Zobrazeno 1 - 10
of 98
pro vyhledávání: '"Zhao, XuLin"'
Autor:
Zhao, Xulin
Absorption features Ca II NIR and Ca II H&K of type Ia supernovae (SNe Ia) are characterized by their strong high-velocity features (HVFs). We find that, for these two features of calcium there is a puzzling anti-correlation between the line strength
Externí odkaz:
http://arxiv.org/abs/2411.15465
Autor:
Lin, Han, Wang, Xiaofeng, Zhang, Jujia, Xiang, Danfeng, Zhang, Tianmeng, Zhao, Xulin, Zhang, Xinghan, Sai, Hanna, Rui, Liming, Mo, Jun, Xi, Gaobo, Huang, Fang, Li, Xue, Cai, Yongzhi, Lin, Weili, Lin, Jie, Wu, Chengyuan, Zhang, Jicheng, Chen, Zhihao, Li, Zhitong, Li, Wenxiong, Li, Linyi, Zhang, Kaicheng, Miao, Cheng, Chen, Juncheng, Fan, Zhou, Fu, Jianning, Qian, Shengbang, Wu, Hong, Wu, Xue-Bing, Yan, Jingzhi, Zhang, Huawei, Zhang, Junbo, Zhang, Liyun, Zheng, Jie, Zhai, Qian
We present 206 unpublished optical spectra of 104 type II supernovae obtained by the Xinglong 2.16m telescope and Lijiang 2.4m telescope during the period from 2011 to 2018, spanning the phases from about 1 to 200 days after the SN explosion. The spe
Externí odkaz:
http://arxiv.org/abs/2401.05889
Autor:
Li, Zhitong, Zhang, Tianmeng, Wang, Xiaofeng, Zhang, Jujia, Galbany, Lluís, Filippenko, Alexei V., Brink, Thomas G., Ashall, Chris, Zheng, WeiKang, de Jaeger, Thomas, Ragosta, Fabio, Deckers, Maxime, Gromadzki, Mariusz, Young, D. R., Xi, Gaobo, Chen, Juncheng, Zhao, Xulin, Sai, Hanna, Yan, Shengyu, Xiang, Danfeng, Chen, Zhihao, Li, Wenxiong, Wang, Bo, Zou, Hu, Sui, Jipeng, Wang, Jiali, Ma, Jun, Nie, Jundan, Xue, Suijian, Zhou, Xu, Zhou, Zhimin
We have conducted photometric and spectroscopic observations of the peculiar Type Ia supernova (SN Ia) 2016ije that was discovered through the Tsinghua-NAOC Transient Survey. This peculiar object exploded in the outskirts of a metal-poor, low-surface
Externí odkaz:
http://arxiv.org/abs/2305.09417
Autor:
Zhao, Xulin1 (AUTHOR) zhaoxulin@bgrimm.com, Wang, Haijun1,2 (AUTHOR) jinjunchao2008@163.com, Luo, Guanghua3 (AUTHOR) luoguanghua@ganfenglithium.com, Dai, Kewei3 (AUTHOR) daikewei@ganfenglithium.com, Hu, Qinghua3 (AUTHOR) huqinghuacsu@163.com, Jin, Junchao2 (AUTHOR), Liu, Yang1 (AUTHOR) miaoyonggang@bgrimm.com, Liu, Baowen3 (AUTHOR) gurk73@163.com, Miao, Yonggang1 (AUTHOR) zhukunlei@bgrimm.com, Zhu, Kunlei1 (AUTHOR) liujianbo@bgrimm.com, Liu, Jianbo1 (AUTHOR), Zhang, Hai3 (AUTHOR) zhanghai01504130@163.com, Wu, Lianhe3 (AUTHOR) so51mn@163.com, Wu, Jianming3 (AUTHOR) ctbwjm@126.com, Lu, Yueming3 (AUTHOR) 13674863094@163.com, Wang, Wei3 (AUTHOR) wangwei_722@163.com, Lv, Dingchao4 (AUTHOR) salman_zhao@126.com
Publikováno v:
Minerals (2075-163X). Oct2024, Vol. 14 Issue 10, p964. 14p.
