A
A. Mirhosseini
Publications - 7
Citations - 867
A. Mirhosseini is an academic researcher. The author has contributed to research in topics: Fast radio burst & Neutron star. The author has an hindex of 4, co-authored 4 publications receiving 579 citations.
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Journal ArticleDOI
A bright millisecond-duration radio burst from a Galactic magnetar
Chime,B. C. Andersen,Kevin Bandura,Mohit Bhardwaj,Akanksha Bij,M. M. Boyce,P. J. Boyle,C. Brar,T. Cassanelli,P. Chawla,T. Chen,J. F. Cliche,A. Cook,D. Cubranic,A. P. Curtin,Nolan Denman,M. A. Dobbs,F. Q. Dong,M. Fandino,Emmanuel Fonseca,Bryan Gaensler,U. Giri,Deborah C. Good,Mark Halpern,Alex S. Hill,Gary Hinshaw,C. Höfer,A. Josephy,J. W. Kania,V. M. Kaspi,T. L. Landecker,Calvin Leung,D. Z. Li,Hsiu-Hsien Lin,Kiyoshi Masui,R. Mckinven,J. Mena-Parra,M. Merryfield,B. W. Meyers,D. Michilli,N. Milutinovic,A. Mirhosseini,Moritz Münchmeyer,A. Naidu,Laura Newburgh,Cherry Ng,C. Patel,Ue-Li Pen,T. Pinsonneault-Marotte,Ziggy Pleunis,Brendan M. Quine,M. Rafiei-Ravandi,Mubdi Rahman,Scott M. Ransom,A. Renard,Pranav Sanghavi,Paul Scholz,J. R. Shaw,Kyung-Hoon Shin,Seth Siegel,Saranjit Singh,Rick Smegal,Kendrick M. Smith,Ingrid H. Stairs,C. M. Tan,Shriharsh P. Tendulkar,I. Tretyakov,Keith Vanderlinde,H. Wang,Dallas Wulf,A. V. Zwaniga +70 more
TL;DR: In this paper, the authors reported the detection of an extremely intense radio burst from the Galactic magnetar SGR 1935+2154 using the Canadian Hydrogen Intensity Mapping Experiment (CHIME) FRB project.
Journal ArticleDOI
Periodic activity from a fast radio burst source
Chime,M. Amiri,B. C. Andersen,Kevin Bandura,Mohit Bhardwaj,P. J. Boyle,Charanjot Brar,P. Chawla,T. Chen,J. F. Cliche,D. Cubranic,Meiling Deng,Nolan Denman,M. A. Dobbs,F. Q. Dong,M. Fandino,Emmanuel Fonseca,Bryan Gaensler,Utkarsh Giri,Deborah C. Good,Mark Halpern,Jason W. T. Hessels,Alex S. Hill,C. Höfer,A. Josephy,J. W. Kania,Ramesh Karuppusamy,Victoria M. Kaspi,A. Keimpema,F. Kirsten,T. L. Landecker,Dustin Lang,Calvin Leung,D. Z. Li,Hsiu-Hsien Lin,Benito Marcote,Kiyoshi Masui,R. Mckinven,J. Mena-Parra,M. Merryfield,Daniele Michilli,N. Milutinovic,A. Mirhosseini,A. Naidu,Laura Newburgh,Cherry Ng,K. Nimmo,Zsolt Paragi,C. Patel,Ue-Li Pen,T. Pinsonneault-Marotte,Ziggy Pleunis,M. Rafiei-Ravandi,Mubdi Rahman,Scott M. Ransom,A. Renard,P. Sanghavi,P. Scholz,J. R. Shaw,Kyung-Hoon Shin,S. R. Siegel,Saranjit Singh,Rick Smegal,Kendrick M. Smith,I. H. Stairs,Shriharsh P. Tendulkar,I. Tretyakov,K. Vanderlinde,H. Wang,X. Wang,Dallas Wulf,P. Yadav,A. V. Zwaniga +72 more
TL;DR: In this paper, the authors reported the detection of a $16.35\pm 0.15$ day periodicity (or possibly a higher-frequency alias of that periodicity) from a repeating fast radio burst (FRB) 180916.J0158+65 detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst Project (CHIME/FRB).
