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Min S. Yun

4 papers hereh-index 5817 citations10 works total

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

author position
  • first author1
  • middle author1
  • last author2

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

fields
  • astro-ph3
  • astro-ph.GA1
same name
  • Min S. Yun — 25 papers, h 9
  • Min S. Yun — 11 papers, h 4
  • Min S. Yun — 5 papers
  • Min S. Yun — 5 papers, h 2
  • Min S. Yun — 5 papers, h 6
  • Min S. Yun — 3 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
19992025
most citedRadio Properties of Infrared Selected Galaxies in the IRAS 2 Jy Sample

929 citations · 1.1k across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2025

ALMA and JWST Identification of Faint Dusty Star-Forming Galaxies up to z~8

Jorge A. Zavala, Andreas L. Faisst, Manuel Aravena +44

We exploit a new sample of around 400 bright dusty galaxies from the ALMA CHAMPS Large Program, together with the rich JWST multi-band data products in the COSMOS field, to explore…

astro-ph2001★ 929 cited

Radio Properties of Infrared Selected Galaxies in the IRAS 2 Jy Sample

Min S. Yun, Naveen A. Reddy, J. J. Condon

The radio counterparts to the IRAS Redshift Survey galaxies are identified in the NRAO VLA Sky Survey (NVSS) catalog. Our new catalog of the infrared flux-limited (S60 >= 2 Jy) com…

astro-ph2000★ 32 cited

Dust Emission from High Redshift QSOs

C. L. Carilli, F. Bertoldi, K. M. Menten +8

We present detections of emission at 250 GHz (1.2 mm) from two high redshift QSOs from the Sloan Digital Sky Survey sample using the bolometer array at the IRAM 30m telescope. The…

astro-ph1999★ 140 cited

The Scatter in the Relationship between Redshift and the Radio-to-Submm Spectral Index

C. L. Carilli, M. S. Yun

We derive the scatter in the relationship between redshift and radio-to-submm spectral index, alpha^{350}_{1.4}, using the observed spectral energy distributions of 17 low redshift…

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