D
Deborah C. Good
Researcher at University of British Columbia
Publications - 80
Citations - 5930
Deborah C. Good is an academic researcher from University of British Columbia. The author has contributed to research in topics: Pulsar & Fast radio burst. The author has an hindex of 29, co-authored 58 publications receiving 3872 citations.
Papers
More filters
Journal ArticleDOI
The NANOGrav 12.5-year Data Set: Search For An Isotropic Stochastic Gravitational-Wave Background
Zaven Arzoumanian,Paul T. Baker,Harsha Blumer,B. Bécsy,Adam Brazier,Paul R. Brook,Sarah Burke-Spolaor,Shami Chatterjee,Siyuan Chen,James M. Cordes,Neil J. Cornish,Fronefield Crawford,H. Thankful Cromartie,Megan E. DeCesar,Paul Demorest,Timothy Dolch,Justin A. Ellis,Elizabeth C. Ferrara,William Fiore,Emmanuel Fonseca,Nathan Garver-Daniels,Peter A. Gentile,Deborah C. Good,Jeffrey S. Hazboun,A. Miguel Holgado,K. Islo,Ross J. Jennings,Megan L. Jones,Andrew R. Kaiser,David L. Kaplan,Luke Zoltan Kelley,Joey Shapiro Key,Nima Laal,Michael T. Lam,T. Joseph W. Lazio,Duncan R. Lorimer,Jing Luo,Ryan S. Lynch,Dustin R. Madison,Maura McLaughlin,Chiara M. F. Mingarelli,Cherry Ng,David J. Nice,Timothy T. Pennucci,Nihan Pol,Scott M. Ransom,Paul S. Ray,Brent J. Shapiro-Albert,Xavier Siemens,Joseph Simon,Renée Spiewak,Ingrid H. Stairs,Daniel R. Stinebring,Kevin Stovall,Jerry P. Sun,Joseph K. Swiggum,Stephen Taylor,J. E. Turner,Michele Vallisneri,Sarah J. Vigeland,Caitlin A. Witt +60 more
TL;DR: In this article, the authors search for an isotropic stochastic GWB in the 12.5-year pulsar timing data set collected by the North American Nanohertz Observatory for Gravitational Waves.
Journal ArticleDOI
The NANOGrav 12.5 yr Data Set: Search for an Isotropic Stochastic Gravitational-wave Background
Zaven Arzoumanian,Paul T. Baker,Harsha Blumer,B. Bécsy,Adam Brazier,Paul R. Brook,Sarah Burke-Spolaor,Sarah Burke-Spolaor,Shami Chatterjee,Siyuan Chen,Siyuan Chen,James M. Cordes,Neil J. Cornish,Fronefield Crawford,H. Thankful Cromartie,H. Thankful Cromartie,Megan E. DeCesar,Megan E. DeCesar,Paul Demorest,Timothy Dolch,Justin A. Ellis,Elizabeth C. Ferrara,William Fiore,Emmanuel Fonseca,Nathan Garver-Daniels,Peter A. Gentile,Deborah C. Good,Jeffrey S. Hazboun,A. Miguel Holgado,A. Miguel Holgado,K. Islo,Ross J. Jennings,Megan L. Jones,Andrew R. Kaiser,David L. Kaplan,Luke Zoltan Kelley,Joey Shapiro Key,Nima Laal,Michael T. Lam,T. Joseph W. Lazio,Duncan R. Lorimer,Jing Luo,Ryan S. Lynch,D. R. Madison,Maura McLaughlin,Chiara M. F. Mingarelli,Chiara M. F. Mingarelli,Cherry Ng,David J. Nice,Timothy T. Pennucci,Timothy T. Pennucci,Nihan Pol,Nihan Pol,Scott M. Ransom,Paul S. Ray,Brent J. Shapiro-Albert,Xavier Siemens,Xavier Siemens,Joseph Simon,Joseph Simon,Renée Spiewak,Ingrid H. Stairs,Daniel R. Stinebring,Kevin Stovall,Jerry P. Sun,Joseph K. Swiggum,Stephen Taylor,Jacob E. Turner,Michele Vallisneri,Sarah J. Vigeland,Caitlin A. Witt +70 more
TL;DR: In this article, the authors search for an isotropic stochastic GWB in the 12.5-yr pulsar-timing data set collected by the North American Nanohertz Observatory for Gravitational Waves.
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
CHIME/FRB Discovery of Eight New Repeating Fast Radio Burst Sources
B. C. Andersen,Kevin Bandura,Mohit Bhardwaj,P. Boubel,M. M. Boyce,P. J. Boyle,C. Brar,Tomas Cassanelli,P. Chawla,D. Cubranic,M. Deng,M. Dobbs,M. Fandino,E. Fonseca,Bryan Gaensler,A. J. Gilbert,A. J. Gilbert,U. Giri,Deborah C. Good,Mark Halpern,Alex S. Hill,Gary Hinshaw,C. Höfer,A. Josephy,Victoria M. Kaspi,Roland Kothes,T. Landecker,T. Landecker,Dustin Lang,D. Z. Li,Hsiu-Hsien Lin,Kiyoshi Masui,J. Mena-Parra,M. Merryfield,R. Mckinven,D. Michilli,D. Michilli,N. Milutinovic,A. Naidu,Laura Newburgh,Chi-Yung Ng,C. Patel,Ue-Li Pen,T. Pinsonneault-Marotte,Ziggy Pleunis,M. Rafiei-Ravandi,M. Rahman,Scott M. Ransom,A. Renard,Paul Scholz,S. R. Siegel,S. Singh,Kendrick M. Smith,Ingrid H. Stairs,S. P. Tendulkar,I. Tretyakov,K. Vanderlinde,P. Yadav,A. V. Zwaniga +58 more
Journal ArticleDOI
A repeating fast radio burst source localized to a nearby spiral galaxy
Benito Marcote,K. Nimmo,K. Nimmo,Jason W. T. Hessels,Jason W. T. Hessels,Shriharsh P. Tendulkar,C. G. Bassa,Zsolt Paragi,A. Keimpema,Mohit Bhardwaj,Ramesh Karuppusamy,V. M. Kaspi,Casey J. Law,Daniele Michilli,Kshitij Aggarwal,B. C. Andersen,Anne M. Archibald,Anne M. Archibald,Kevin Bandura,Geoffrey C. Bower,P. J. Boyle,C. Brar,Sarah Burke-Spolaor,Bryan J. Butler,T. Cassanelli,P. Chawla,Paul Demorest,M. A. Dobbs,Emmanuel Fonseca,U. Giri,U. Giri,Deborah C. Good,K. Gourdji,A. Josephy,A. Yu. Kirichenko,A. Yu. Kirichenko,F. Kirsten,T. L. Landecker,Dustin Lang,T. J. W. Lazio,D. Z. Li,Hsiu-Hsien Lin,J. D. Linford,Kiyoshi Masui,J. Mena-Parra,A. Naidu,Cherry Ng,C. Patel,Ue-Li Pen,Ziggy Pleunis,M. Rafiei-Ravandi,Mubdi Rahman,A. Renard,P. Scholz,P. Scholz,S. R. Siegel,Kendrick M. Smith,Ingrid H. Stairs,K. Vanderlinde,A. V. Zwaniga +59 more
TL;DR: Only one repeating fast radio burst has been localized, to an irregular dwarf galaxy; now another is found to come from a star-forming region of a nearby spiral galaxy, suggesting that repeating FRBs may have a wide range of luminosities, and originate from diverse host galaxies and local environments.