New Limits on Gravitational Radiation using Pulsars

A. N. Lommen

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New Limits on Gravitational Radiation using Pulsars

A. N. Lommen

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Abstract

We calculate a new gravitational wave background limit using timing residuals from PSRs J1713+0747, B1855+09, and B1937+21. The new limit is based on 17 years of continuous data pieced together from 3 different observing projects: 2 at the Arecibo Observatory and 1 at the 140ft Green Bank Telescope. This project represents the earliest results from the `Pulsar Timing Array' which will soon be able detect the stochastic background from early massive black hole mergers.

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A. N. Lommen. 2002-08-30. New Limits on Gravitational Radiation using Pulsars. https://arxiv.org/abs/astro-ph/0208572

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