most citedUpper limits on gravitational wave emission from 78 radio pulsars

195 citations · 401 across the 7 of their papers we have counts for

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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-qc20075 cited

Binary system delays and timing noise in searches for gravitational waves from known pulsars

Matthew Pitkin, Graham Woan

The majority of fast millisecond pulsars are in binary systems, so that any periodic signal they emit is modulated by both Doppler and relativistic effects. Here we show how well-e…

gr-qc200751 cited

An Evidence Based Search Method For Gravitational Waves From Neutron Star Ring-downs

J. Clark, I. S. Heng, M. Pitkin +1

The excitation of quadrupolar quasi-normal modes in a neutron star leads to the emission of a short, distinctive, burst of gravitational radiation in the form of a decaying sinusoi…

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…