activity
20042023
most citedHigh-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array

481 citations · 1.3k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2023★ 101 cited

The second data release from the European Pulsar Timing Array II. Customised pulsar noise models for spatially correlated gravitational waves

J. Antoniadis, P. Arumugam, S. Arumugam +95

The nanohertz gravitational wave background (GWB) is expected to be an aggregate signal of an ensemble of gravitational waves emitted predominantly by a large population of coalesc…

astro-ph.HE2019★ 44 cited

The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy

Christopher P. L. Berry, Scott A. Hughes, Carlos F. Sopuerta +6

The inspiral of a stellar-mass compact object into a massive (-) black hole produces an intricate gravitational-wave signal. Due to the extreme-mass…

astro-ph.HE2018

Linking gravitational waves and X-ray phenomena with joint LISA and Athena observations

Sean McGee, Alberto Sesana, Alberto Vecchio

The evolution of cosmic structures, the formation and growth of the first black holes and the connection to their baryonic environment are key unsolved problems in astrophysics. Th…

astro-ph.HE2016★ 481 cited

High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array

G. Desvignes, R. N. Caballero, L. Lentati +40

We report on the high-precision timing of 42 radio millisecond pulsars (MSPs) observed by the European Pulsar Timing Array (EPTA). This EPTA Data Release 1.0 extends up to mid-2014…

astro-ph.IM2016★ 123 cited

From Spin Noise to Systematics: Stochastic Processes in the First International Pulsar Timing Array Data Release

L. Lentati, R. M. Shannon, W. A. Coles +80

We analyse the stochastic properties of the 49 pulsars that comprise the first International Pulsar Timing Array (IPTA) data release. We use Bayesian methodology, performing model…

astro-ph.HE2015★ 35 cited

Infalling clouds onto super-massive black hole binaries - I. Formation of discs, accretion and gas dynamics

F. G. Goicovic, J. Cuadra, A. Sesana +3

There is compelling evidence that most -if not all- galaxies harbour a super-massive black hole (SMBH) at their nucleus, hence binaries of these massive objects are an inevitable p…