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S. Peng Oh

3 papers here

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

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.CO1
ORCID 0000-0002-1013-4657

identity via Semantic Scholar / OpenAlex

most citedEarly Cosmological HII/HeIII Regions and Their Impact on Second-Generation Star Formation

208 citations · 347 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.CO2009★ 13 cited

Cosmology from the Highly-Redshifted 21 cm Line

Steven Furlanetto, Adam Lidz, Abraham Loeb +26

One of the next decade's most exciting prospects is to explore the cosmic "dark ages," during which the first stars in the Universe formed, with the 21 cm line of neutral hydrogen.…

astro-ph2006★ 208 cited

Early Cosmological HII/HeIII Regions and Their Impact on Second-Generation Star Formation

Naoki Yoshida, S. Peng Oh, Tetsu Kitayama +1

(Abridged) We present the results of three-dimensional radiation-hydrodynamics simulations of the formation and evolution of early HII/HeIII regions around the first stars. Cooling…

astro-ph2006★ 126 cited

The Effects of Dark Matter Decay and Annihilation on the High-Redshift 21 cm Background

Steven Furlanetto, S. Peng Oh, Elena Pierpaoli

The radiation background produced by the 21 cm spin-flip transition of neutral hydrogen at high redshifts can be a pristine probe of fundamental physics and cosmology. At z~30-300,…

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