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Autori principali: Li, Jiang-Tao, Yu, Xiaodi, Mao, Huiyang, Chen, Hanxiao, Yang, Tiancheng, Qu, Zhijie, Bian, Fuyan, Bregman, Joel N., Cai, Zheng, Fan, Xiaohui, Fang, Taotao, Ji, Li, Ji, Zhiyuan, Johnson, Sean D., Li, Guoliang, Liu, Weizhe, Song, Ying-Yi, Wang, Feige, Wang, Tao, Wang, Xin, Williams, Christina, Xu, Mingxuan, Yang, Jinyi, Yang, Yang, Zheng, Xianzhong
Natura: Preprint
Pubblicazione: 2024
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Accesso online:https://arxiv.org/abs/2411.05396
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author Li, Jiang-Tao
Yu, Xiaodi
Mao, Huiyang
Chen, Hanxiao
Yang, Tiancheng
Qu, Zhijie
Bian, Fuyan
Bregman, Joel N.
Cai, Zheng
Fan, Xiaohui
Fang, Taotao
Ji, Li
Ji, Zhiyuan
Johnson, Sean D.
Li, Guoliang
Liu, Weizhe
Song, Ying-Yi
Wang, Feige
Wang, Tao
Wang, Xin
Williams, Christina
Xu, Mingxuan
Yang, Jinyi
Yang, Yang
Zheng, Xianzhong
author_facet Li, Jiang-Tao
Yu, Xiaodi
Mao, Huiyang
Chen, Hanxiao
Yang, Tiancheng
Qu, Zhijie
Bian, Fuyan
Bregman, Joel N.
Cai, Zheng
Fan, Xiaohui
Fang, Taotao
Ji, Li
Ji, Zhiyuan
Johnson, Sean D.
Li, Guoliang
Liu, Weizhe
Song, Ying-Yi
Wang, Feige
Wang, Tao
Wang, Xin
Williams, Christina
Xu, Mingxuan
Yang, Jinyi
Yang, Yang
Zheng, Xianzhong
contents The He II reionization epoch is expected to take place at $z\sim3-5$. In this stage, the helium and metals in the inter-galactic medium (IGM) are further ionized with additional contributions from harder non-stellar sources, and some large-scale gravitationally bound systems approach virialization. The "Probing the He II re-Ionization ERa via Absorbing C IV Historical Yield (HIERACHY)" program utilizes high- and medium-resolution spectra of bright background quasars at $z\approx3.9-5.2$ to investigate Ly$α$, C IV, and other metal absorption lines during this epoch. Additionally, we employ narrow-band imaging to search for Ly$α$ emitters associated with C IV absorbers, alongside multi-wavelength observations to identify and study particularly intriguing cases. In this paper, we present the design of the HIERACHY program, its current status, major scientific goals, and examples of initial data products from completed Magellan/MIKE, MagE spectroscopy, and MDM imaging observations. We also provide a brief outlook on future multi-wavelength observations that may significantly impact the related science.
format Preprint
id arxiv_https___arxiv_org_abs_2411_05396
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Probing the He II re-Ionization ERa via Absorbing C IV Historical Yield (HIERACHY) II: Project Design, Current Status, and Examples of Initial Data Products
Li, Jiang-Tao
Yu, Xiaodi
Mao, Huiyang
Chen, Hanxiao
Yang, Tiancheng
Qu, Zhijie
Bian, Fuyan
Bregman, Joel N.
Cai, Zheng
Fan, Xiaohui
Fang, Taotao
Ji, Li
Ji, Zhiyuan
Johnson, Sean D.
Li, Guoliang
Liu, Weizhe
Song, Ying-Yi
Wang, Feige
Wang, Tao
Wang, Xin
Williams, Christina
Xu, Mingxuan
Yang, Jinyi
Yang, Yang
Zheng, Xianzhong
Astrophysics of Galaxies
Cosmology and Nongalactic Astrophysics
The He II reionization epoch is expected to take place at $z\sim3-5$. In this stage, the helium and metals in the inter-galactic medium (IGM) are further ionized with additional contributions from harder non-stellar sources, and some large-scale gravitationally bound systems approach virialization. The "Probing the He II re-Ionization ERa via Absorbing C IV Historical Yield (HIERACHY)" program utilizes high- and medium-resolution spectra of bright background quasars at $z\approx3.9-5.2$ to investigate Ly$α$, C IV, and other metal absorption lines during this epoch. Additionally, we employ narrow-band imaging to search for Ly$α$ emitters associated with C IV absorbers, alongside multi-wavelength observations to identify and study particularly intriguing cases. In this paper, we present the design of the HIERACHY program, its current status, major scientific goals, and examples of initial data products from completed Magellan/MIKE, MagE spectroscopy, and MDM imaging observations. We also provide a brief outlook on future multi-wavelength observations that may significantly impact the related science.
title Probing the He II re-Ionization ERa via Absorbing C IV Historical Yield (HIERACHY) II: Project Design, Current Status, and Examples of Initial Data Products
topic Astrophysics of Galaxies
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2411.05396