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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Proceedings ArticleDOI
New Discoveries from the GBT 350‐MHz Drift‐Scan Survey
Jason Boyles,Duncan R. Lorimer,Maura McLaughlin,Scott M. Ransom,Ryan S. Lynch,V. M. Kaspi,Anne M. Archibald,Ingrid H. Stairs,Christie A. McPhee,Mallory S. E. Roberts,V. I. Kondratiev,Jason W. T. Hessels,Jason W. T. Hessels,J. van Leeuwen,J. van Leeuwen,D. J. Champion,Adam Deller,B. H. Dunlap +17 more
TL;DR: In this article, the authors present the new pulsars discovered in the 350MHz survey with the Green Bank Telescope. But they highlight only one pulsar, J2222−0137, a pulsar with a minimum mass companion of 1.1 M⊙ and the second lowest dispersion measure.
Journal ArticleDOI
Multiwavelength Observations of the Runaway Binary HD 15137
M. Virginia McSwain,M. Virginia McSwain,Michaël De Becker,Mallory S. E. Roberts,Tabetha S. Boyajian,Tabetha S. Boyajian,Douglas R. Gies,Erika D. Grundstrom,Erika D. Grundstrom,Christina Aragona,Christina Aragona,Amber N. Marsh,Amber N. Marsh,Rachael M. Roettenbacher,Rachael M. Roettenbacher +14 more
TL;DR: In this paper, a new orbital solution for the spectroscopic binary and physical parameters of the O star primary was derived and the first XMM-Newton observations of the system were presented.
Posted Content
Recent Observations of EGRET Pulsar Wind Nebulae
TL;DR: In this article, the authors present recent X-ray and radio observations of pulsar wind nebulae discovered in EGRET error boxes, and discuss three PWN that are HESS TeV sources including a new HESS source associated with the Eel nebula.
Journal ArticleDOI
Two Pulsar Wind Nebulae: Chandra/XMM-Newton Imaging of GeV J1417-6100
TL;DR: In this article, Chandra ACIS and XMM-Newton MOS/PN imaging observations of two pulsar wind nebulae (K3/PSR J1420-6048 and G313.3+0.1=`the rabbit') associated with the Galactic unidentified gamma-ray source GeV J1417-6100 were reported.
Journal ArticleDOI
The Green Bank North Celestial Cap Pulsar Survey. IV. Four New Timing Solutions
R. J. Aloisi,A. Cruz,L. Daniels,N. Meyers,R. Roekle,A. Schuett,Joseph K. Swiggum,Megan E. DeCesar,David L. Kaplan,Ryan S. Lynch,Ryan S. Lynch,Kevin Stovall,Lina Levin,Anne M. Archibald,S. Banaszak,Christopher M. Biwer,Jason Boyles,P. Chawla,L. P. Dartez,Bingyi Cui,D. Day,A. J. Ford,J. Flanigan,Emmanuel Fonseca,Jason W. T. Hessels,Jason W. T. Hessels,J. Hinojosa,C. Karako-Argaman,V. M. Kaspi,V. I. Kondratiev,V. I. Kondratiev,S. Leake,G. Lunsford,J. G. Martinez,A. Mata,Maura McLaughlin,H. Al Noori,Scott M. Ransom,Mallory S. E. Roberts,M. D. Rohr,X. Siemens,Renée Spiewak,Ingrid H. Stairs,J. van Leeuwen,J. van Leeuwen,A. N. Walker,B. L. Wells,B. L. Wells +47 more
TL;DR: In this article, the authors presented timing solutions for four pulsars discovered in the Green Bank Northern Celestial Cap survey, all of which have spin periods between 0.26 and 1.84 s and a period derivative of 7.6 × 10−19 s s−1.