Zobrazeno 1 - 10
of 532
pro vyhledávání: '"S M Jia"'
Autor:
D. A. Kann, S. Agayeva, V. Aivazyan, S. Alishov, C. M. Andrade, S. Antier, A. Baransky, P. Bendjoya, Z. Benkhaldoun, S. Beradze, D. Berezin, M. Boër, E. Broens, S. Brunier, M. Bulla, O. Burkhonov, E. Burns, Y. Chen, Y. P. Chen, M. Conti, M. W. Coughlin, W. W. Cui, F. Daigne, B. Delaveau, H. A. R. Devillepoix, T. Dietrich, D. Dornic, F. Dubois, J.-G. Ducoin, E. Durand, P.-A. Duverne, H.-B. Eggenstein, S. Ehgamberdiev, A. Fouad, M. Freeberg, D. Froebrich, M. Y. Ge, S. Gervasoni, V. Godunova, P. Gokuldass, E. Gurbanov, D. W. Han, E. Hasanov, P. Hello, T. Hussenot-Desenonges, R. Inasaridze, A. Iskandar, N. Ismailov, A. Janati, T. Jegou du Laz, S. M. Jia, S. Karpov, A. Kaeouach, R. W. Kiendrebeogo, A. Klotz, R. Kneip, N. Kochiashvili, N. Kunert, A. Lekic, S. Leonini, C. K. Li, W. Li, X. B. Li, J. Y. Liao, L. Logie, F. J. Lu, J. Mao, D. Marchais, R. Ménard, D. Morris, R. Natsvlishvili, V. Nedora, K. Noonan, K. Noysena, N. B. Orange, P. T. H. Pang, H. W. Peng, C. Pellouin, J. Peloton, T. Pradier, O. Pyshna, Y. Rajabov, S. Rau, C. Rinner, J.-P. Rivet, F. D. Romanov, P. Rosi, V. A. Rupchandani, M. Serrau, A. Shokry, A. Simon, K. Smith, O. Sokoliuk, M. Soliman, L. M. Song, A. Takey, Y. Tillayev, L. M. Tinjaca Ramirez, I. Tosta e Melo, D. Turpin, A. de Ugarte Postigo, S. Vanaverbeke, V. Vasylenko, D. Vernet, Z. Vidadi, C. Wang, J. Wang, L. T. Wang, X. F. Wang, S. L. Xiong, Y. P. Xu, W. C. Xue, X. Zeng, S. N. Zhang, H. S. Zhao, X. F. Zhao
Publikováno v:
The Astrophysical Journal Letters, Vol 948, Iss 2, p L12 (2023)
Object GRB 221009A is the brightest gamma-ray burst (GRB) detected in more than 50 yr of study. In this paper, we present observations in the X-ray and optical domains obtained by the GRANDMA Collaboration and the Insight Collaboration. We study the
Externí odkaz:
https://doaj.org/article/5ebca5e7256647c995f697755b6c737d
Autor:
X. Ma, L. Zhang, L. Tao, Q. C. Bu, J. L. Qu, S. N. Zhang, D. K. Zhou, Y. Huang, S. M. Jia, L. M. Song, S. Zhang, M. Y. Ge, H. X. Liu, Z. X. Yang, W. Yu, E. S. Yorgancioglu
Publikováno v:
The Astrophysical Journal, Vol 948, Iss 2, p 116 (2023)
We report the X-ray timing results of the black hole candidate MAXI J1820+070 during its 2018 outburst using the Hard X-ray Modulation Telescope (Insight-HXMT) and Neutron Star Interior Composition Explorer Mission (NICER) observations. Low-frequency
Externí odkaz:
https://doaj.org/article/47256c6a157e4f089c82153405ce662c
Publikováno v:
Metalurgija, Vol 60, Iss 3-4, Pp 195-197 (2021)
According to the production practice of 14 tons flat ingot, the influence of heat preservation measures on solidification state of ingot head is analyzed by the software ProCAST. The results show that the heating riser and electromagnetic heating ris
Externí odkaz:
https://doaj.org/article/1a1f053b38614b6c94502ea2383fb857
Autor:
S M Jia, J L Qu, F J Lu, L Zhang, S N Zhang, L M Song, S Zhang, Y Huang, X Ma, L Tao, H X Liu, W Yu
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:4792-4800
We present a detailed spectral-timing analysis of the normal branch oscillations (NBOs) observed in two Z sources, Cyg X−2 and Sco X−1, using the data of the Neutron star Interior Composition Explorer (NICER). This is the first study of the NBO p
Publikováno v:
Journal of Management Information Systems. 2024, Vol. 41 Issue 1, pi-i. 1p.
