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researcher

G. Zhu

46 papers hereh-index 3510.8k citations69 works total

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

author position
  • sole author2
  • first author8
  • middle author19
  • last author13

Across the 42 of 46 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA19
  • astro-ph.CO17
  • astro-ph.IM6
  • astro-ph3
  • astro-ph.SR1
same name
  • G. Zhu — 43 papers, h 18
  • G. Zhu — 29 papers, h 8
  • G. Zhu — 24 papers, h 22
  • G. Zhu — 9 papers, h 0
  • G. Zhu — 7 papers, h 5
  • G. Zhu — 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
20062023
most citedThe Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey

1.5k citations · 7.6k across the 45 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.IM2018★ 356 cited

The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library

D. S. Aguado, Romina Ahumada, Andres Almeida +230

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years o…

astro-ph.GA2018★ 192 cited

The Sloan Digital Sky Survey Reverberation Mapping Project: Sample Characterization

Yue Shen, Patrick B. Hall, Keith Horne +24

We present a detailed characterization of the 849 broad-line quasars from the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project. Our quasar sample covers a redshift…

astro-ph.GA2018★ 8 cited

Extreme circumgalactic HI and CIII absorption around the most massive, quenched galaxies

Marijana Smailagić, Jason Xavier Prochaska, Joseph Burchett +2

Luminous red galaxies (LRGs) are the most massive galaxies at z∼0.5 and, by selection, have negligible star formation. These objects have halo masses between those of L∗​…

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