A
A. P. Curtin
Publications - 11
Citations - 494
A. P. Curtin is an academic researcher. The author has contributed to research in topics: Fast radio burst & Population. The author has an hindex of 2, co-authored 3 publications receiving 266 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
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.
Posted Content
No Evidence for Galactic Latitude Dependence of the Fast Radio Burst Sky Distribution
A. Josephy,P. Chawla,A. P. Curtin,V. M. Kaspi,Mohit Bhardwaj,P. J. Boyle,Charanjot Brar,Tomas Cassanelli,Emmanuel Fonseca,Bryan Gaensler,Calvin Leung,Hsiu-Hsien Lin,Kiyoshi Masui,R. Mckinven,J. Mena-Parra,Daniele Michilli,Cherry Ng,Ziggy Pleunis,M. Rafiei-Ravandi,Mubdi Rahman,P. Sanghavi,P. Scholz,K. M. Smith,I. H. Stairs,Shriharsh P. Tendulkar,A. V. Zwaniga +25 more
TL;DR: In this paper, the authors investigate whether the sky rate of fast radio bursts depends on Galactic latitude using the first catalog of FRBs detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project.
Journal ArticleDOI
CHIME/FRB Discovery of 25 Repeating Fast Radio Burst Sources
T. C. C. B. C. Andersen,Kevin Bandura,Mohit Bhardwaj,P. J. Boyle,C. Brar,T. Cassanelli,S. Chatterjee,P. Chawla,Amanda Cook,A. P. Curtin,Matt Dobbs,Feng Dong,Jakob Faber,M. Fandino,Emmanuel Fonseca,Bryan Gaensler,U. Giri,Antonio Herrera-Martín,Alex S. Hill,Adaeze Ibik,A. Josephy,Jane F. Kaczmarek,Zarif Kader,Victoria M. Kaspi,T. L. Landecker,Adam Lanman,Mattias Lazda,Calvin Leung,Hsiu-Hsien Lin,Kiyoshi Masui,R. Mckinven,J. Mena-Parra,B. W. Meyers,D. Michilli,Cherry Ng,Ayush Pandhi,Aaron B. Pearlman,Ue Li Pen,Emily Petroff,Ziggy Pleunis,M. Rafiei-Ravandi,Mubdi Rahman,Scott M. Ransom,A. Renard,Ketan R. Sand,Pranav Sanghavi,Paul Scholz,V. Shah,Kaitlyn Shin,Seth Siegel,Ingrid H. Stairs,Jian Nong Su,Shriharsh P. Tendulkar,K. Vanderlinde,Haochen Wang,Dallas Wulf,A. V. Zwaniga +56 more
TL;DR: In this paper , a new repeating fast radio burst (FRB) sources were found among CHIME/FRB events detected between 2019 September 30 and 2021 May 1, using a new clustering algorithm that looks for multiple events colocated on the sky having similar dispersion measures (DMs).
Journal ArticleDOI
An FRB Sent Me a DM: Constraining the Electron Column of the Milky Way Halo with Fast Radio Burst Dispersion Measures from CHIME/FRB
Amanda Cook,Mohit Bhardwaj,Bryan Gaensler,Paul Scholz,Gwendolyn Eadie,Alex S. Hill,Victoria M. Kaspi,Kiyoshi Masui,A. P. Curtin,Feng Dong,Emmanuel Fonseca,Antonio Herrera-Martín,Jane F. Kaczmarek,Adam Lanman,Mattias Lazda,B. W. Meyers,D. Michilli,Ayush Pandhi,Aaron B. Pearlman,Ziggy Pleunis,Scott M. Ransom,Mubdi Rahman,Ketan R. Sand,Kaitlyn Shin,Kendrick M. Smith,Ingrid H. Stairs,David C. Stenning David A. Dunlap Institute Department o AstronomyAstrophysics,Universityof Toronto,Dunlap Institute for AstronomyAstrophysics,McGill Space Institute,M. University,D. Physics,C. University,Dominion Observatory,Astronomy,U. Columbia,Mit Kavli Institute for Astrophysics,S. Research,M. I. O. Technology,W. University,Center for Gravitational Waves,Cosmology,International Centre for Radio Astronomy Research,C. University,National Radio Astronomy Observatory,S. Research,Perimeter Institute for Theoretical Physics,Department of Materials Science,Simon Fraser University +48 more
TL;DR: In this paper , the authors estimate the total Galactic electron column density from FRB dispersion measures (DMs) as a function of Galactic latitude using four different estimators, including ones that assume spherical symmetry of the ionized MW halo and ones that imply more latitudinal variation in density.