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researcher

J. Pyo

3 papers hereh-index 141k citations123 works total

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

author position
  • middle author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO2
  • astro-ph.GA1
same name
  • J. Pyo — 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
20152017
most citedScience Impacts of the SPHEREx All-Sky Optical to Near-Infrared Spectral Survey: Report of a Community Workshop Examining Extragalactic, Galactic, Stellar and Planetary Science

41 citations · 69 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2017

Near-Infrared Polarimetric Study of N159/N160 Star-Forming Complex in the Large Magellanic Cloud

Jaeyeong Kim, Woong-Seob Jeong, Jeonghyun Pyo +4

We present near-infrared polarimetric results for N159/N160 star-forming complex, in the Large Magellanic Cloud (LMC) with SIRPOL, the polarimeter of the Infrared Survey Facility (…

astro-ph.CO2016★ 41 cited

Science Impacts of the SPHEREx All-Sky Optical to Near-Infrared Spectral Survey: Report of a Community Workshop Examining Extragalactic, Galactic, Stellar and Planetary Science

Olivier Doré, Michael W. Werner, Matt Ashby +65

SPHEREx is a proposed SMEX mission selected for Phase A. SPHEREx will carry out the first all-sky spectral survey and provide for every 6.2" pixel a spectra between 0.75 and 4.18 $…

astro-ph.CO2015★ 28 cited

AKARI Observation of the Sub-degree Scale Fluctuation of the Near-infrared Background

H. J. Seo, Hyung Mok Lee, T. Matsumoto +3

We report spatial fluctuation analysis of the sky brightness in near-infrared from observations toward the north ecliptic pole (NEP) by the AKARI at 2.4 and 3.2 micron. As a follow…

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