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The third observing run of advanced LIGO, Virgo and KAGRA broughtunprecedented sensitivity towards a variety of quasi-monochromatic, persistentgravitational-wave signals. Continuous waves allow us to probe not just theexistence of canonical asymmetrically rotating neutron stars, but alsodifferent forms of dark matter, thus showing the wide-ranging astrophysicalimplications of using a relatively simple signal model. I will describe themajor results from the numerous continuous-wave searches that were performed inO3, both inside and outside the LIGO/Virgo/KAGRA collaborations, and show howimpactful to multi-messenger physics that they have been.

Recent results from continuous gravitational wave searches using data from LIGO/Virgo/KAGRA's third observing run