http://arxiv.org/abs/2404.02604
Autor:
Tanious, M., Gal, R. Le, Neri, R., Faure, A., Gupta, A., Law, C. J., Huang, J., Cuello, N., Williams, J. P., Ménard, F.
Publikováno v:
A&A 687, A92 (2024)
Over the past few years, chemical studies have revealed multiple structures in the vicinity of young stellar objects (YSOs). It has become evident that specific physical conditions are associated with the emission of particular molecular lines, allow
Externí odkaz:
http://arxiv.org/abs/2403.18905