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20022022
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations · 6.1k across the 50 of their papers we have counts for

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Showing 2021Show all

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astro-ph.HE2021

Timing observations of three Galactic millisecond pulsars

D. R. Lorimer, A. M. Kawash, P. C. C. Freire +16

We report observed and derived timing parameters for three millisecond pulsars (MSPs) from observations collected with the Parkes 64-m telescope, Murriyang. The pulsars were found…

astro-ph.HE20213 cited

Back to quiescence: post-outburst evolution of the pulsar J1119-6127 and its wind nebula

Harsha Blumer, Samar Safi-Harb, Alice Borghese +4

We report on the analysis of a deep Chandra observation of the high-magnetic field pulsar (PSR) J1119-6127 and its compact pulsar wind nebula (PWN) taken in October 2019, three yea…

astro-ph.HE2021

Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620

Emmanuel Fonseca, H. Thankful Cromartie, Timothy T. Pennucci +42

We report results from continued timing observations of PSR J0740+6620, a high-mass, 2.8-ms radio pulsar in orbit with a likely ultra-cool white dwarf companion. Our data set consi…

astro-ph.HE202116 cited

Reactivation of the high-magnetic field pulsar PSR J1846--0258 with magnetar-like bursts

Harsha Blumer, Samar Safi-Harb, Maura A. McLaughlin +1

We report on the 2020 reactivation of the energetic high-magnetic field pulsar PSR J1846-0258 and its pulsar wind nebula (PWN) after 14 years of quiescence with new Chandra and Gre…

astro-ph.IM202111 cited

Commissioning the HI Observing Mode of the Beamformer for the Cryogenically Cooled Focal L-band Array for the GBT (FLAG)

N. M. Pingel, D. J. Pisano, M. Ruzindana +19

We present the results of commissioning observations for a new digital beamforming back end for the Focal plane L-band Array for the Robert C. Byrd Green Bank Telescope (FLAG), a c…

astro-ph.GA2021

The NANOGrav 11yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500Mpc

Zaven Arzoumanian, Paul T. Baker, Adam Brazier +54

Supermassive black hole binaries (SMBHBs) should form frequently in galactic nuclei as a result of galaxy mergers. At sub-parsec separations, binaries become strong sources of low-…