Zobrazeno 1 - 10
of 39
pro vyhledávání: '"Liming Rui"'
Autor:
Danfeng Xiang, Xiaofeng Wang, Xinghan Zhang, Hanna Sai, Jujia Zhang, Thomas G Brink, Alexei V Filippenko, Jun Mo, Tianmeng Zhang, Zhihao Chen, Luc Dessart, Zhitong Li, Shengyu Yan, Sergei I Blinnikov, Liming Rui, E Baron, J M DerKacy
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 520:2965-2982
We present extensive optical/ultraviolet observations and modelling analysis for the nearby SN 1987A-like peculiar Type II supernova (SN) 2018hna. Both photometry and spectroscopy covered phases extending to $>$500 days after the explosion, making it
Autor:
Xulin Zhao, Melissa L. Graham, H. Yuk, WeiKang Zheng, Weili Lin, F. Huang, Hanna Sai, Jun Mo, Alexei V. Filippenko, Peter J. Brown, Han Lin, T. G. Brink, Liming Rui, Jujia Zhang, Danfeng Xiang, Yongzhi Cai, Tianmeng Zhang, Xinghan Zhang, Goni Halevi, Xue Li, Xiaofeng Wang, Isaac Shivvers
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 505:4890-4905
We present optical and ultraviolet photometry, as well as optical spectra, for the type II supernova (SN) 2015bf. Our observations cover the phases from ∼2 to ∼200 d after explosion. The first spectrum is characterized by a blue continuum with a
Autor:
Lingzhi Wang, Liming Rui, Danfeng Xiang, Hua Feng, Hanna Sai, Jicheng Zhang, Weili Lin, Wenxiong Li, Yong Zhao, D. O. Mirzaqulov, Shuhrat A. Ehgamberdiev, Tianrui Sun, Jujia Zhang, Han Lin, Xulin Zhao, Jie Lin, Xinghan Zhang, Xue Li, Tianmeng Zhang, Chengyuan Wu, Jun Mo, Jianfeng Wu, Xiaofeng Wang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 504:4226-4241
MAXI J1820+070 is a low-mass black hole X-ray binary system with high luminosity in both optical and X-ray bands during the outburst periods. We present extensive photometry in X-ray, ultraviolet, and optical bands, as well as densely-cadenced optica
Autor:
Jun Mo, T. Zhang, A. Pastorello, G. C. Anupama, D. K. Sahu, Subhash Bose, Nancy Elias-Rosa, Mridweeka Singh, Anjasha Gangopadhyay, F. Huang, Shashi B. Pandey, Junqiang Zhang, Raya Dastidar, L. Tomasella, Kuntal Misra, Giacomo Terreran, Brijesh Kumar, P. Ochner, Liming Rui, X. F. Wang, Shengyu Yan, Leonardo Tartaglia
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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instname
We present the photometric and spectroscopic analysis of three Type II SNe: 2014cx, 2014cy and 2015cz. SN 2014cx is a conventional Type IIP with a shallow slope (0.2 mag/50d) and an atypical short plateau ($\sim$86 d). SNe 2014cy and 2015cz show rela
Autor:
Xiaofeng Wang, A. S. Moskvitin, Danfeng Xiang, Han Lin, Sergei Blinnikov, Elena A. Balakina, Liming Rui, Maria Pruzhinskaya, Huijuan Wang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 501:5797-5810
In this work we present the photometric and spectroscopic observations of Type IIb Supernova 2017gpn. This supernova was discovered in the error-box of LIGO/Virgo G299232 gravitational-wave event. We obtained the light curves in B and R passbands and
Autor:
András Pál, F. Huang, Łukasz Wyrzykowski, A. Ordasi, Ádám Sódor, T. G. Brink, R. Szakats, Attila Bódi, G. Zsidi, L. Kriskovics, Jujia Zhang, Alexei V. Filippenko, Vinkó József, J. M. Derkacy, K. Vida, G. Csörnyei, O. Hanyecz, Cs. Kalup, Jun Mo, P. Mikołajczyk, Hanna Sai, X. Zhang, Réka Könyves-Tóth, B. Ignácz, E. Baron, Huijuan Wang, Qian Zhai, Xiaofeng Wang, Krisztián Sárneczky, WeiKang Zheng, Liming Rui, Tianmeng Zhang
