Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Donggeun Tak"'
Autor:
Z. Lucas Uhm, Donggeun Tak, Bing Zhang, Judith Racusin, Daniel Kocevski, Sylvain Guiriec, Bin-Bin Zhang, Julie McEnery
Publikováno v:
The Astrophysical Journal Letters, Vol 963, Iss 1, p L30 (2024)
One of the difficulties in nailing down the physical mechanism of gamma-ray bursts (GRBs) comes from the fact that there has been no clear observational evidence on how far from the central engine the prompt gamma rays of GRBs are emitted. Here we pr
Externí odkaz:
https://doaj.org/article/30a2d257c9fb4e3491a06debb8b0fb0d
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 1, p 54 (2024)
A kilonova, the electromagnetic emission produced by compact binary mergers, is formed through a delicate interplay of physical processes, involving r -process nucleosynthesis and interactions between heavy elements and photons through radiative tran
Externí odkaz:
https://doaj.org/article/3c8560c8d5ef4d1c9a41440be60ce8a2
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 2, p 121 (2023)
A kilonova is a short-lived explosive event in the Universe, resulting from the merger of two compact objects. Despite its importance as a primary source of heavy elements through r -process nucleosynthesis, its nature is not well understood due to i
Externí odkaz:
https://doaj.org/article/9ee4e82af81049eb828c50cdbd540d43
Autor:
Donggeun Tak, Z. Lucas Uhm, Judith Racusin, Bing Zhang, Sylvain Guiriec, Daniel Kocevski, Bin-Bin Zhang, Julie McEnery
Publikováno v:
The Astrophysical Journal, Vol 949, Iss 2, p 110 (2023)
We perform a detailed analysis of broad pulses in bright gamma-ray bursts (GRBs) to understand the evolution of GRB broad pulses. Using the temporal and spectral properties, we test the high-latitude emission (HLE) scenario in the decaying phase of b
Externí odkaz:
https://doaj.org/article/ea11f5d0a6404ebab162553895253a1b
Multiwavelength observation of the gamma-ray burst, GRB 190114C, opens a new window for studying the emission mechanism of GRB afterglows. Its very high energy (VHE; ≳ 100 GeV) detection has motivated an inverse Compton interpretation for the emiss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4dedf7dc20b70451b85c8442ccba8356
https://bib-pubdb1.desy.de/record/479853
https://bib-pubdb1.desy.de/record/479853
Autor:
Regina Caputo, Marco Ajello, Carolyn A. Kierans, Jeremy S. Perkins, Judith L. Racusin, Luca Baldini, Matthew G. Baring, Elisabetta Bissaldi, Eric Burns, Nicholas Cannady, Eric Charles, Rui M. Curado da Silva, Ke Fang, Henrike Fleischhack, Chris Fryer, Yasushi Fukazawa, J. Eric Grove, Dieter Hartmann, Eric J. Howell, Manoj Jadhav, Christopher M. Karwin, Daniel Kocevski, Naoko Kurahashi, Luca Latronico, Tiffany R. Lewis, Richard Leys, Amy Lien, Lea Marcotulli, Israel Martinez-Castellanos, Mario Nicola Mazziotta, Julie McEnery, Jessica Metcalfe, Kohta Murase, Michela Negro, Lucas Parker, Bernard Phlips, Chanda Prescod-Weinstein, Soebur Razzaque, Peter S. Shawhan, Yong Sheng, Tom A. Shutt, Daniel Shy, Clio Sleator, Amanda L. Steinhebel, Nicolas Striebig, Yusuke Suda, Donggeun Tak, Hiro Tajima, Janeth Valverde, Tonia M. Venters, Zorawar Wadiasingh, Richard S. Woolf, Eric A. Wulf, Haocheng Zhang, Andreas Zoglauer
