Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Fang-Ting Yuan"'
Publikováno v:
The Astrophysical Journal Letters, Vol 974, Iss 1, p L20 (2024)
We investigate the star-forming properties of 23 Lyman continuum (LyC) leakers at z > 3 in the Great Observatories Origins Deep Survey-South field based on a systematic review of LyC observations from the literature. Using data from the Hubble Space
Externí odkaz:
https://doaj.org/article/03fd75bcce2a4064bfe6c8c4341dc327
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 1, p 53 (2024)
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 (∼60%–70%) of which
Externí odkaz:
https://doaj.org/article/d540c96d6f764da693aea7b077dea2d7
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 1, p 60 (2024)
We investigate the suppression of star formation in galaxy pairs based on the isolated galaxy pair sample derived from the Sloan Digital Sky Survey survey. By comparing the star formation rate between late-type galaxies (LTGs) in galaxy pairs and tho
Externí odkaz:
https://doaj.org/article/3655e8a4da114e278cdcf57fb44a194b
Autor:
Shuairu Zhu, Zhen-Ya Zheng, James Rhoads, Junxian Wang, Linhua Jiang, Chunyan Jiang, Fang-Ting Yuan, P. T. Rahna, Weida Hu, Ruqiu Lin, Huanyuan Shan, Chun Xu, Leopoldo Infante, L. Felipe Barrientos, Xianzhong Zheng, Guanwen Fang, Zhixiong Liang
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 271, Iss 1, p 5 (2024)
We present the first results of the Hubble Deep Hydrogen Alpha (HDH α ) project, which analyzes the space-borne deep H α narrowband imaging data in the GOODS-S region. The HDH α data comprises 72 orbits’ images taken with the Hubble Space Telesc
Externí odkaz:
https://doaj.org/article/4d1422682ad7468aa26b8700df54563f
Publikováno v:
The Astrophysical Journal Letters, Vol 946, Iss 1, p L7 (2023)
Using a sample of face-on star-forming galaxies selected from the Sloan Digital Sky Survey, we statistically derive the typical optical depth τ _cl of individual H ii regions based on the “Chocolate Chip Cookie” model of Lu et al. (2022). By bin
Externí odkaz:
https://doaj.org/article/308ac27a85604ab88d6bb2c4a3b9ed76
Using a sample of face-on star-forming galaxies selected from the Sloan Digital Sky Survey, we statistically derive the typical optical depth $\tau_{\rm{cl}}$ of individual HII regions based on the ``Chocolate Chip Cookie" model of Lu2022. By binning
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::85e556d1da76766acaa5aa7d93f7b934
http://arxiv.org/abs/2303.12303
http://arxiv.org/abs/2303.12303
Autor:
Ruqiu Lin, Zhen-Ya Zheng, Weida Hu, Chunyan Jiang, Xiang Pan, Chenwei Yang, Fang-Ting Yuan, P. T. Rahna, Jian-Guo Wang, Yibo Wang, Ning Jiang, Shuairu Zhu
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d1b2afb55f166b8f4499663f5c90b4d
Autor:
Gaoxiang Jin, Y. Sophia Dai, Hsi-An Pan, Lihwai Lin, Cheng Li, Bau-Ching Hsieh, Shiyin Shen, Fang-Ting Yuan, Shuai Feng, Cheng Cheng, Hai Xu, Jia-Sheng Huang, Kai Zhang
Publikováno v:
The Astrophysical Journal, vol 923, iss 1
The role of active galactic nuclei (AGNs) during galaxy interactions and how they influence the star formation in the system are still under debate. We use a sample of 1156 galaxies in galaxy pairs or mergers (hereafter `pairs') from the MaNGA survey
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::27ed64e1dc6445729cb73920571fbd7f
http://arxiv.org/abs/2109.11084
http://arxiv.org/abs/2109.11084
Publikováno v:
The Astrophysical Journal. 938:139
We present a new two-component dust geometry model, the Chocolate Chip Cookie model, where the clumpy nebular regions are embedded in a diffuse stellar/interstellar medium disk, like chocolate chips in a cookie. By approximating the binomial distribu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ed623175084f17c86be57d578c95811b
https://doi.org/10.3847/1538-4357/ac92e9
https://doi.org/10.3847/1538-4357/ac92e9
Publikováno v:
Proceedings of the International Astronomical Union. 15:201-205
At high redshift, the contribution of strong emission lines to the broadband photometry can cause large uncertainties when estimating galaxy physical properties. To examine this effect, we investigate a sample of 54 LBGs at 3 < zspec < 3.8 with detec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::066a103330f23ad6275f4a19e613416f
https://doi.org/10.1017/s174392131900276x
https://doi.org/10.1017/s174392131900276x