J
John F. Beacom
Researcher at Ohio State University
Publications - 359
Citations - 28360
John F. Beacom is an academic researcher from Ohio State University. The author has contributed to research in topics: Neutrino & Supernova. The author has an hindex of 80, co-authored 338 publications receiving 24601 citations. Previous affiliations of John F. Beacom include Fermilab & University of Wisconsin-Madison.
Papers
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Journal ArticleDOI
On the Normalization of the Cosmic Star Formation History
Andrew M. Hopkins,John F. Beacom +1 more
TL;DR: In this article, the authors investigate the sequence of assumptions and corrections that together affect the cosmic star formation history (SFH) normalization to test their accuracy, both in this redshift range and beyond.
Journal ArticleDOI
On the normalisation of the cosmic star formation history
Andrew M. Hopkins,John F. Beacom +1 more
TL;DR: In this article, strong constraints on the cosmic star formation history (SFH) have been established using ultraviolet and far-infrared measurements, refining the results of numerous measurements over the past decade.
Journal ArticleDOI
The man behind the curtain: x-rays drive the uv through nir variability in the 2013 active galactic nucleus outburst in ngc 2617
Benjamin J. Shappee,J. L. Prieto,Dirk Grupe,Christopher S. Kochanek,Krzysztof Z. Stanek,G. De Rosa,Smita Mathur,Ying Zu,Bradley M. Peterson,Richard W. Pogge,Stefanie Komossa,Myungshin Im,Jacob Jencson,T W-S Holoien,U. Basu,John F. Beacom,D. M. Szczygiel,Joseph Brimacombe,Scott M. Adams,Abdo Campillay,Changsu Choi,Carlos Contreras,M. Dietrich,M. Dubberley,M. Elphick,S. Foale,Margherita Giustini,C. Gonzalez,E. Hawkins,D. A. Howell,D. A. Howell,Eric Hsiao,Michael Koss,Karen M. Leighly,Nidia Morrell,D. Mudd,D. Mullins,Jenna M. Nugent,J. Parrent,Mark M. Phillips,G. Pojmanski,Wayne Rosing,R. Ross,David J. Sand,Donald M. Terndrup,Stefano Valenti,Stefano Valenti,Z. Walker,Yosep Yoon +48 more
TL;DR: In this article, the authors reported that NGC 2617 went through a dramatic outburst, during which its X-ray flux increased by over an order of magnitude followed by an increase of its optical/ultraviolet (UV) continuum flux.
Journal ArticleDOI
The Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617
Benjamin J. Shappee,J. L. Prieto,Dirk Grupe,Christopher S. Kochanek,K. Z. Stanek,G. De Rosa,S. Mathur,Ying Zu,Bradley M. Peterson,R. W. Pogge,S. Komossa,Myungshin Im,J. E. Jencson,T W-S Holoien,U. Basu,John F. Beacom,D. M. Szczygiel,Joseph Brimacombe,Scott M. Adams,A. Campillay,Changsu Choi,C. Contreras,M. Dietrich,M. Dubberley,M. Elphick,S. Foale,Margherita Giustini,C. Gonzalez,E. Hawkins,D. A. Howell,Eric Hsiao,Michael Koss,Karen M. Leighly,N. I. Morrell,D. Mudd,D. Mullins,Jenna M. Nugent,J. T. Parrent,M. M. Phillips,G. Pojmanski,Wayne Rosing,R. Ross,David J. Sand,Donald M. Terndrup,S. Valenti,Z. Walker,Yosep Yoon +46 more
TL;DR: In this article, the authors reported that NGC 2617 went through a dramatic outburst, during which its X-ray flux increased by over an order of magnitude followed by an increase of its optical/ultraviolet (UV) continuum flux.