Publikováno v:
Monthly Notices of the Royal Astronomical Society
We present extensive observations of SN 2018zd covering the first $\sim450$\,d after the explosion. This SN shows a possible shock-breakout signal $\sim3.6$\,hr after the explosion in the unfiltered light curve, and prominent flash-ionisation spectra
Autor:
Danfeng Xiang, Justyn R. Maund, Xiaofeng Wang, Jujia Zhang, Jun Mo, Tianmeng Zhang, Lifan Wang, Liming Rui, Avishy Gal-Yam
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 485:1990-2000
We presented a detailed analysis of progenitor properties of type IIP supernova 2017eaw in NGC 6946, based on the pre-explosion images and early-time observations obtained immediately after the explosion. An unusually red star, with M$_{F814W}$ = $-$
Autor:
Danfeng Xiang, Zhihao Chen, Jun Mo, Hanna Sai, Y Hsiao, Wenxiong Li, T. G. Brink, Gaobo Xi, Liming Rui, Alexei V. Filippenko, Sh. A. Ehgamberdiev, X. F. Wang, Ling-Jun Wang, WeiKang Zheng, Weili Lin, Liang-Duan Liu, Jie Zhang, Shengyu Yan, D. O. Mirzaqulov, E. Baron, Xiaolin Li, Xinghan Zhang, Chengyuan Wu, J. M. Derkacy, J. Zhang, T. Zhang
SN 2018hti is a Type I superluminous supernova (SLSN~I) with an absolute $g$-band magnitude of $-22.2$ at maximum brightness, discovered in a metal-poor galaxy at a redshift of 0.0612. We present extensive photometric and spectroscopic observations o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7140a8c252dd0a07f919c9c93882c379
Autor:
Auni Somero, L. Tomasella, Eran O. Ofek, Erik C. Kool, Tuomas Kangas, F. Ciabattari, Leonardo Tartaglia, Stefano Valenti, Giacomo Terreran, A. Pastorello, J. Zhang, A. Nyholm, Zhi-Ping Jin, Jun Mo, Massimo Turatto, Jussi Harmanen, Adam Rubin, Nancy Elias-Rosa, H. Tan, Liming Rui, Xiang-Yu Wang, Claes Fransson, Dale Andrew Howell, T. M. Reynolds, Tianmeng Zhang, Curtis McCully, Stefano Benetti, E. Callis, Danfeng Xiang, Cristina Barbarino, Ana Sagués Carracedo, Morgan Fraser, Enrico Cappellaro, Francesco Taddia, Seppo Mattila, Wenxiong Li, A. Morales-Garoffolo, Jesper Sollerman, Christoffer Fremling, Griffin Hosseinzadeh, Fang Huang, David J. Sand, Peter Lundqvist, X. Gao
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
BASE-Bielefeld Academic Search Engine
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BASE-Bielefeld Academic Search Engine
Full author list: L. Tartaglia, A. Pastorello, J. Sollerman, C. Fransson, S. Mattila, M. Fraser, F. Taddia, L. Tomasella, M. Turatto, A. Morales-Garoffolo, N. Elias-Rosa, P. Lundqvist, J. Harmanen, T. Reynolds, E. Cappellaro, C. Barbarino, A. Nyholm,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::21823d3202156207806f5139f31b132f
http://hdl.handle.net/10261/234254
http://hdl.handle.net/10261/234254
Autor:
L. Tomasella, Hongbin Li, Leonardo Tartaglia, S. Taubenberger, Xiaojun Jiang, Nancy Elias-Rosa, Xiaofeng Wang, S. Benetti, P. Ochner, Liming Rui, Ulisse Munari, Xulin Zhao, Han Lin, F. Huang, Jujia Zhang, Giacomo Terreran, Linyi Li, Zhenyu Wu, Jianrong Shi, J. Craig Wheeler, Wenxiong Li, Danfeng Xiang, Alessandro Siviero, Jin-Ming Bai, Tianmeng Zhang, A. Pastorello, Kaicheng Zhang, Hao Song
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 481:878-893
We present extensive spectroscopic observations for one of the closest type Ia supernovae (SNe Ia), SN 2014J discovered in M82, ranging from 10.4 days before to 473.2 days after B-band maximum light. The diffuse interstellar band (DIB) features detec