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20102026
most citedRelativistic Shapiro delay measurements of an extremely massive millisecond pulsar

1.6k citations · 16.3k across the 139 of their papers we have counts for

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Showing 2019Show all

14 papers · 1 filter

astro-ph.HE2019★ 48 cited

The NANOGrav 11-Year Data Set: Limits on Gravitational Wave Memory

K. Aggarwal, Z. Arzoumanian, P. T. Baker +58

The mergers of supermassive black hole binaries (SMBHBs) promise to be incredible sources of gravitational waves (GWs). While the oscillatory part of the merger gravitational wavef…

astro-ph.HE2019★ 38 cited

Which bright fast radio bursts repeat?

C. W. James, S. Oslowski, C. Flynn +13

A handful of fast radio bursts (FRBs) are now known to repeat. However, the question remains --- do they all? We report on an extensive observational campaign with the Australian S…

astro-ph.EP2019★ 17 cited

The NANOGrav 11-year Data Set: Constraints on Planetary Masses Around 45 Millisecond Pulsars

E. A. Behrens, S. M. Ransom, D. R. Madison +27

We search for extrasolar planets around millisecond pulsars using pulsar timing data and seek to determine the minimum detectable planetary masses as a function of orbital period.…

astro-ph.IM2019★ 1 cited

Canada and the SKA from 2020-2030

Kristine Spekkens, Cynthia Chiang, Roland Kothes +57

This white paper submitted for the 2020 Canadian Long-Range Planning process (LRP2020) presents the prospects for Canada and the Square Kilometre Array (SKA) from 2020-2030, focuss…

astro-ph.IM2019★ 93 cited

LRP 2020 Whitepaper: The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD)

K. Vanderlinde, K. Bandura, L. Belostotski +20

The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD) is a next-generation radio telescope, proposed for construction to start immediately. CHORD is a pan-Canadian…

astro-ph.HE2019★ 43 cited

The NANOGrav 11-Year Data Set: Evolution of Gravitational Wave Background Statistics

J. S. Hazboun, J. Simon, S. R. Taylor +60

An ensemble of inspiraling supermassive black hole binaries should produce a stochastic background of very low frequency gravitational waves. This stochastic background is predicte…