Zobrazeno 1 - 10
of 157
pro vyhledávání: '"Zhang, Xinhan"'
Autor:
Liu, Qichun, Lin, Jie, Wang, Xiaofeng, Gu, Shenghong, Shi, Jianrong, Zhang, Liyun, Xi, Gaobo, Mo, Jun, Cai, Yongzhi, Chen, Liyang, Chen, Zhihao, Guo, Fangzhou, Jiang, Xiaojun, Li, Gaici, Li, Wenxiong, Lin, Han, Lin, Weili, Liu, Jialian, Miao, Cheng, Ma, Xiaoran, Peng, Haowei, Xiang, Danfeng, Yan, Shengyu, Zhang, Jicheng, Zhang, Xinhan
Publikováno v:
Mon. Not. Roy. Astron. Soc. 523, 2193-2208 (2023)
Tsinghua University-Ma Huateng Telescopes for Survey (TMTS) aims to detect fast-evolving transients in the Universe, which has led to the discovery of thousands of short-period variables and eclipsing binaries since 2020. In this paper, we present th
Externí odkaz:
http://arxiv.org/abs/2302.00197
Autor:
Liu, Wei, Yan, Jingzhi, Reig, Pablo, Wang, Xiaofeng, Xiao, Guangcheng, Lin, Han, Zhang, Xinhan, Sai, Hanna, Chen, Zhihao, Yan, Shengyu, Liu, Qingzhong
Publikováno v:
A&A 666, A110 (2022)
We have obtained optical spectroscopy and photometry data during four years after the event. The long-term photometric light-curve and the equivalent widths of the Halpha and He I 6678 lines were used to monitor the state of the Be star disk. The Hal
Externí odkaz:
http://arxiv.org/abs/2208.00151
Autor:
Qie, Zhipeng, Zhang, Xinhan, Wang, Ze, Liu, Zhongbao, Alhassawi, Hassan, Li, Hengfan, Chen, Guoqing, Zhao, Guangbo
Publikováno v:
In Journal of Industrial and Engineering Chemistry 25 November 2024 139:611-619
Autor:
Ma, Xiaowu, Jiao, Juying, Yang, Bo, Zhao, Wenting, Ling, Qi, Zhang, Xinhan, Han, Jianqiao, Du, Pengfei, Chen, Yin, Chen, Hao
Publikováno v:
In Journal of Hydrology November 2024 644
Publikováno v:
In Catena November 2024 246
Autor:
Zeng, Jinsong, Ma, Yue, Li, Pengfei, Zhang, Xinhan, Gao, Wenhua, Wang, Bin, Xu, Jun, Chen, Kefu
Publikováno v:
In Carbohydrate Polymers 15 April 2024 330
Autor:
Zhang, Xinhan, Li, Pengfei, Zeng, Jinsong, Li, Jinpeng, Gao, Wenhua, Wang, Bin, Xu, Jun, Chen, Kefu
Publikováno v:
In Chemical Engineering Journal 1 January 2024 479
Autor:
Zhang, Jujia, Wang, Xiaofeng, Vinko, Jozsef, Zhai, Qian, Zhang, Tianmeng, Filippenko, Alexei V., Brink, Thomas G., Zheng, WeiKang, Wyrzykowski, Lukasz, Mikolajczyk, Przemyslaw, Huang, Fang, Rui, Liming, Mo, Jun, Sai, Hanna, Zhang, Xinhan, Wang, Huijuan, DerKacy, James M., Baron, Eddie, Sarneczky, K., Bodi, A., Csornyei, G., Hanyecz, O., Ignacz, B., Kalup, Cs., Kriskovics, L., Konyves-Toth, R., Ordasi, A., Pal, A., Sodor, A., Szakats, R., Vida, K., Zsidi, G.
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
Externí odkaz:
http://arxiv.org/abs/2007.14348
Autor:
Jacobson-Galán, Wynn V., Margutti, Raffaella, Kilpatrick, Charles D., Hiramatsu, Daichi, Perets, Hagai, Khatami, David, Foley, Ryan J., Raymond, John, Yoon, Sung-Chul, Bobrick, Alexey, Zenati, Yossef, Galbany, Lluís, Andrews, Jennifer, Brown, Peter J., Cartier, Régis, Coppejans, Deanne L., Dimitriadis, Georgios, Dobson, Matthew, Hajela, Aprajita, Howell, D. Andrew, Kuncarayakti, Hanindyo, Milisavljevic, Danny, Rahman, Mohammed, Rojas-Bravo, César, Sand, David J., Shepherd, Joel, Smartt, Stephen J., Stacey, Holland, Stroh, Michael, Swift, Jonathan J., Terreran, Giacomo, Vinko, Jozsef, Wang, Xiaofeng, Anderson, Joseph P., Baron, Edward A., Berger, Edo, Blanchard, Peter K., Burke, Jamison, Coulter, David A., DeMarchi, Lindsay, DerKacy, James M., Fremling, Christoffer, Gomez, Sebastian, Gromadzki, Mariusz, Hosseinzadeh, Griffin, Kasen, Daniel, Kriskovics, Levente, McCully, Curtis, Müller-Bravo, Tomás E., Nicholl, Matt, Ordasi, András, Pellegrino, Craig, Piro, Anthony L., Pál, András, Ren, Juanjuan, Rest, Armin, Rich, R. Michael, Sai, Hanna, Sárneczky, Krisztián, Shen, Ken J., Short, Philip, Siebert, Matthew, Stauffer, Candice, Szakáts, Róbert, Zhang, Xinhan, Zhang, Jujia, Zhang, Kaicheng
We present panchromatic observations and modeling of the Calcium-rich supernova 2019ehk in the star-forming galaxy M100 (d$\approx$16.2 Mpc) starting 10 hours after explosion and continuing for ~300 days. SN 2019ehk shows a double-peaked optical ligh
Externí odkaz:
http://arxiv.org/abs/2005.01782
Autor:
Gangopadhyay, Anjasha, Misra, Kuntal, Hiramatsu, Daichi, Wang, Shan-Qin, Hosseinzadeh, Griffin, Wang, Xiaofeng, Valenti, Stefano, Zhang, Jujia, Howell, D. Andrew, Arcavi, Iair, Anupama, G. C., Burke, Jamison, Dastidar, Raya, Itagaki, Koichi, Kumar, Brajesh, Kumar, Brijesh, Li, Long, McCully, Curtis, Mo, Jun, Pandey, Shashi Bhushan, Pellegrino, Craig, Sai, Hanna, Sahu, D. K., Sanwal, Pankaj, Singh, Avinash, Singh, Mridweeka, Zhang, Jicheng, Zhang, Tianmeng, Zhang, Xinhan
We present photometric and spectroscopic observations of the type Ibn supernova (SN) 2019uo, the second ever SN Ibn with flash ionization (He II, C III, N III) features in its early spectra. SN 2019uo displays a rapid post-peak luminosity decline of
Externí odkaz:
http://arxiv.org/abs/1912.07878