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researcher

Ran Wang

4 papers hereh-index 340 citations13 works total

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
same name
  • Ran Wang — 4 papers, h 3
  • Ran Wang — 4 papers, h 3
  • Ran Wang — 4 papers, h 4
  • Ran Wang — 3 papers, h 2
  • Ran Wang — 3 papers, h 2
  • Ran Wang — 2 papers, h 1

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

collaborators

4 papers

astro-ph.GA2026

Cm-wavelength Studies of Molecular Gas and Star Formation at High Redshift with the SKA

Ran Wang, Jeff Wagg, Mark T. Sargent +6

The Square Kilometre Array will be a revolutionary instrument for the study of gas in the distant Universe. At frequencies below ~50 GHz, observations of redshifted emission from l…

astro-ph.GA2026

High-Resolution ALMA Imaging for a Gravitationally-lensed Quasar at z=6.5: Constraining the AGN Contribution to Galactic-Scale Dust Heating

Minghao Yue, Xiaohui Fan, Anna-Christina Eilers +6

We present high-resolution (beam size $0\farcs076\times0\farcs040$) Atacama Large Millimeter/submillimeter Array (ALMA) observations of the far-infrared $(λ_\text{rest}=162.7μ\rm…

astro-ph.GA2026

CO(7-6) and [C I](2-1) survey in z > 6 quasars

Fuxiang Xu, Roberto Decarli, Ran Wang +13

High-redshift (z≳6) quasars trace the earliest supermassive black holes and intense star formation, offering key laboratories for black hole-galaxy evolution at cosmic dawn…

astro-ph.GA2025

The SUPERCOLD-CGM survey: II. [\ion{C}{1}](1−0) emission and the physical conditions of cold gas in Enormous LyI^± nebulae at z∼2

Jianan Li, Bjorn H. C. Emonts, Zheng Cai +13

We report ALMA and ACA observations of atomic carbon ([\ion{C}{1}](1−0)) and dust continuum in 10 Enormous LyI^± Nebulae hosting ultra-luminous Type-I QSOs at z=2.2−2.5, as pa…

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