Journal ArticleDOI
Neutrino Physics with JUNO
Fengpeng An,Guangpeng An,Qi An,Vito Antonelli,Eric Baussan,John F. Beacom,L. B. Bezrukov,Simon Blyth,R. Brugnera,Margherita Buizza Avanzini,Jose Busto,Anatael Cabrera,Hao Cai,Xiao Cai,Antonio Cammi,Guofu Cao,Jun Cao,Yun Chang,Shaomin Chen,S. M. Chen,Yi Chen,Davide Chiesa,Massimiliano Clemenza,Barbara Clerbaux,Janet Conrad,D. D'Angelo,Herve De Kerret,Zhi Deng,Ziyan Deng,Yayun Ding,Zelimir Djurcic,Damien Dornic,Marcos Dracos,O. Drapier,S. Dusini,Stephen T. Dye,Timo Enqvist,Donghua Fan,Jian Fang,Laurent Favart,Richard Ford,M. Göger-Neff,Haonan Gan,A. Garfagnini,Marco Giammarchi,Maxim Gonchar,Guanghua Gong,Hui Gong,M. Gonin,Marco Grassi,Christian Grewing,Mengyun Guan,Vic Guarino,Gang Guo,Wanlei Guo,Xin Heng Guo,Caren Hagner,Ran Han,Miao He,Yuekun Heng,Y. B. Hsiung,Jun Hu,Shouyang Hu,Tao Hu,Hanxiong Huang,Xingtao Huang,Lei Huo,Ara Ioannisian,Manfred Jeitler,Xiangdong Ji,Xiaoshan Jiang,Cécile Jollet,Li Kang,Michael Karagounis,Narine Kazarian,Z. V. Krumshteyn,Andre Kruth,Pasi Kuusiniemi,Tobias Lachenmaier,Rupert Leitner,Chao Li,Jiaxing Li,Wei Li,Weiguo Li,Xiaomei Li,X. N. Li,Yi Li,Yufeng Li,Zhibing Li,Hao Liang,Guey-Lin Lin,Tao Lin,Yen-Hsun Lin,Jiajie Ling,Jiajie Ling,Ivano Lippi,D. W. Liu,Hongbang Liu,Hu Liu,Jianglai Liu,Jianli Liu,Jinchang Liu,Qian Liu,Shubin Liu,Shulin Liu,Paolo Lombardi,Yongbing Long,Haoqi Lu,J. G. Lu,Jingbin Lu,Junguang Lu,Bayarto Lubsandorzhiev,Livia Ludhova,Shu Luo,Vladimir Lyashuk,R. Möllenberg,Xubo Ma,Fabio Mantovani,Yajun Mao,Stefano Maria Mari,William F. McDonough,G. Meng,Anselmo Meregaglia,E. Meroni,Mauro Mezzetto,Lino Miramonti,Thomas Mueller,Dmitry V. Naumov,Lothar Oberauer,Juan Pedro Ochoa-Ricoux,Alexander Olshevskiy,Fausto Ortica,Alessandro Paoloni,H. Peng,Jen-Chieh Peng,Ezio Previtali,Ming Qi,Sen Qian,Xin Qian,Yong Zhong Qian,Yong Zhong Qian,Zhonghua Qin,Georg G. Raffelt,Gioacchino Ranucci,Barbara Ricci,Markus Robens,Aldo Romani,Xiangdong Ruan,Xichao Ruan,G. Salamanna,M. H. Shaevitz,V. V. Sinev,Chiara Sirignano,Monica Sisti,Oleg Smirnov,M. Soiron,Achim Stahl,Luca Stanco,Jochen Steinmann,Xilei Sun,Yongjie Sun,Dmitriy Taichenachev,Jian Tang,Igor Tkachev,Wladyslaw Henryk Trzaska,Stefan van Waasen,Cristina Volpe,V. Vorobel,Lucia Votano,Chung Hsiang Wang,Guo-Li Wang,Hao Wang,Meng Wang,Ruiguang Wang,Siguang Wang,Wei Wang,Yi Wang,Yi Wang,Yifang Wang,Zhe Wang,Zheng Wang,Zheng Wang,Zhimin Wang,Wei Wei,Liangjian Wen,Christopher Wiebusch,Björn Wonsak,Qun Wu,Claudia-Elisabeth Wulz,Michael Wurm,Yufei Xi,Dongmei Xia,Yuguang Xie,Zhi-zhong Xing,Jilei Xu,Baojun Yan,Changgen Yang,C. G. Yang,Guang Yang,Lei Yang,Yifan Yang,Yu Yao,Ugur Yegin,F. Yermia,Zhengyun You,Boxiang Yu,Chunxu Yu,Zeyuan Yu,Sandra Zavatarelli,Liang Zhan,Chao Zhang,Honghao Zhang,Jiawen Zhang,Jingbo Zhang,Qingmin Zhang,Yumei Zhang,Zhenyu Zhang,Zhenghua Zhao,Yangheng Zheng,Weili Zhong,Guorong Zhou,Jing Zhou,Li Zhou,Rong Zhou,Shun Zhou,Wenxiong Zhou,Xiang Zhou,Ye-Ling Zhou,Y. H. Zhou,Jiaheng Zou +229 more
TL;DR: The Jiangmen Underground Neutrino Observatory (JUNO) as mentioned in this paper is a 20kton multi-purpose underground liquid scintillator detector with the determination of neutrino mass hierarchy (MH) as a primary physics goal.