J
Jong-Hak Woo
Researcher at Seoul National University
Publications - 268
Citations - 17937
Jong-Hak Woo is an academic researcher from Seoul National University. The author has contributed to research in topics: Galaxy & Active galactic nucleus. The author has an hindex of 68, co-authored 257 publications receiving 16466 citations. Previous affiliations of Jong-Hak Woo include Southern Nazarene University & National Science Foundation.
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Journal ArticleDOI
Y 2 Isochrones with an Improved Core Overshoot Treatment
TL;DR: In this article, the authors provide a patch to the Y2 isochrones with an improved treatment of convective core overshoot, which covers the transition mass range from no convective cores to a fully developed core.
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Active Galactic Nucleus Black Hole Masses and Bolometric Luminosities
Jong-Hak Woo,C. Megan Urry +1 more
TL;DR: In this paper, the authors collected and compared all AGN black hole mass estimates from the literature; these 177 masses are mostly based on the virial assumption for the broad emission lines, with the broad-line region size determined from either reverberation mapping or optical luminosity.
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The Low-luminosity End of the Radius-Luminosity Relationship for Active Galactic Nuclei
Misty C. Bentz,Kelly D. Denney,Catherine J. Grier,Aaron J. Barth,Bradley M. Peterson,Marianne Vestergaard,Marianne Vestergaard,Vardha N. Bennert,Gabriela Canalizo,Gisella De Rosa,Alexei V. Filippenko,Elinor L. Gates,Jenny E. Greene,Weidong Li,Matthew A. Malkan,Richard W. Pogge,Daniel Stern,Tommaso Treu,Jong-Hak Woo +18 more
TL;DR: In this article, the authors present an updated and revised analysis of the relationship between the H{beta} broadline region (BLR) radius and the luminosity of the active galactic nucleus (AGN).
Journal ArticleDOI
AGN Black Hole Masses and Bolometric Luminosities
Jong-Hak Woo,C. Megan Urry +1 more
TL;DR: In this paper, the authors collected and compared all AGN black hole mass estimates from the literature; these 177 masses are mostly based on the virial assumption for the broad emission lines, with the broad-line region size determined from either reverberation mapping or optical luminosity.
Journal ArticleDOI
The lick agn monitoring project: Broad-line region radii and black hole masses from reverberation mapping of Hβ
Misty C. Bentz,Jonelle L. Walsh,Aaron J. Barth,Nairn Baliber,Nairn Baliber,Vardha N. Bennert,Vardha N. Bennert,Gabriela Canalizo,Alexei V. Filippenko,Mohan Ganeshalingam,Elinor L. Gates,Jenny E. Greene,Jenny E. Greene,M. G. Hidas,M. G. Hidas,M. G. Hidas,Kyle D. Hiner,Nicholas Lee,Weidong Li,Matthew A. Malkan,Takeo Minezaki,Yu Sakata,Frank J. D. Serduke,Jeffrey M. Silverman,Thea N. Steele,Daniel Stern,Rachel Street,Rachel Street,Carol E. Thornton,Tommaso Treu,Tommaso Treu,Xiaofeng Wang,Xiaofeng Wang,Jong-Hak Woo,Jong-Hak Woo,Yuzuru Yoshii +35 more
TL;DR: In this paper, a 64-night spectroscopic monitoring campaign at the Lick Observatory 3m Shane telescope with the aim of measuring the masses of the black holes in 12 nearby (z < 0: 05) Seyfert 1 galaxies with expected masses in the range of 10 6 -10 7, and also the well-studied nearby active galactic nucleus (AGN) NGC 5548.