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Jeonghee Rho

19 papers hereh-index 151.3k citations31 works total

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

author position
  • first author2
  • middle author15
  • last author1

Across the 18 of 19 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE12
  • astro-ph3
  • astro-ph.GA2
  • astro-ph.SR2
same name
  • Jeonghee Rho — 1 paper

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
20022026
most citedAbsolute Calibration and Characterization of the Multiband Imaging Photometer for Spitzer. I. The Stellar Calibrator Sample and the 24 micron Calibration

313 citations · 641 across the 18 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.SR2020★ 62 cited

Near-Infrared and Optical Observations of Type Ic SN2020oi and broad-lined Ic SN2020bvc: Carbon Monoxide, Dust and High-Velocity Supernova Ejecta

J. Rho, A. Evans, T. R. Geballe +33

We present near-infrared and optical observations of the Type Ic Supernova (SN) 2020oi in the galaxy M100 and the broad-lined Type Ic SN2020bvc in UGC 9379, using Gemini, LCO, SOAR…

astro-ph.GA2020★ 7 cited

A Galactic Dust Devil: far-infrared observations of the Tornado Supernova Remnant candidate

Hannah Chawner, Alex D. P. Howard, Haley L. Gomez +10

We present complicated dust structures within multiple regions of the candidate supernova remnant (SNR) the `Tornado' (G357.7-0.1) using observations with Spitzer and Herschel. We…

astro-ph.GA2020★ 27 cited

A Complete Catalogue of Dusty Supernova Remnants

Hannah Chawner, Haley Gomez, Mikako Matsuura +9

We search for far-infrared (FIR) counterparts of known supernova remnants (SNRs) in the Galactic plane (360 degrees in longitude and b = +/- 1 deg ) at 70 - 500 micron with Hersche…

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