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Pulsar timing arrays (PTAs) are sensitive to oscillations in the gravitational potential along the line-of-sight due to ultralight particle pressure.
M. Safarzadeh and D. N. Spergel, doi:10.3847/1538-4357/ab7db2 [arXiv:1906.11848 [astro-ph.CO]]
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A. Khmelnitsky and V. Rubakov, “Pulsar timing signal from ultralight scalar dark matter,” JCAP 02
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J. M. Armaleo, D. López Nacir and F. R. Urban, “Searching for spin-2 ULDM with gravitational waves interferometers,” JCAP 04
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