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researcher

Yongquan Xue

72 papers hereh-index 323.4k citations117 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author3
  • middle author40
  • last author15

Across the 59 of 72 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA40
  • astro-ph.HE16
  • astro-ph7
  • astro-ph.CO6
  • astro-ph.IM3
same name
  • Yongquan Xue — 26 papers, h 6
  • Yongquan Xue — 18 papers, h 13
  • Yongquan Xue — 15 papers, h 4
  • Yongquan Xue — 9 papers, h 1
  • Yongquan Xue — 1 paper
  • Yongquan Xue — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20042026
most citedThe Chandra Deep Field-South Survey: 4 Ms Source Catalogs

581 citations · 4.1k across the 72 of their papers we have counts for

collaborators
Showing 2024 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2024★ 4 cited

Photometric Selection of type 1 Quasars in the XMM-LSS Field with Machine Learning and the Disk-Corona Connection

Jian Huang, Bin Luo, W. N. Brandt +4

We present photometric selection of type 1 quasars in the ≈5.3 deg2 XMM-Large Scale Structure (XMM-LSS) survey field with machine learning. We constructed our trai…

astro-ph.GA2024

Dust-Obscured Galaxies in the XMM-SERVS Fields: Selection, Multiwavelength Characterization, and Physical Nature

Zhibo Yu, W. N. Brandt, Fan Zou +7

Dust-obscured galaxies (DOGs) are enshrouded by dust, and many are believed to host accreting supermassive black holes (SMBHs), which makes them unique objects for probing the coev…

astro-ph.GA2024

The Cosmic Evolution of the Supermassive Black Hole Population: A Hybrid Observed Accretion and Simulated Mergers Approach

Fan Zou, W. N. Brandt, Elena Gallo +4

Supermassive black holes (SMBHs) can grow through both accretion and mergers. It is still unclear how SMBHs evolve under these two channels from high redshifts to the SMBH populati…

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