Zobrazeno 1 - 10
of 360
pro vyhledávání: '"Ge, M. -Y."'
Autor:
Li, P. P., Tao, L., Ma, R. C., Ge, M. Y., Zhao, Q. C., Zhao, S. J., Zhang, L., Bu, Q. C., Kong, L. D., Tuo, Y. L., Ji, L., Zhang, S., Qu, J. L., Zhang, S. N., Huang, Y., Ma, X., Ye, W. T., Shui, Q. C.
We present a comprehensive timing analysis on the Be/X-ray binary pulsar RX J0440.9+4431 using observations from \textit{NICER} and \textit{Insight}-HXMT during the 2022--2023 outburst. The power density spectrum (PDS) of RX J0440.9+4431 exhibits typ
Externí odkaz:
http://arxiv.org/abs/2402.14226
Autor:
Xiao, Y. X., Xu, Y. J., Ge, M. Y., Lu, F. J., Zhang, S. N., Zhang, S., Tao, L., Qu, J. L., Wang, P. J., Kong, L. D., Tuo, Y. L., You, Y., Zhao, S. J., Peng, J. Q., Du, Y. F., Zhang, Y. H., Ye, W. T.
We report the phase-resolved spectral results of the first Galactic Pulsating Ultra-Luminous X-ray source (PULX) Swift J0243.6+6124, modeling at its 2017-2018 outburst peak using data collected by the Hard X-ray Modulation Telescope (Insight-HXMT). T
Externí odkaz:
http://arxiv.org/abs/2401.15992
Autor:
Zhao, S. J., Tao, L., Li, P. P., Soria, R., Feng, H., Zhang, Y. X., Ma, R. C., Zhang, W. D., Qiao, E. L., Yin, Q. Q., Zhang, S. N., Zhang, L., Bu, Q. C., Ma, X., Huang, Y., Ge, M. Y., Li, X. B., Zhao, Q. C., Peng, J. Q., Xiao, Y. X.
Publikováno v:
A&A 685, A42 (2024)
The black hole X-ray binary source 4U 1543--47 experienced a super-Eddington outburst in 2021, reaching a peak flux of up to $\sim1.96\times10^{-7}\rm erg\ \rm cm^{-2}\ \rm s^{-1}$ ($\sim 8.2$ Crab) in the 2--10\,keV band. Soon after the outburst beg
Externí odkaz:
http://arxiv.org/abs/2312.09632
Autor:
Liu, P., Yuan, J. -P., Ge, M. -Y., Ye, W. -T., Zhou, S. -Q., Dang, S. -J., Zhou, Z. -R., Gügercinoğlu, E., Wang, W. -H., Wang, P., Li, A., Li, D., Wang, N.
PSR J1048$-$5832 (B1046$-$58) is a Vela-like pulsar that has exhibited multiple glitch events. In this study, we analyze the timing data spanning nearly 16 years, acquired from both the Fermi Gamma-ray Space Telescope and the Parkes 64 m radio telesc
Externí odkaz:
http://arxiv.org/abs/2312.04305
Autor:
Li, P. P., Tao, L., Tuo, Y. L., Ge, M. Y., Kong, L. D., Zhang, L., Bu, Q. C., Ji, L., Qu, J. L., Zhang, S., Zhang, S. N., Huang, Y., Ma, X., Ye, W. T., Zhao, Q. C., Ma, R. C., Zhao, S. J., Hou, X., Yang, Z. X., Wang, P. J., Jia, S. M., Shui, Q. C., Guan, J.
RX J0440.9+4431, a Be/X-ray binary, had its brightest outburst in 2022 since its discovery, with a peak X-ray flux of 2.25 Crab (as recorded by Swift/BAT, 15-50 keV). We analyze the timing properties of this giant outburst using data from Insight-HXM
Externí odkaz:
http://arxiv.org/abs/2309.14858
Autor:
Zhang, P., Soria, R., Zhang, S., Ji, L., Kong, L. D., Chen, Y. P., Zhang, S. N., Chang, Z., Ge, M. Y., Li, J., Liu, G. C., Liu, Q. Z., Ma, X., Peng, J. Q., Qu, J. L., Shui, Q. C., Tao, L., Tian, H. J., Wang, P. J., Yan, J. Z., Zeng, X. Y.
