activity
20122021
most citedMulti-Messenger Astrophysics with Pulsar Timing Arrays

27 citations · 27 across the 3 of their papers we have counts for

collaborators

5 papers

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-…

astro-ph.IM2019

NANOGrav Education and Outreach: Growing a Diverse and Inclusive Collaboration for Low-Frequency Gravitational Wave Astronomy

The NANOGrav Collaboration, P. T. Baker, H. Blumer +25

The new field of gravitational wave astrophysics requires a growing pool of students and researchers with unique, interdisciplinary skill sets. It also offers an opportunity to bui…

astro-ph.HE201927 cited

Multi-Messenger Astrophysics with Pulsar Timing Arrays

Luke Zoltan Kelley, Maria Charisi, Sarah Burke-Spolaor +29

Pulsar timing arrays (PTAs) are on the verge of detecting low-frequency gravitational waves (GWs) from supermassive black hole binaries (SMBHBs). With continued observations of a l…

astro-ph.IM2016

Interpreting the Recent Upper Limit on the Gravitational Wave Background from the Parkes Pulsar Timing Array

The NANOGrav Collaboration

We provide comments on the article by Shannon et al. (Sep 2015) entitled "Gravitational waves from binary supermassive black holes missing in pulsar observations". The purpose of t…

astro-ph.IM2012

Why Gravitational Wave Science Needs Pulsar Timing Arrays And Why Pulsar Timing Arrays Need Both Arecibo and the GBT: A Response to the NSF-AST Portfolio Review from the NANOGrav Collaboration

The NANOGrav Collaboration

Gravitational waves (GWs) are ripples in space-time that are known to exist but have not yet been detected directly. Once they are, a key feature of any viable theory of gravity wi…