activity
20192022
most citedThe International Pulsar Timing Array second data release: Search for an isotropic Gravitational Wave Background

344 citations · 379 across the 5 of their papers we have counts for

collaborators

9 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.GA20204 cited

Multi-Messenger Gravitational Wave Searches with Pulsar Timing Arrays: Application to 3C66B Using the NANOGrav 11-year Data Set

Zaven Arzoumanian, Paul T. Baker, Adam Brazier +56

When galaxies merge, the supermassive black holes in their centers may form binaries and, during the process of merger, emit low-frequency gravitational radiation in the process. I…

astro-ph.GA2020

The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View

Alessandra De Rosa, Cristian Vignali, Tamara Bogdanović +27

The quest for binary and dual supermassive black holes (SMBHs) at the dawn of the multi-messenger era is compelling. Detecting dual active galactic nuclei (AGN) -- active SMBHs at…

astro-ph.GA2020

Correlation between Optical and UV Variability of Quasars

Chengcheng Xin, Maria Charisi, Zoltán Haiman +1

The variability of quasars across multiple wavelengths is a useful probe of physical conditions in active galactic nuclei. In particular, variable accretion rates, instabilities, a…

astro-ph.HE2019

Spikey: Self-Lensing Flares from Eccentric SMBH Binaries

Betty X. Hu, Daniel J. D'Orazio, Zoltan Haiman +4

We examine the light curves of two quasars, motivated by recent suggestions that a supermassive black hole binary (SMBHB) can exhibit sharp lensing spikes. We model the variability…

astro-ph.GA2019

Testing the relativistic Doppler boost hypothesis for the binary candidate quasar PG1302-102 with multi-band Swift data

Chengcheng Xin, Maria Charisi, Zoltan Haiman +4

The bright quasar PG1302-102 has been identified as a candidate supermassive black hole binary from its near-sinusoidal optical variability. While the significance of its optical p…