Publikováno v:
A&A 677, A178 (2023)
We investigate the dynamical properties of low frequency quasi-periodic oscillations (QPOs) observed from the black hole X-ray binary MAXI J1820+070 during the early part of its 2018 outburst, when the system was in a bright hard state. To this aim,
Externí odkaz:
http://arxiv.org/abs/2307.07709
Autor:
Yang, Zi-Xu, Zhang, Liang, Zhang, S. N., Méndez, M., García, Federico, Huang, Yue, Bu, Qingcui, Liu, He-Xin, Yu, Wei, Wang, P. J., Tao, L., Altamirano, D., Qu, Jin-Lu, Zhang, S., Ma, X., Song, L. M., Jia, S. M., Ge, M. Y., Liu, Q. Z., Yan, J. Z., Li, T. M., Ren, X. Q., Ma, R. C., Zhang, Yuexin, Xu, Y. C., Ma, B. Y., Du, Y. F., Fu, Y. C., Xiao, Y. X., Li, P. P, Jin, P., Zhao, S. J., Zhao, Q. C.
Fast transitions between different types of power density spectra (PDS) happening over timescales of several tens of seconds are rare phenomena in black hole X-ray binaries. In this paper, we report a broadband spectral-timing analysis of the fast tr
Externí odkaz:
http://arxiv.org/abs/2303.07588
Autor:
Ma, X., Zhang, L., Tao, L., Bu, Q. C., Qu, J. L., Zhang, S. N., Zhou, D. K., Huang, Y., Jia, S. M., Song, L. M., Zhang, S., Ge, M. Y., Liu, H. X., Yang, Z. X., Yu, W., Yorgancioglu, E. S.
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:
http://arxiv.org/abs/2303.00481
Autor:
Kann, D. A., Agayeva, S., Aivazyan, V., Alishov, S., Andrade, C. M., Antier, S., Baransky, A., Bendjoya, P., Benkhaldoun, Z., Beradze, S., Berezin, D., Boër, M., Broens, E., Brunier, S., Bulla, M., Burkhonov, O., Burns, E., Chen, Y., Chen, Y. P., Conti, M., Coughlin, M. W., Cui, W. W., Daigne, F., Delaveau, B., Devillepoix, H. A. R., Dietrich, T., Dornic, D., Dubois, F., Ducoin, J. -G., Durand, E., Duverne, P. -A., Eggenstein, H. -B., Ehgamberdiev, S., Fouad, A., Freeberg, M., Froebrich, D., Ge, M. Y., Gervasoni, S., Godunova, V., Gokuldass, P., Gurbanov, E., Han, D. W., Hasanov, E., Hello, P., Hussenot-Desenonges, T., Inasaridze, R., Iskandar, A., Ismailov, N., Janati, A., Laz, T. Jegou du, Jia, S. M., Karpov, S., Kaeouach, A., Kiendrebeogo, R. W., Klotz, A., Kneip, R., Kochiashvili, N., Kunert, N., Lekic, A., Leonini, S., Li, C. K., Li, W., Li, X. B., Liao, J. Y., Logie, L., Lu, F. J., Mao, J., Marchais, D., Ménard, R., Morris, D., Natsvlishvili, R., Nedora, V., Noonan, K., Noysena, K., Orange, N. B., Pang, P. T. H., Peng, H. W., Pellouin, C., Peloton, J., Pradier, T., Pyshna, O., Rajabo, Y., Rau, S., Rinner, C., Rivet, J. -P., Romanov, F. D., Rosi, P., Rupchandani, V. A., Serrau, M., Shokry, A., Simon, A., Smith, K., Sokoliuk, O., Soliman, M., Song, L. M., Takey, A., Tillayev, Y., Ramirez, L. M. Tinjaca, Melo, I. Tosta e, Turpin, D., Postigo, A. de Ugarte, Vanaverbeke, S., Vasylenko, V., Vernet, D., Vidadi, Z., Wang, C., Wang, J., Wang, L. T., Wang, X. F., Xiong, Shaolin L., Xu, Y. P., Xue, W. C., Zeng, X., Zhang, S. N., Zhao, H. S., Zhao, X. F.
GRB 221009A is the brightest Gamma-Ray Burst (GRB) detected in more than 50 years of study. In this paper, we present observations in the X-ray and optical domains after the GRB obtained by the GRANDMA Collaboration (which includes observations from
Externí odkaz:
http://arxiv.org/abs/2302.06225
Autor:
Fu, Yu-Cong, Song, L. M., Ding, G. Q., Ge, M. Y., Tuo, Y. L., Zhang, S., Zhang, S. N., Hou, X., Qu, J. L., Zhang, J., Zhang, L., Bu, Q. C., Huang, Y., Ma, X., Zhou, X., Yan, W. M., Yang, Z. X., Lu, X. F., Li, T. M., Xu, Y. C., Wang, P. J., Xiao, S. H., Liu, H. X., Ren, X. Q., Du, Y. F., zhao, Q. X., Xiao, Y. X.
We report the evolution of the X-ray pulsations of EXO 2030+375 during its 2021 outburst using the observations from \textit{Insight}-HXMT. Based on the accretion torque model, we study the correlation between the spin frequency derivatives and the l
Externí odkaz:
http://arxiv.org/abs/2302.02167