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D. Jeong

94 papers hereh-index 394.7k citations110 works total

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

author position
  • first author18
  • middle author54
  • last author17

Across the 89 of 94 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO75
  • astro-ph.GA11
  • astro-ph3
  • astro-ph.IM2
  • hep-ph2
  • astro-ph.HE1
same name
  • D. Jeong — 10 papers, h 3
  • D. Jeong — 8 papers, h 36
  • D. Jeong — 6 papers, h 17
  • D. Jeong — 6 papers, h 10
  • D. Jeong — 5 papers, h 2
  • D. Jeong — 3 papers, h 6

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 citedLarge-Scale Galaxy Bias

818 citations · 5.1k across the 93 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2008★ 71 cited

Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling

Masatoshi Shoji, Donghui Jeong, Eiichiro Komatsu

We present a method for extracting the angular diameter distances, DA​, and the expansion rates, H, of the universe from the {\it two-dimensional} Baryon Acoustic Oscillations…

astro-ph2008★ 93 cited

Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space

Donghui Jeong, Eiichiro Komatsu

We calculate the non-linear galaxy power spectrum in real space, including non-linear distortion of the Baryon Acoustic Oscillations, using the standard 3rd-order perturbation theo…

astro-ph2006★ 193 cited

Perturbation Theory Reloaded: Analytical Calculation of Non-linearity in Baryonic Oscillations in the Real Space Matter Power Spectrum

Donghui Jeong, Eiichiro Komatsu

We compare the non-linear matter power spectrum in real space calculated analytically from 3rd-order perturbation theory with N-body simulations at 1<z<6. We find that the perturba…

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