Zobrazeno 1 - 10
of 843
pro vyhledávání: '"JIANG, CHUNYAN"'
Autor:
Lin, Ruqiu, Zheng, Zhen-Ya, Jiang, Chunyan, Yuan, Fang-Ting, Ho, Luis C., Wang, Junxian, Jiang, Linhua, Rhoads, James E., Malhotra, Sangeeta, Barrientos, L. Felipe, Wold, Isak, Infante, Leopoldo, Zhu, Shuairu, Ji, Xiang, Fu, Xiaodan
Recently, the James Webb Space Telescope (JWST) has revealed a new class of high redshift (high-$z$, $z>4$) compact galaxies which are red in the rest-frame optical and blue in the rest-frame UV as V-shaped spectral energy distributions (SEDs), refer
Externí odkaz:
http://arxiv.org/abs/2412.08396
Understanding the ionizing photon escape from galaxies is essential for studying Cosmic Reionization. With a sample of 23 Lyman Continuum (LyC) leakers at $3
Externí odkaz:
http://arxiv.org/abs/2412.08395
Lyman continuum (LyC) emitters at $z>3$ provide critical samples for studying the contribution of galaxies to the ionizing background in the Epoch of Reionization. We collect a sample of $z>3$ LyC emitters, a dominant fraction ($\sim$60%-70%) of whic
Externí odkaz:
http://arxiv.org/abs/2409.20352
Autor:
Lin, Ruqiu, Zheng, Zhen-Ya, Yuan, Fang-Ting, Wang, Jun-Xian, Jiang, Chunyan, Jiang, Ning, Wang, Lingzhi, Jiang, Linhua, Ji, Xiang, Zhu, Shuairu, Fu, Xiaodan
Publikováno v:
2024SCPMA..6709811L
The scaling relation of central massive black holes (MBHs) and their host galaxies is well-studied for supermassive BHs (SMBHs, $M_{\rm BH}\ \ge 10^6\, M_{\rm \odot}$). However, this relation has large uncertainties in the mass range of the intermedi
Externí odkaz:
http://arxiv.org/abs/2409.20350
We investigate the star-forming properties of 23 Lyman Continuum (LyC) leakers at z > 3 in the Great Observatories' Deep Survey-South (GOODS-S) field based on a systematic review of LyC observations from the literature. Using data from the Hubble Spa
Externí odkaz:
http://arxiv.org/abs/2409.20349
Autor:
Zhu, Shuairu, Zheng, Zhen-Ya, Rhoads, James, Wang, Junxian, Jiang, Linhua, Jiang, Chunyan, Yuan, Fang-Ting, Rahna, P. T., Hu, Weida, Lin, Ruqiu, Shan, Huanyuan, Xu, Chun, Infante, Leopoldo, Barrientos, L. Felipe, Zheng, Xianzhong, Fang, Guanwen, Liang, Zhixiong
We present the first results of the Hubble Deep Hydrogen Alpha (HDH$\alpha$) project, which analyzes the space-borne deep H$\alpha$ narrowband imaging data in the GOODS-S region. The HDH$\alpha$ data comprises 72 orbits' images taken with the HST ACS
Externí odkaz:
http://arxiv.org/abs/2312.06345
Autor:
Lin, Ruqiu, Zheng, Zhen-Ya, Wang, Jun-Xian, Yuan, Fang-Ting, Rhoads, James E., Malhotra, Sangeeta, An, Tao, Jiang, Chunyan, Zhu, Shuairu, Rahna, P. T., Ji, Xiang, Singha, Mainak
Although double-peaked narrow emission-line galaxies have been studied extensively in the past years, only a few are reported with the green pea galaxies (GPs). Here we present our discovery of five GPs with double-peaked narrow [OIII] emission lines
Externí odkaz:
http://arxiv.org/abs/2304.08284
Autor:
Lin, Ruqiu, Zheng, Zhen-Ya, Hu, Weida, Jiang, Chunyan, Pang, Xiang, Yang, Chenwei, Yuan, Fang-Ting, T., Rahna P., Wang, Jian-Guo, Wang, Yibo, Jiang, Ning, Zhu, Shuairu
Emission-line galaxies (ELGs) are crucial in understanding the formation and evolution of galaxies, while little is known about their variability. Here we report the study on the optical variability of a sample of ELGs selected in the COSMOS field, w
Externí odkaz:
http://arxiv.org/abs/2209.07087
Autor:
Liang, Cheng, Han, Yiman, Xu, Haoyang, Liu, Dan, Jiang, Chunyan, Li, Qingyu, Hu, Yungao, Xiang, Xunchao
Publikováno v:
In Carbohydrate Polymers 15 January 2025 348 Part A
Autor:
Harish, Santosh, Wold, Isak G. B., Malhotra, Sangeeta, Rhoads, James, Hu, Weida, Wang, Junxian, Zheng, Zhen-ya, Barrientos, L. Felipe, González-López, Jorge, Perez, Lucia A., Khostovan, Ali Ahmad, Infante, Leopoldo, Jiang, Chunyan, Moya-Sierralta, Cristóbal, Pharo, John, Valdes, Francisco, Yang, Huan
We report spectroscopic confirmations of 15 Lyman-alpha galaxies at $z\sim7$, implying a spectroscopic confirmation rate of $\sim$80% on candidates selected from LAGER (Lyman-Alpha Galaxies in the Epoch of Reionization), which is the largest (24 deg$
Externí odkaz:
http://arxiv.org/abs/2111.01173