C
Cherie K. Day
Researcher at Swinburne University of Technology
Publications - 50
Citations - 2218
Cherie K. Day is an academic researcher from Swinburne University of Technology. The author has contributed to research in topics: Galaxy & Fast radio burst. The author has an hindex of 17, co-authored 43 publications receiving 1449 citations. Previous affiliations of Cherie K. Day include Australia Telescope National Facility & Commonwealth Scientific and Industrial Research Organisation.
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Journal ArticleDOI
A single fast radio burst localized to a massive galaxy at cosmological distance
Keith W. Bannister,Adam Deller,Chris Phillips,Jean-Pierre Macquart,Jason X. Prochaska,Jason X. Prochaska,Nicolas Tejos,Stuart D. Ryder,Elaine M. Sadler,Elaine M. Sadler,Ryan Shannon,Sunil Simha,Cherie K. Day,Matthew McQuinn,F. O. North-Hickey,Shivani Bhandari,W. Arcus,Vardha N. Bennert,J. N. Burchett,M. Bouwhuis,Richard Dodson,Ron Ekers,Ron Ekers,Wael Farah,Chris Flynn,C. W. James,Matthew Kerr,Emil Lenc,Elizabeth K. Mahony,John M. O'Meara,Stefan Oslowski,Hao Qiu,Hao Qiu,Tommaso Treu,T. Bateman,Douglas C.-J. Bock,R. J. Bolton,Anthony G. A. Brown,John D. Bunton,Aaron Chippendale,F. R. Cooray,Tim J. Cornwell,N. Gupta,Douglas B. Hayman,Michael Kesteven,Bärbel S. Koribalski,A. Macleod,Naomi McClure-Griffiths,S. Neuhold,Ray P. Norris,Ray P. Norris,M. A. Pilawa,R.-Y. Qiao,John Reynolds,Daniel N. Roxby,Timothy W. Shimwell,Maxim Voronkov,Christine D. Wilson +57 more
TL;DR: In this paper, the authors reported the interferometric localization of the single-pulse fast radio burst (FRB 180924) to a position 4 kiloparsecs from the center of a luminous galaxy at redshift 0.3214.
Journal ArticleDOI
A census of baryons in the Universe from localized fast radio bursts.
Jean-Pierre Macquart,Jason X. Prochaska,Jason X. Prochaska,Matthew McQuinn,Keith W. Bannister,Shivani Bhandari,Cherie K. Day,Cherie K. Day,Adam Deller,Ron Ekers,Ron Ekers,C. W. James,Lachlan Marnoch,Lachlan Marnoch,Stefan Oslowski,Chris Phillips,Stuart D. Ryder,D. R. Scott,Ryan Shannon,Nicolas Tejos +19 more
TL;DR: In this paper, the dispersion of a sample of localized fast radio bursts was used to determine the electron column density along each line of sight and accounts for every ionized baryon.
Journal ArticleDOI
The low density and magnetization of a massive galaxy halo exposed by a fast radio burst.
J. Xavier Prochaska,J. Xavier Prochaska,Jean-Pierre Macquart,Matthew McQuinn,Sunil Simha,Ryan Shannon,Cherie K. Day,Cherie K. Day,Lachlan Marnoch,Lachlan Marnoch,Stuart D. Ryder,Adam Deller,Keith W. Bannister,Shivani Bhandari,Rongmon Bordoloi,John D. Bunton,Hyerin Cho,Chris Flynn,Elizabeth K. Mahony,Chris Phillips,Hao Qiu,Nicolas Tejos +21 more
TL;DR: In this article, the authors reported the detection of a fast radio burst (FRB 181112), localized with arcsecond precision, that passes through the halo of a foreground galaxy.
Journal ArticleDOI
A census of baryons in the Universe from localized fast radio bursts
Jean-Pierre Macquart,Jason X. Prochaska,Jason X. Prochaska,Matthew McQuinn,Keith W. Bannister,Shivani Bhandari,Cherie K. Day,Cherie K. Day,Adam Deller,Ron Ekers,Ron Ekers,C. W. James,Lachlan Marnoch,Lachlan Marnoch,Stefan Oslowski,Chris Phillips,Stuart D. Ryder,D. R. Scott,Ryan Shannon,Nicolas Tejos +19 more
TL;DR: The baryon density determined along the lines of sight to localized fast radio bursts is consistent with that determined from the cosmic microwave background and required by Big Bang nucleosynthesis.
Journal ArticleDOI
The low density and magnetization of a massive galaxy halo exposed by a fast radio burst
J. Xavier Prochaska,J. Xavier Prochaska,Jean-Pierre Macquart,Matthew McQuinn,Sunil Simha,Ryan Shannon,Cherie K. Day,Cherie K. Day,Lachlan Marnoch,Lachlan Marnoch,Stuart D. Ryder,Adam Deller,Keith W. Bannister,Shivani Bhandari,Rongmon Bordoloi,John D. Bunton,Hyerin Cho,Chris Flynn,Elizabeth K. Mahony,Chris Phillips,Hao Qiu,Nicolas Tejos +21 more
TL;DR: In this article, the authors reported the detection of a fast radio burst (FRB 181112) with arcsecond precision, which passes through the halo of a foreground galaxy.