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Young-Beom Jeon
Researcher at Seoul National University
Publications - 39
Citations - 653
Young-Beom Jeon is an academic researcher from Seoul National University. The author has contributed to research in topics: Stars & Globular cluster. The author has an hindex of 16, co-authored 39 publications receiving 622 citations. Previous affiliations of Young-Beom Jeon include Korea Astronomy and Space Science Institute.
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Journal ArticleDOI
The Earliest Near-infrared Time-series Spectroscopy of a Type Ia Supernova
Eric Hsiao,G. H. Marion,Mark M. Phillips,Christopher R. Burns,Claudia Winge,Nidia Morrell,Carlos Contreras,Wendy L. Freedman,Markus Kromer,E. E. E. Gall,Christopher L. Gerardy,P. Höflich,Myungshin Im,Young-Beom Jeon,Robert P. Kirshner,Peter Nugent,Peter Nugent,S. E. Persson,Giuliano Pignata,M. Roth,Vallery Stanishev,Maximilian Stritzinger,Nicholas B. Suntzeff +22 more
TL;DR: In this paper, the authors presented ten medium-resolution, high signal-to-noise ratio near-infrared (NIR) spectra of SN?2011fe from SpeX on the NASA Infrared Telescope Facility (IRTF) and Gemini Near-Infrared Spectrograph (GNIRS) on Gemini North, obtained as part of the Carnegie Supernova Project.
Journal ArticleDOI
The Earliest Near-infrared Time-series Spectroscopy of a Type Ia Supernova
Eric Hsiao,G. H. Marion,Mark M. Phillips,Christopher R. Burns,Claudia Winge,N. I. Morrell,C. Contreras,Wendy L. Freedman,M. Kromer,E. E. E. Gall,Christopher L. Gerardy,P. Hoeflich,Myungshin Im,Young-Beom Jeon,R. P. Kirshner,Peter Nugent,S. E. Persson,Giuliano Pignata,M. Roth,Vallery Stanishev,Maximilian Stritzinger,N. B. Suntzeff +21 more
TL;DR: In this article, the authors presented ten medium-resolution, high signal-to-noise ratio near-infrared (NIR) spectra of SN 2011fe from SpeX on the NASA Infrared Telescope Facility (IRTF) and Gemini Near-Infrared Spectrograph (GNIRS) on Gemini North, obtained as part of the Carnegie Supernova Project.
Journal ArticleDOI
SX Phoenicis Stars in the Globular Cluster NGC 5466
TL;DR: Using time-series CCD photometry of the globular cluster NGC 5466, Zhang et al. as discussed by the authors detected nine SX Phoenicis stars, including three new ones.
Journal ArticleDOI
Around-the-Clock Observations of the Q0957+561A,B Gravitationally Lensed Quasar. II. Results for the Second Observing Season
Wesley N. Colley,Rudolph E. Schild,C. Abajas,D. Alcalde,Zeki Aslan,I. F. Bikmaev,V. H. Chavushyan,Luis Chinarro,Jean-Philippe Cournoyer,R. Crowe,V. N. Dudinov,Anna Evans,Young-Beom Jeon,Luis J. Goicoechea,Orhan Golbasi,Irek Khamitov,Kjetil Kjernsmo,Hyun Ju Lee,Jong Hwan Lee,Ki-Won Lee,Myung Gyoon Lee,Omar Lopez-Cruz,Omar Lopez-Cruz,Omar Lopez-Cruz,Evencio Mediavilla,Anthony F. J. Moffat,Raúl Mújica,A. Ullán,Jose F. Muñoz,A. Oscoz,Myeong-Gu Park,Norman Purves,Oyvind Saanum,N. A. Sakhibullin,Miquel Serra-Ricart,Igor Sinelnikov,R. Stabell,Alan Stockton,J. Teuber,Roy Thompson,Hwa-Sung Woo,A. P. Zheleznyak +41 more
TL;DR: In this article, the brightness of the later arriving Q0957+561B image was compared with the previously published brightness observations of the first-arriving) A image, and the authors found a 417.09 ± 0.07 day time delay.
Journal ArticleDOI
Around the Clock Observations of the Q0957+561 A,B Gravitationally Lensed Quasar II: Results for the second observing season
Wesley N. Colley,Rudolph E. Schild,C. Abajas,D. Alcalde,Zeki Aslan,Zeki Aslan,I. F. Bikmaev,V. H. Chavushyan,Luis Chinarro,Jean-Philippe Cournoyer,R. Crowe,V. N. Dudinov,Anna Kathinka,Dalland Evans,Young-Beom Jeon,Luis J. Goicoechea,Orhan Golbasi,I. M. Khamitov,Kjetil Kjernsmo,Hyun Ju Lee,Jong Hwan Lee,Ki-Won Lee,Ki-Won Lee,Myung Gyoon Lee,Omar Lopez-Cruz,Omar Lopez-Cruz,Evencio Mediavilla,Anthony F.J. Moffatt,Raúl Mújica,A. Ullán,A. Oscoz,Myeong-Gu Park,Norman G. Purves,N. A. Sakhibullin,Igor Sinelnikov,R. Stabell,Alan Stockton,J. Teuber,Roy Thompson,Hwa-Sung Woo,A. P. Zheleznyak +40 more
TL;DR: In this article, the brightness of the later arriving Q0957+561 B image was compared with the previously published brightness observations of the (first arriving) A image, and it was shown that the structure function is statistically non-stationary.