High Redshift Obscured Quasars and the Need for Optical to NIR, Massively Multiplexed, Spectroscopic Facilities
by Andreea Petric, Mark Lacy, Stéphanie Juneau, Yue Shen, Xiaohui Fan, Nicolas Flagey, Yjan Gordon, Daryl Haggard, Patrick B. Hall, Nimish Hathi, Dragana Ilic, Claudia D.P. Lagos, Xin Liu, Christopher O'Dea, Luka C. Popović, Andy Sheinis, Yiping Wang, and Yongquan Xue
Published onMay 31, 2019
High Redshift Obscured Quasars and the Need for Optical to NIR, Massively Multiplexed, Spectroscopic Facilities
·
Abstract
We emphasize the need for future massively multiplexed spectroscopic instruments that can perform dedicated surveys in the optical and NIR to pin down the nature and demographics of obscured growing black-holes at z > 1. These key studies will shed light on the role of black holes in galaxy evolution during the epoch of peak growth activity.
The full text of this article is only available in PDF format:
Creative Commons Attribution 4.0 International License (CC-BY 4.0)
