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Pulsar timing experiments aimed at the detection of gravitational radiation have been performed for decades now.
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It should be emphasized that the expression of the one-way Doppler response given here presumes the mass of the graviton to be null. This simplification is justified by the fact that the existing upper-limits to the values of the mass of the graviton are rather small, and they result in unnoticeable changes to the sensitivities calculated by relying on Eq. ( 1
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Although this effect was noticed by Lee et al
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J. P. W. Verbiest, M. Bailes, W. A. Coles, G. B. Hobbs, W. van Straten, D. J. Champion, F. A. Jenet, R. N. Manchester, N. D. R. Bhat, J. M. Sarkissian, D. Yardley, S. Burke-Spolaor, A. W. Hotan, and X. P. You, Mon. Not. R. Astron. Soc. 400
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M. Alves, O. Miranda, and J. de Araujo, Class. Quantum Grav. 27
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