activity
20062018
most citedThe SPEAR Instrument and On-Orbit Performance

63 citations · 258 across the 13 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2018★ 5 cited

MIRIS Paα Galactic Plane Survey. I. Comparison with IPHAS Hα in l = 96°-116°

Il-Joong Kim, Jeonghyun Pyo, Woong-Seob Jeong +11

The Multipurpose InfraRed Imaging System (MIRIS) performed the MIRIS Paα Galactic Plane Survey (MIPAPS), which covers the entire Galactic plane within the latitude range of -3° < b…

astro-ph.GA2018★ 16 cited

MIRIS observation of near-infrared diffuse Galactic light

Y. Onishi, K. Sano, S. Matsuura +17

We report near-infrared (IR) observations of high Galactic latitude clouds to investigate diffuse Galactic light (DGL), which is starlight scattered by interstellar dust grains. Th…

astro-ph.GA2016★ 6 cited

Radiative transfer in disc galaxies V. The accuracy of the KB approximation

Dukhang Lee, Maarten Baes, Kwang-Il Seon +3

We investigate the accuracy of an approximate radiative transfer technique that was first proposed by Kylafis & Bahcall (hereafter the KB approximation) and has been popular in mod…

astro-ph.GA2011

Implications of the SPEAR FUV Maps on Our Understanding of the ISM

Eric J. Korpela, Martin Sirk, Jerry Edelstein +3

The distribution of a low-density transition temperature (10^4.5 - 10^5.5 K) gas in the interstellar medium conveys the character and evolution of diffuse matter in the Galaxy. Thi…

astro-ph.GA2010★ 4 cited

Far-ultraviolet Emission-line Morphologies of the Supernova Remnant G65.3+5.7

I. -J. Kim, K. -I. Seon, K. -W. Min +3

We present the first far-ultraviolet (FUV) emission-line morphologies of the whole region of the supernova remnant (SNR) G65.3+5.7 using the FIMS/SPEAR data. The morphologies of th…

astro-ph.SR2010★ 15 cited

Analysis of Spatial Structure of the SPica H II Region

J. -W. Park, K. -W. Min, K. -I. Seon +2

Far ultraviolet (FUV) spectral images of the Spica H II region are first presented here for the Si II* 1533.4A and Al II 1670.8A lines and then compared with the optical Halpha ima…