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researcher

C. Chuang

127 papers hereh-index 6021.4k citations151 works total

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

author position
  • first author11
  • middle author91
  • last author6

Across the 108 of 127 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO115
  • astro-ph.IM7
  • astro-ph.GA4
  • astro-ph1
same name
  • C. Chuang — 4 papers, h 3
  • C. Chuang — 3 papers, h 11
  • C. Chuang — 2 papers, h 28
  • C. Chuang — 2 papers, h 5
  • C. Chuang — 1 paper, h 6
  • C. Chuang — 1 paper, h 7

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
20052025
most citedThe clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

3.1k citations · 23.9k across the 124 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.CO2012★ 45 cited

Toward More Realistic Forecasting of Dark Energy Constraints from Galaxy Redshift Surveys

Yun Wang, Chia-Hsun Chuang, Christopher M. Hirata

Galaxy redshift surveys are becoming increasingly important as a dark energy probe. We improve the forecasting of dark energy constraints from galaxy redshift surveys by using the…

astro-ph.CO2012★ 331 cited

Modeling the Anisotropic Two-Point Galaxy Correlation Function on Small Scales and Improved Measurements of H(z), D_A(z), and f(z)sigma_8(z) from the Sloan Digital Sky Survey DR7 Luminous Red Galaxies

Chia-Hsun Chuang, Yun Wang

We present a simple and efficient phenomenological model for the two-dimensional two-point galaxy correlation function that works well over a wide range of scales, from large scale…

astro-ph.CO2012★ 33 cited

Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies

Chia-Hsun Chuang, Yun Wang

Galaxy clustering data can be used to measure the cosmic expansion history H(z), the angular-diameter distance D_A(z), and the linear redshift-space distortion parameter beta(z). H…

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