Journal ArticleDOI
Periodic activity from a fast radio burst source
M. Amiri,B. C. Andersen,Kevin Bandura,Mohit Bhardwaj,P. J. Boyle,Charanjot Brar,P. Chawla,T. Chen,J. F. Cliche,D. Cubranic,Meiling Deng,Nolan Denman,M. A. Dobbs,F. Q. Dong,M. Fandino,Emmanuel Fonseca,Bryan Gaensler,Utkarsh Giri,Deborah C. Good,Mark Halpern,Jason W. T. Hessels,Alex S. Hill,C. Höfer,A. Josephy,J. W. Kania,Ramesh Karuppusamy,Victoria M. Kaspi,A. Keimpema,F. Kirsten,T. L. Landecker,Dustin Lang,Calvin Leung,D. Z. Li,Hsiu-Hsien Lin,Benito Marcote,Kiyoshi Masui,R. Mckinven,J. Mena-Parra,M. Merryfield,Daniele Michilli,N. Milutinovic,A. Mirhosseini,A. Naidu,Laura Newburgh,Cherry Ng,K. Nimmo,Zsolt Paragi,C. Patel,Ue-Li Pen,T. Pinsonneault-Marotte,Ziggy Pleunis,M. Rafiei-Ravandi,Mubdi Rahman,Scott M. Ransom,A. Renard,P. Sanghavi,P. Scholz,J. R. Shaw,Kyung-Hoon Shin,S. R. Siegel,Saranjit Singh,Rick Smegal,Kendrick M. Smith,I. H. Stairs,Shriharsh P. Tendulkar,I. Tretyakov,K. Vanderlinde,H. Wang,X. Wang,Dallas Wulf,P. Yadav,A. V. Zwaniga +71 more
TL;DR: A periodicity of roughly 16 days is detected for the fast radio burst 180916.J0158+65, suggesting that the burst arises from a periodically modulated mechanism instead of a cataclysmic or sporadic process.
Journal ArticleDOI
A bright millisecond-duration radio burst from a Galactic magnetar
Chime,B. C. Andersen,Kevin Bandura,Mohit Bhardwaj,Akanksha Bij,M. M. Boyce,P. J. Boyle,C. Brar,T. Cassanelli,P. Chawla,T. Chen,J. F. Cliche,A. Cook,D. Cubranic,A. P. Curtin,Nolan Denman,M. A. Dobbs,F. Q. Dong,M. Fandino,Emmanuel Fonseca,Bryan Gaensler,U. Giri,Deborah C. Good,Mark Halpern,Alex S. Hill,Gary Hinshaw,C. Höfer,A. Josephy,J. W. Kania,V. M. Kaspi,T. L. Landecker,Calvin Leung,D. Z. Li,Hsiu-Hsien Lin,Kiyoshi Masui,R. Mckinven,J. Mena-Parra,M. Merryfield,B. W. Meyers,D. Michilli,N. Milutinovic,A. Mirhosseini,Moritz Münchmeyer,A. Naidu,Laura Newburgh,Cherry Ng,C. Patel,Ue-Li Pen,T. Pinsonneault-Marotte,Ziggy Pleunis,Brendan M. Quine,M. Rafiei-Ravandi,Mubdi Rahman,Scott M. Ransom,A. Renard,Pranav Sanghavi,Paul Scholz,J. R. Shaw,Kyung-Hoon Shin,Seth Siegel,Saranjit Singh,Rick Smegal,Kendrick M. Smith,Ingrid H. Stairs,C. M. Tan,Shriharsh P. Tendulkar,I. Tretyakov,Keith Vanderlinde,H. Wang,Dallas Wulf,A. V. Zwaniga +70 more
TL;DR: The detection of an extremely intense radio burst from the Galactic magnetar SGR 1935+2154 using the Canadian Hydrogen Intensity Mapping Experiment (CHIME) FRB project implies a burst energy at 400 to 800 megahertz of approximately 3 × 1034 erg, which is three orders of magnitude higher than the burst energy of any radio-emitting magnetar detected thus far.
Journal ArticleDOI
An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment
Mandana Amiri,Kevin Bandura,Ana Bošković,Tian-Lu Chen,J. F. Cliche,Meiling Deng,Nolan Denman,Matt Dobbs,M. Fandino,Simon Foreman,Mark Halpern,D. S. Hanna,Alex S. Hill,Gary Hinshaw,C. Höfer,Joseph Kania,P. Klages,T. L. Landecker,J. MacEachern,Kiyoshi Masui,J. Mena-Parra,N. Milutinovic,A. Mirhosseini,Laura Newburgh,Rick Nitsche,A. Ordog,Ue Li Pen,T. Pinsonneault-Marotte,Ava Polzin,Ali Reda,A. Renard,J. Richard Shaw,Seth Siegel,Saurabh Singh,Rick Smegal,I. Tretyakov,Kwinten Van Gassen,K. Vanderlinde,Haochen Wang,D. V. Wiebe,James S. Willis,Dallas Wulf +41 more
TL;DR: The Canadian Hydrogen Intensity Mapping Experiment (CHIME) as discussed by the authors is a drift scan radio telescope operating across the 400-800 MHz band with a 256-element dual-polarization linear feed array.