Autor:
Zi-Xu Yang, Liang Zhang, S N Zhang, M Méndez, Federico García, Yue Huang, Qingcui Bu, He-Xin Liu, Wei Yu, P J Wang, L Tao, D Altamirano, Jin-Lu Qu, S Zhang, X Ma, L M Song, S M Jia, M Y Ge, Q Z Liu, J Z Yan, T M Li, X Q Ren, R C Ma, Yuexin Zhang, Y C Xu, B Y Ma, Y F Du, Y C Fu, Y X Xiao, P P Li, P Jin, S J Zhao, Q C Zhao
Fast transitions between different types of power density spectra (PDS) happening over time-scales of several tens of seconds are rare phenomena in black hole X-ray binaries. In this paper, we report a broad-band spectral-timing analysis of the fast
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::85ef3e4956e94644ea6f1d3337b83944
http://arxiv.org/abs/2303.07588
http://arxiv.org/abs/2303.07588
Autor:
P J Wang, L D Kong, Y P Chen, S Zhang, S N Zhang, R Soria, L Ji, J L Qu, Y Huang, L Tao, M Y Ge, F J Lu, L Chen, T P Li, Y P Xu, X L Cao, Y Chen, C Z Liu, Q C Bu, C Cai, Z Chang, T X Chen, Y B Chen, W W Cui, Y Y Du, G H Gao, H Gao, Y D Gu, J Guan, C C Guo, D W Han, J Huo, S M Jia, W C Jiang, J Jin, B Li, C K Li, G Li, W Li, X Li, X B Li, X F Li, Z W Li, X H Liang, J Y Liao, B S Liu, H X Liu, H W Liu, X J Liu, X F Lu, Q Luo, T Luo, R C Ma, X Ma, B Meng, Y Nang, J Y Nie, G Ou, X Q Ren, N Sai, L M Song, X Y Song, L Sun, Y Tan, Y L Tuo, C Wang, L J Wang, W S Wang, Y S Wang, X Y Wen, B Y Wu, B B Wu, M Wu, G C Xiao, S Xiao, S L Xiong, R J Yang, S Yang, Yan Ji Yang, Yi Jung Yang, Q B Yi, Q Q Yin, Y You, F Zhang, H M Zhang, J Zhang, P Zhang, W C Zhang, W Zhang, Y F Zhang, Y H Zhang, H S Zhao, X F Zhao, S J Zheng, Y G Zheng, D K Zhou
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 512:4541-4555
We studied the 2018 outburst of the black hole transient H 1743 − 322 with a series of Insight-HXMT, NICER, and NuSTAR observations, covering the 1–120 keV band. With our broad-band X-ray spectral modelling, we confirm that the source remained in
Autor:
A. E. Camisasca, C. Guidorzi, L. Amati, F. Frontera, X. Y. Song, S. Xiao, S. L. Xiong, S. N. Zhang, R. Margutti, S. Kobayashi, C. G. Mundell, M. Y. Ge, A. Gomboc, S. M. Jia, N. Jordana-Mitjans, C. K. Li, X. B. Li, R. Maccary, M. Shrestha, W. C. Xue, S. Zhang
The dissipation process of GRB prompt emission is still unknown. Study of temporal variability may provide a unique way to discriminate the imprint of the inner engine activity from geometry and propagation related effects. We define the minimum vari
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6b79e6ee4f47945857d2773935a4be2c
Autor:
R C Ma, R Soria, L Tao, W Zhang, J L Qu, S N Zhang, L Zhang, E L Qiao, S J Zhao, M Y Ge, X B Li, Y Huang, L M Song, S Zhang, Q C Bu, Y N Wang, X Ma, S M Jia
We studied the transient Galactic black hole candidate MAXI J0637−430 with data from Insight-HXMT, Swift, and XMM–Newton. The broad-band X-ray observations from Insight-HXMT help us constrain the power-law component. MAXI J0637–430 is located a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a40129654699bb443deea6fe9b91bef5
http://arxiv.org/abs/2206.03409
http://arxiv.org/abs/2206.03409
Autor:
Zi-Xu Yang, Liang Zhang, Qing-Cui Bu, Yue Huang, He-Xin Liu, Wei Yu, P. J. Wang, L. Tao, J. L. Qu, S. Zhang, S. N. Zhang, X. Ma, L. M. Song, S. M. Jia, M. Y. Ge, Q. Z. Liu, J. Z. Yan, D. K. Zhou, T. M. Li, B. Y. Wu, X. Q. Ren, R. C. Ma, Y. X. Zhang, Y. C. Xu, B. Y. Ma, Y. F. Du, Y. C. Fu, Y. X. Xiao
Publikováno v:
Astrophysical Journal, 932(1):7. IOP PUBLISHING LTD
Here we present a detailed study of the broadband noise in the power density spectra of the black hole X-ray binary MAXI J1820+070 during the hard state of its 2018 outburst, using Hard X-ray Modulation Telescope observations. The broadband noise sho