Autor:
Li, Zhitong, Zhang, Tianmeng, Wang, Xiaofeng, Sai, Hanna, Zhang, Jujia, Chen, Juncheng, Zhao, Xulin, Yan, Shengyu, Wang, Bo, Phillips, Mark M., Hsiao, Eric Y., Morrell, Nidia, Contreras, Carlos, Burns, Christopher R., Ashall, Christopher, Stritzinger, Maximilian, Krisciunas, Kevin, Prieto, Jose, Zou, Hu, Wang, Jiali, Ma, Jun, Nie, Jundan, Xue, Suijian, Zhou, Xu, Zhou, Zhimin, Xiang, Danfeng, Xi, Gaobo
In this paper, we present photometric and spectroscopic observations of a subluminous type Ia supernova (SN Ia) 2012ij, which has an absolute $B$-band peak magnitude $M_{B,\rm{max}}$ = $-$17.95 $\pm$ 0.15 mag. The $B$-band light curve exhibits a fast
Externí odkaz:
http://arxiv.org/abs/2201.06066
Autor:
Lin, Han, Wang, Xiaofeng, Zhang, Jujia, Lin, Weili, Mo, Jun, Filippenko, Alexei V., Zheng, WeiKang, Brown, Peter J., Xiang, Danfeng, Huang, Fang, Cai, Yongzhi, Zhang, Tianmeng, Li, Xue, Rui, Liming, Zhang, Xinghan, Sai, Hanna, Zhao, Xulin, Graham, Melissa L., Shivvers, I., Halevi, G., Yuk, H., Brink, Thomas G.
We present optical and ultraviolet photometry, as well as optical spectra, for the type II supernova (SN) 2015bf. Our observations cover the phases from $\sim 2$ to $\sim 200$ d after explosion. The first spectrum is characterised by a blue continuum
Externí odkaz:
http://arxiv.org/abs/2106.04375
Autor:
Sai, Hanna, Wang, Xiaofeng, Wu, Jianfeng, Lin, Jie, Feng, Hua, Zhang, Tianmeng, Li, Wenxiong, Zhang, Jujia, Mo, Jun, Sun, Tianrui, Ehgamberdiev, Shuhrat A., Mirzaqulov, Davron, Rui, Liming, Lin, Weili, Zhao, Xulin, Lin, Han, Zhang, Jicheng, Zhang, Xinghan, Zhao, Yong, Li, Xue, Xiang, Danfeng, Wang, Lingzhi, Wu, Chengyuan
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
Externí odkaz:
http://arxiv.org/abs/2104.10370
We studied the spectral features of Si II $\lambda\lambda$4130, 5972, 6355 and S II W-trough for a large sample of Type Ia supernovae (SNe Ia). We find that in NV (Normal-Velocity) subclass of SNe Ia, these features tend to reach a maximum line stren
Externí odkaz:
http://arxiv.org/abs/2104.02875
Autor:
Zhang, Tianmeng, Wang, Xiaofeng, Zhao, Xulin, Xu, Dong, Reguitti, Andrea, Zhang, Jujia, Pastorello, Andrea, Tomasella, Lina, Ochner, Paolo, Tartaglia, Leonardo, Benetti, Stefano, Turatto, Massimo, Harutyunyan, Avet, Elias-Rosa, Nancy, Huang, Fang, Zhang, Kaicheng, Chen, Juncheng, Jiang, Zhaoji, Ma, Jun, Nie, Jundan, Peng, Xiyan, Zhou, Xu, Zhou, Zhimin, Zou, Hu
In this paper, we present extensive optical and ultraviolet (UV) observations of the type Ia supernova (SN Ia) 2013gs discovered during the Tsinghua-NAOC Transient Survey. The photometric observations in the optical show that the light curves of SN 2
Externí odkaz:
http://arxiv.org/abs/1901.01353
Autor:
Wang, Xiaofeng, Chen, Jia, Wang, Lifan, Hu, Maokai, Xi, Gaobo, Yang, Yi, Zhao, Xulin, Li, Wenxiong
Type Ia supernovae (SNe Ia) play key roles in revealing the accelerating expansion of the universe, but our knowledge about their progenitors is still very limited. Here we report the discovery of a rigid dichotomy in circumstellar (CS) environments
Externí odkaz:
http://arxiv.org/abs/1810.11936