most citedUpper limits on gravitational wave emission from 78 radio pulsars

195 citations · 415 across the 7 of their papers we have counts for

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gr-qc20086 cited

Markov chain Monte Carlo searches for Galactic binaries in Mock LISA Data Challenge 1B data sets

Miquel Trias, Alberto Vecchio, John Veitch

We are developing a Bayesian approach based on Markov chain Monte Carlo techniques to search for and extract information about white dwarf binary systems with the Laser Interferome…

gr-qc200864 cited

A Bayesian approach to the follow-up of candidate gravitational wave signals

John Veitch, Alberto Vecchio

Ground-based gravitational wave laser interferometers (LIGO, GEO-600, Virgo and Tama-300) have now reached high sensitivity and duty cycle. We present a Bayesian evidence-based app…

gr-qc200764 cited

Report on the second Mock LISA Data Challenge

Stanislav Babak, John G. Baker, Matthew J. Benacquista +40

The Mock LISA Data Challenges are a program to demonstrate LISA data-analysis capabilities and to encourage their development. Each round of challenges consists of several data set…

gr-qc200719 cited

Inference on inspiral signals using LISA MLDC data

Christian Röver, Alexander Stroeer, Ed Bloomer +11

In this paper we describe a Bayesian inference framework for analysis of data obtained by LISA. We set up a model for binary inspiral signals as defined for the Mock LISA Data Chal…

gr-qc200719 cited

Inference on white dwarf binary systems using the first round Mock LISA Data Challenges data sets

Alexander Stroeer, John Veitch, Christian Roever +11

We report on the analysis of selected single source data sets from the first round of the Mock LISA Data Challenges (MLDC) for white dwarf binaries. We implemented an end-to-end pi…

gr-qc2007195 cited

Upper limits on gravitational wave emission from 78 radio pulsars

The LIGO Scientific Collaboration, B. Abbott, M. Kramer +1

We present upper limits on the gravitational wave emission from 78 radio pulsars based on data from the third and fourth science runs of the LIGO and GEO600 gravitational wave dete…