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researcher

Y. Shen

16 papers hereh-index 9761 citations69 works total

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

author position
  • middle author8

Across the 8 of 16 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE11
  • astro-ph.GA3
  • astro-ph.IM2
same name
  • Y. Shen — 23 papers, h 9
  • Y. Shen — 11 papers, h 19
  • Y. Shen — 9 papers
  • Y. Shen — 9 papers, h 12
  • Y. Shen — 7 papers, h 11
  • Y. Shen — 6 papers

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
20182026
most citedThe eROSITA Final Equatorial-Depth Survey (eFEDS): Identification and characterization of the counterparts to the point-like sources

122 citations · 218 across the 16 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2026★ 2 cited

Robust AGN and host-galaxy decomposition in optical spectral fitting

C. Aydar, A. Merloni, G. Zeltyn +24

Unraveling the growth of supermassive black holes and their connection to host galaxies requires disentangling the Active Galactic Nuclei (AGN) emission from that of the stellar po…

astro-ph.GA2024★ 15 cited

Estimating Masses of Supermassive Black Holes in Active Galactic Nuclei from the Halpha Emission Line

E. Dalla Bontà, B. M. Peterson, C. J. Grier +19

The goal of this project is to construct an estimator for the masses of supermassive black holes in active galactic nuclei (AGNs) based on the broad Halpha emission line. We make u…

astro-ph.GA2018★ 14 cited

UV-Luminous, Star-Forming Hosts of z~2 Reddened Quasars in the Dark Energy Survey

C. F. Wethers, M. Banerji, P. C. Hewett +55

We present the first rest-frame UV population study of 17 heavily reddened, high-luminosity (E(B-V)QSO​≳ 0.5; Lbol​> 1046ergs−1) broad-line quasar…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.