activity
20162022
most citedThe Final SDSS High-Redshift Quasar Sample of 52 Quasars at z>5.7

340 citations · 957 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2022★ 26 cited

Demographics of z ~ 6 Quasars in the Black Hole Mass-Luminosity Plane

Jin Wu, Yue Shen, Linhua Jiang +8

We study the demographics of z ~ 6 broad-line quasars in the black hole (BH) mass-luminosity plane using a sample of more than 100 quasars at 5.7 < z < 6.5. These quasars have well…

astro-ph.GA2022★ 50 cited

Definitive upper bound on the negligible contribution of quasars to cosmic reionization

Linhua Jiang, Yuanhang Ning, Xiaohui Fan +7

Cosmic (hydrogen) reionization marks one of the major phase transitions of the universe at redshift z >= 6. During this epoch, hydrogen atoms in the intergalactic medium (IGM) were…

astro-ph.GA2021★ 12 cited

Quasar UV Luminosity Function at from SDSS Deep Imaging Data

Zhiwei Pan, Linhua Jiang, Xiaohui Fan +2

We present a well-designed sample of more than 1000 type 1 quasars at and derive UV quasar luminosity functions (QLFs) in this redshift range. These quasars were selected…

astro-ph.GA2021★ 44 cited

The Magellan M2FS Spectroscopic Survey of High- Galaxies: Lyα Emitters at and the Evolution of Lyα Luminosity Function over

Yuanhang Ning, Linhua Jiang, Zhen-Ya Zheng +1

We present a sample of Lyα emitters (LAEs) at from our spectroscopic survey of high-redshift galaxies using the multi-object spectrograph M2FS on the Magellan Clay te…

astro-ph.GA2021★ 39 cited

Metallicity in Quasar Broad Line Regions at Redshift 6

Shu Wang, Linhua Jiang, Yue Shen +10

Broad line regions (BLRs) in high-redshift quasars provide crucial information of chemical enrichment in the early universe. Here we present a study of BLR metallicities in 33 quas…

astro-ph.GA2020★ 21 cited

Strong Mg II and Fe II Absorbers at 2.2 < z < 6.0

Siwei Zou, Linhua Jiang, Yue Shen +13

We present a study of strong intervening absorption systems in the near-IR spectra of 31 luminous quasars at . The quasar spectra were obtained with {\it Gemini} GNIRS that…