M
Mallory S. E. Roberts
Researcher at New York University Abu Dhabi
Publications - 194
Citations - 12337
Mallory S. E. Roberts is an academic researcher from New York University Abu Dhabi. The author has contributed to research in topics: Pulsar & Millisecond pulsar. The author has an hindex of 53, co-authored 189 publications receiving 11369 citations. Previous affiliations of Mallory S. E. Roberts include McGill University & Sonoma State University.
Papers
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Journal ArticleDOI
Phase-coherent timing of PSR J1811-1925: the pulsar at the heart of G11.2-0.3
TL;DR: In this article, a preliminary analysis of the PSR J1811-1925's hard spectrum was performed using the Rossi X-ray Timing Explorer/Proportional Counting Array (RXTE/PCA) timing observations of the pulsar that were designed to measure its braking index.
Journal ArticleDOI
The Green Bank Northern Celestial Cap Pulsar Survey II: The Discovery and Timing of Ten Pulsars
Adam Kawash,Maura McLaughlin,David L. Kaplan,Megan E. DeCesar,Lina Levin,D. R. Lorimer,R. S. Lynch,Kevin Stovall,Joseph K. Swiggum,Emmanuel Fonseca,Anne M. Archibald,S. Banaszak,Christopher M. Biwer,J. Boyles,Bingyi Cui,L. P. Dartez,D. Day,S. Ernst,A. J. Ford,J. Flanigan,S. A. Heatherly,J. W. T. Hessels,J. Hinojosa,Fredrick A. Jenet,C. Karako-Argaman,V. M. Kaspi,V. I. Kondratiev,S. Leake,G. Lunsford,J. G. Martinez,A. Mata,T. D. Matheny,Alexander McEwen,M. Mingyar,A. L. Orsini,Scott M. Ransom,Mallory S. E. Roberts,M. D. Rohr,Xavier Siemens,R. Spiewak,Ingrid H. Stairs,J. van Leeuwen,Arielle N. Walker,B. L. Wells +43 more
TL;DR: In this article, the authors presented phase-connected solutions for ten pulsars discovered in 350 MHz searches with the Green Bank Telescope, including PSR J0930$-$2301, a pulsar with nulling fraction lower limit of $\sim$30\% and nulling timescale of seconds to minutes.
Journal ArticleDOI
The Green Bank Telescope 350 MHz Drift-scan Survey II: Data Analysis and the Timing of 10 New Pulsars, Including a Relativistic Binary
Ryan S. Lynch,Ryan S. Lynch,Jason Boyles,Jason Boyles,Scott M. Ransom,Ingrid H. Stairs,Duncan R. Lorimer,Duncan R. Lorimer,Maura McLaughlin,Jason W. T. Hessels,Jason W. T. Hessels,Victoria M. Kaspi,V. I. Kondratiev,V. I. Kondratiev,Anne M. Archibald,Aaron Berndsen,R. F. Cardoso,Angus Cherry,Courtney R. Epstein,C. Karako-Argaman,Christie A. McPhee,Timothy T. Pennucci,Mallory S. E. Roberts,Kevin Stovall,Kevin Stovall,Joeri van Leeuwen,Joeri van Leeuwen +26 more
TL;DR: Boyles et al. as discussed by the authors conducted a drift scan survey using the Robert C. Byrd Green Bank Telescope with the goal of finding new radio pulsars, especially millisecond pulsars that can be timed to high precision.
Journal ArticleDOI
The GBT 350-MHz Drift Scan Pulsar Survey : III. Detection of a magnetic field in the eclipsing material of PSR J2256-1024
Kathryn Crowter,Ingrid H. Stairs,Christie A. McPhee,Anne M. Archibald,Anne M. Archibald,J. Boyles,Jason W. T. Hessels,Jason W. T. Hessels,C. Karako-Argaman,Duncan R. Lorimer,Ryan S. Lynch,Ryan S. Lynch,Maura McLaughlin,Scott M. Ransom,Mallory S. E. Roberts,Kevin Stovall,Joeri van Leeuwen,Joeri van Leeuwen +17 more
TL;DR: In this paper, the first measurement of a non-zero magnetic field in the eclipsing material of a black widow pulsar was presented, and the radio timing solution for PSR J2256-1024, polarization profiles at 350, 820, and 1500 MHz were presented.
Journal ArticleDOI
The Unusual Binary Pulsar PSR J1744–3922: Radio Flux Variability, Near-Infrared Observation, and Evolution
Rene P. Breton,Mallory S. E. Roberts,Scott M. Ransom,Victoria M. Kaspi,Martin Durant,Pierre Bergeron,A. J. Faulkner +6 more
TL;DR: The PSR J1744-3922 system as mentioned in this paper is a binary pulsar exhibiting highly variable pulsed radio emission, which suggests that this phenomenon is extrinsic to the pulsar and possibly tied to the companion, although not strongly correlated with orbital phase.