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::774309717fe565cc93412713c6c14b43
https://hdl.handle.net/11589/251023
https://hdl.handle.net/11589/251023
Autor:
Matthew Lundy, A. Brill, M. Capasso, Hugh Dickinson, Manel Errando, T. J. Williamson, S. Kumar, S. Patel, Vladimir Vassiliev, M. J. Lang, David Hanna, P. Moriarty, John L. Quinn, Orel Gueta, donggeun tak, David A. Williams, Michael Laraia, Sameer Patel, Jodi Christiansen, P. Wilcox, Thomas Brian Humensky, C. E. McGrath, Alasdair E. Gent, R.R. Prado, Avery Archer, K. Ragan, M. Kertzman, C. Adams, M. Nievas-Rosillo, J. H. Buckley, Reshmi Mukherjee, David Kieda, Tobias Kleiner, A. J. Chromey, A. D. Falcone, Philip Kaaret, James M. Ryan, Wystan Benbow, Lucy Fortson, A. N. Otte, R. A. Ong, C. Giuri, K. A. Farrell, G. M. Foote, Deivid Ribeiro, Stephen Serjeant, E. Roache, Martin Pohl, Binita Hona, Jamie Holder, G. H. Sembroski, Daniel Nieto, K. Pfrang, S. O'Brien, Kevin Flanagan, Amanda Weinstein, Gary Gillanders, Marcos Santander, Q. Feng, I. Sadeh, Darryl Wright, R. Shang, W. Jin, Olivier Hervet, Gernot Maier, P. T. Reynolds, Amy Furniss, E. Pueschel
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Muons from extensive air showers appear as rings in images taken with imaging atmospheric Cherenkov telescopes, such as VERITAS. These muon-ring images are used for the calibration of the VERITAS telescopes, however the calibration accuracy can be im
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::92318da11a79a96607b5d5e0132dabf2
https://doi.org/10.22323/1.395.0766
https://doi.org/10.22323/1.395.0766
Autor:
Matthew Lundy, Massimo Capasso, Rene Ong, Iftach Sadeh, Philip Kaaret, Weidong Jin, Wystan Benbow, Reshmi Mukherjee, Raul Prado, Sameer Patel, Patrick Moriarty, Gernot Maier, Amy Furniss, Ken Ragan, David Williams, James Buckley, Lucy Fortson, John Quinn, Jamie Holder, Chiara Giuri, Elisa Pueschel, Daniel Nieto, Colin Adams, Stephan O'Brien, Deivid Ribeiro, Konstantin Pfrang, Orel Gueta, Gregory M Foote, Amanda Weinstein, Sajan Kumar, Tyler Williamson, Donggeun Tak, Conor McGrath, Tobias Kai Kleiner, Martin Pohl, Paul Reynolds, Binita Hona, David Hanna, Marcos Santander, Glenn Sembroski, Sonal Ramesh Patel, Manel Errando, Mary Kertzman, Olivier Hervet, Mireia Nievas-Rosillo, Mark Lang, Emmet Roache, Thomas Brian Humensky, Ruo-Yu Shang, Vladimir Vassiliev, Alisha Chromey, Abe Falcone, Jodi Christiansen, Adam Otte, Alasdair E. Gent, Aryeh Brill, James Ryan, Kayla Farrell, Gary Gillanders, Qi Feng, Avery Archer, David Kieda
1A 0535+262 is a Be X-ray binary pulsar and one of the only galactic pulsar systems to show radio jet emission. Characterizing the very high energy emission (VHE, >100 GeV) in these extreme microquasars is critical to understanding their contribution
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::771e08a45d506651e0c7b10ebeea96a0
http://arxiv.org/abs/2108.09350
http://arxiv.org/abs/2108.09350
Autor:
