Presence of the (l,m,n) = (4,4,0) quasi-normal mode in GW250114
Ascertain whether the Kerr quasi-normal mode with angular indices (l, m, n) = (4, 4, 0) (the 440 mode) is present in the GW250114 ringdown signal.
References
As a result, the analysis cannot by itself establish whether the 440 QNM is present in the data.
— Black Hole Spectroscopy and Tests of General Relativity with GW250114
(2509.08099 - Collaboration et al., 9 Sep 2025) in BH spectroscopy with full signal (pSEOBNR analysis discussion)