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Aaron Smith

28 papers hereh-index 15587 citations38 works total

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

author position
  • first author11
  • middle author14
  • last author2

Across the 27 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA20
  • astro-ph.CO7
  • astro-ph.SR1
same name
  • Aaron Smith — 37 papers, h 7
  • Aaron Smith — 30 papers, h 11
  • Aaron Smith — 18 papers, h 9
  • Aaron Smith — 10 papers, h 1
  • Aaron Smith — 8 papers, h 3
  • Aaron Smith — 6 papers, h 2

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
20112023
most citedThe THESAN project: properties of the intergalactic medium and its connection to Reionization-era galaxies

125 citations · 1.1k across the 28 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.GA2023★ 3 cited

THESAN-HR: Galaxies in the Epoch of Reionization in warm dark matter, fuzzy dark matter and interacting dark matter

Xuejian Shen, Josh Borrow, Mark Vogelsberger +8

Using high-resolution cosmological radiation-hydrodynamic (RHD) simulations (THESAN-HR), we explore the impact of alternative dark matter (altDM) models on galaxies during the Epoc…

astro-ph.GA2023★ 2 cited

Efficient simulations of ionized ISM emission lines: A detailed comparison between the FIRE high-redshift suite and observations

Shengqi Yang, Adam Lidz, Aaron Smith +2

The Atacama Large Millimeter/Submillimeter Array (ALMA) in the sub-millimeter and the James Webb Space Telescope (JWST) in the infrared have achieved robust spectroscopic detection…

astro-ph.GA2023

X-ray scaling relations of early-type galaxies in IllustrisTNG and a new way of identifying backsplash objects

Yunchong Wang, Mark Vogelsberger, Dong-Woo Kim +9

We investigate how feedback and environment shapes the X-ray scaling relations of early-type galaxies (ETGs), especially at the low-mass end. We select central-ETGs from the Illust…

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