C
Cherry Ng
Researcher at University of Toronto
Publications - 219
Citations - 14331
Cherry Ng is an academic researcher from University of Toronto. The author has contributed to research in topics: Pulsar & Millisecond pulsar. The author has an hindex of 50, co-authored 186 publications receiving 10978 citations. Previous affiliations of Cherry Ng include Search for extraterrestrial intelligence & University of Hong Kong.
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Journal ArticleDOI
The High Time Resolution Universe Pulsar Survey – XII. Galactic plane acceleration search and the discovery of 60 pulsars
Cherry Ng,D. J. Champion,Matthew Bailes,Ewan Barr,S D Bates,N. D. R. Bhat,M Burgay,Sarah Burke-Spolaor,C.M.L. Flynn,A. Jameson,Simon Johnston,Michael Keith,Michael Kramer,Lina Levin,E. Petroff,Andrea Possenti,Ben Stappers,W. van Straten,Caterina Tiburzi,Ralph Eatough,Andrew Lyne +20 more
TL;DR: In this paper, the authors present initial results from the low-latitude Galactic plane region of the High Time Resolution Universe pulsar survey conducted at the Parkes 64m radio telescope.
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
Astrophysics Milestones For Pulsar Timing Array Gravitational Wave Detection
Nihan Pol,Stephen Taylor,Luke Zoltan Kelley,Sarah J. Vigeland,Joseph Simon,Siyuan Chen,Zaven Arzoumanian,Paul T. Baker,B. Bécsy,Adam Brazier,Paul R. Brook,Sarah Burke-Spolaor,Shami Chatterjee,James M. Cordes,Neil J. Cornish,Fronefield Crawford,H. Thankful Cromartie,Megan E. DeCesar,Paul Demorest,Timothy Dolch,Elizabeth C. Ferrara,William Fiore,Emmanuel Fonseca,Nathan Garver-Daniels,Deborah C. Good,Jeffrey S. Hazboun,Ross J. Jennings,Megan L. Jones,Andrew R. Kaiser,David L. Kaplan,Joey Shapiro Key,Michael T. Lam,T. Joseph W. Lazio,Jing Luo,Ryan S. Lynch,Dustin R. Madison,Alexander McEwen,Maura McLaughlin,Chiara M. F. Mingarelli,Cherry Ng,David J. Nice,Timothy T. Pennucci,Scott M. Ransom,Paul S. Ray,Brent J. Shapiro-Albert,Xavier Siemens,Ingrid H. Stairs,Daniel R. Stinebring,Joseph K. Swiggum,Michele Vallisneri,Haley M. Wahl,Caitlin A. Witt +51 more
TL;DR: In this article, a wide range of interpulsar-correlated GWB signals were injected into the NANOGrav dataset, allowing for a generalization to other pulsar-timing array datasets.
Journal ArticleDOI
Repeated, delayed torque variations following x-ray flux enhancements in the magnetar 1e 1048.1–5937
Robert F. Archibald,Victoria M. Kaspi,Cherry Ng,Paul Scholz,A. P. Beardmore,Neil Gehrels,J. A. Kennea +6 more
TL;DR: In this paper, the authors report on two years of flux and spin evolution monitoring of 1E 1048.1-5937, a 6.5 s X-ray pulsar identified as a magnetar.
Journal ArticleDOI
Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620
Emmanuel Fonseca,H. Thankful Cromartie,Timothy T. Pennucci,Paul S. Ray,Aida Yu. Kirichenko,Scott M. Ransom,Paul Demorest,Ingrid H. Stairs,Zaven Arzoumanian,Lucas Guillemot,Aditya Parthasarathy,Matthew Kerr,Ismaël Cognard,Paul T. Baker,Harsha Blumer,Paul R. Brook,Megan E. DeCesar,Timothy Dolch,F. Adam Dong,Elizabeth C. Ferrara,William Fiore,N. Garver-Daniels,Deborah C. Good,Ross J. Jennings,Megan L. Jones,Victoria M. Kaspi,Michael T. Lam,Duncan R. Lorimer,Jing Luo,Alexander McEwen,James Mckee,Maura McLaughlin,Natasha McMann,B. W. Meyers,A. Naidu,Cherry Ng,David J. Nice,Nihan Pol,Henri A. Radovan,Brent J. Shapiro-Albert,C. M. Tan,Shriharsh P. Tendulkar,Joseph K. Swiggum,Haley M. Wahl,Weiwei Zhu +44 more
TL;DR: In this paper, the relativistic Shapiro time delay of the radio pulsar J0740+6620 has been improved to 1.14+0.17 + 0.15 kpc by using a combination of the 100m Green Bank Telescope and the Canadian Hydrogen Intensity Mapping Experiment telescope.