Matthew Lundy, Massimo Capasso, Rene Ong, Iftach Sadeh, Philip Kaaret, Weidong Jin, Wystan Benbow, Reshmi Mukherjee, Raul Prado, Sameer Patel, Patrick Moriarty, Gernot Maier, Amy Furniss, Ken Ragan, David Williams, James Buckley, Lucy Fortson, John Quinn, Jamie Holder, Chiara Giuri, Elisa Pueschel, Daniel Nieto, Colin Adams, Stephan O'Brien, Deivid Ribeiro, Konstantin Pfrang, Orel Gueta, Gregory M Foote, Amanda Weinstein, Sajan Kumar, Tyler Williamson, Donggeun Tak, Conor McGrath, Tobias Kai Kleiner, Martin Pohl, Paul Reynolds, Binita Hona, David Hanna, Marcos Santander, Glenn Sembroski, Sonal Ramesh Patel, Manel Errando, Mary Kertzman, Olivier Hervet, Mireia Nievas-Rosillo, Mark Lang, Emmet Roache, Thomas Brian Humensky, Ruo-Yu Shang, Vladimir Vassiliev, Alisha Chromey, Abe Falcone, Jodi Christiansen, Adam Otte, Alasdair E. Gent, Aryeh Brill, James Ryan, Kayla Farrell, Gary Gillanders, Qi Feng, Avery Archer, David Kieda
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Fast radio burst (FRBs) are an exciting class of bright, extragalactic, millisecond radio transients. The recent development of large field-of-view (FOV) radio telescopes has caused a rapid rise in the number of identified single burst and repeating
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::65145672b8d6d892e7c01740dbedb843
https://doi.org/10.22323/1.395.0857
https://doi.org/10.22323/1.395.0857
Autor:
David R. Williams, Antoine Kouchner, K. A. Farrell, Alasdair E. Gent, V. V. Vassiliev, Fabian Schüssler, H. A. Peña-Herazo, Georgios Paraschos, R. Shang, D. S. Hanna, Q. Feng, John L. Quinn, D. Ribeiro, Daniel Nieto, A. Brill, Giacomo Bonnoli, M. Kertzman, Lucy Fortson, Yong Sheng, Olivier Hervet, T. B. Humensky, Francesco Massaro, S. O'Brien, Alessio Berti, M. J. Lang, donggeun tak, Teddy Cheung, Suvi Gezari, Joern Wilms, A. D. Falcone, P. T. Reynolds, Miguel Perez-Torres, Andrea Tramacere, Reshmi Mukherjee, G. M. Foote, Binita Hona, C. Giuri, Raniere de Menezes, P. Kaaret, I. Sadeh, Frank J. Masci, Emilio Fernandez-Garcia, W. Jin, Wystan Benbow, Uwe Bach, R. R. Prado, P. Moriarty, Jonas Heßdörfer, M. Pohl, Matthias Kadler, Steven Hämmerich, Gernot Maier, G. H. Sembroski, Andrea Gokus, R. A. Ong, M. Capasso, Ivan Agudo, Marcos Santander, C. E. McGrath, T. J. Williamson, A. J.R. Weinstein, E. Roache, A. Archer, Jorge Otero-Santos, Simone Garrappa, Alex Kraus, G. H. Gillanders, A. J. Castro-Tirado, Alexis Coleiro, Jodi Christiansen, Jamie Holder, K. Ragan, Meenakshi Rajagopal, A. N. Otte, Alessandro Paggi, K. Pfrang, Orel Gueta, Marcello Giroletti, Cristina Nanci, Javier Moldon, M. Nievas-Rosillo, Elisa Bernardini, C. Adams, Werner Colmar, Y. D. Hu, J. A. Ryan, Richard Walters, M. Lundy, Florian Eppel, Tobias Kleiner, R. Sanchez-Ramirez, J. H. Buckley, A. J. Chromey, Amy Furniss, Charlotte Ward, Konstancja Satalecka, E. Pueschel, Manel Errando, Sara Buson, S. Kumar, S. Patel, M. D. Caballero-Garcia, Marco Ajello
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0df37b57919dd1c2b11ee5153ecb2af5
https://doi.org/10.22323/1.395.0955
https://doi.org/10.22323/1.395.0955