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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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Discovery of high-energy Gamma-Ray pulsations from PSR J2021+3651 with AGILE

TL;DR: In this article, the authors reported the discovery of γ-ray pulsations from PSR J2021+3651 in the 100-1500 MeV range using data from the AGILE satellite gathered over 8 months, folded on a densely sampled, contemporaneous radio ephemeris obtained for this purpose at the Green Bank Telescope.
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Two Pulsar Wind Nebulae: Chandra/XMM-Newton Imaging of GeV J1417?6100

TL;DR: In this paper, 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 γ-ray source GeV J1417-6100.
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Detection of X-ray emission from the PSR 1259-63/SS 2883 binary system

TL;DR: The radio pulsar PSR 1259-63 was found to be in a binary system with a massive main-sequence companion, and it is the most highly eccentric binary system known to contain a neutron star as discussed by the authors.
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Observations of 4U 1700-37 with BATSE

TL;DR: In this paper, an upper limit of 4% on the pulse fraction has been obtained for pulse periods between 2 and 700 s. The authors used Monte Carlo simulations to propagate errors in measured and assumed parameters.
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A First Search for coincident Gravitational Waves and High Energy Neutrinos using LIGO, Virgo and ANTARES data from 2007

S. Adrián-Martínez, +955 more
TL;DR: In this paper, the results of the first search for gravitational wave bursts associated with high energy neutrinos were presented, which could reveal new, hidden sources that are not observed by conventional photon astronomy, particularly at high energy.