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researcher

B. Koo

90 papers hereh-index 344k citations260 works total

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

author position
  • sole author1
  • first author20
  • middle author54
  • last author13

Across the 88 of 90 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA43
  • astro-ph29
  • astro-ph.HE11
  • astro-ph.SR5
  • astro-ph.CO2
same name
  • B. Koo — 15 papers, h 6
  • B. Koo — 6 papers, h 9
  • B. Koo — 3 papers, h 35
  • B. Koo — 2 papers, h 7
  • B. Koo — 1 paper, h 7
  • B. Koo — 1 paper, h 8

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
19992023
most citedThe Infrared Astronomical Mission AKARI

842 citations · 3.1k across the 89 of their papers we have counts for

collaborators
Showing 2009 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2009★ 70 cited

AKARI and BLAST Observations of the Cassiopeia A Supernova Remnant and Surrounding Interstellar Medium

B. Sibthorpe, P. A. R. Ade, J. J. Bock +30

We use new large area far infrared maps ranging from 65 - 500 microns obtained with the AKARI and the Balloon-borne Large Aperture Submillimeter Telescope (BLAST) missions to chara…

astro-ph.HE2009★ 8 cited

Infrared Studies of Molecular Shocks in the Supernova Remnant HB 21: II. Thermal Admixture of Shocked H2​ Gas in the South

Jong-Ho Shinn, Bon-Chul Koo, Michael G. Burton +2

We present near- and mid-infrared observations on the shock-cloud interaction region in the southern part of the supernova remnant HB 21, performed with the InfraRed Camera (IRC) a…

astro-ph.HE2009★ 21 cited

Dense Iron Ejecta and Core-collapse Supernova Explosion in the Young Supernova Remnant G11.2-0.3

Dae-Sik Moon, Bon-Chul Koo, Ho-Gyu Lee +5

We present the results of near-infrared spectroscopic observations of dense ($\simgt$ 103 cm−3) iron ejecta in the young core-collapse supernova remnant G11.2-0.3. Five eje…

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