Acknowledgements . We thank Angela Borchers for her advice on extracting individual modes from NRSur7dq4. We also thank Thomas Dent, Aditya Vijaykumar, Will Farr, Tjonnie Li and Cecilio Garcia-Quiros for useful discussions and comments on the manuscript. JCB is funded by a fellowship from 'la Caixa' Foundation (ID100010474) and from the European Union's Horizon2020 research and innovation programme under the Marie Skodowska-Curie grant agreement No 847648. The fellowship code is LCF/BQ/PI20/11760016. JCB is also supported by the research grant PID2020-118635GB-I00 from the Spain-Ministerio de Ciencia e Innovacion
and by its Ramon y Cajal program (grant RYC2022036203-I). ADR acknowledges support through (i) Maria Zambrano grant ZA21-048 with reference UP2021-044 from the Spanish Ministerio de Universidades, funded within the European Union-Next Generation EU, and (ii) Atraccion de Talento Cesar Nombela grant No 2023-T1/TEC-29023, funded by Comunidad de Madrid (Spain). ADR further acknowledges financial support via the Spanish Grants PID2020-116567GBC21, funded by MCIN/AEI/10.13039/501100011033, and PID2023-149560NB-C21, funded by MCIU /AEI/10.13039/501100011033/FEDER, UE. NSG acknowledges support from the Spanish Ministerio de Universidades, through a Mar´ ıa Zambrano grant (ZA21-031) with reference UP2021-044, funded within the European Union-Next Generation EU, and from the Spanish Ministry of Science and Innovation via the Ramon y Cajal programme (grant RYC2022-037424-I), funded by MCIN/AEI/ 10.13039/501100011033 and by 'ESF Investing in your future'. NSG is further supported by the Spanish Agencia Estatal de Investigacion (Grant PID2021-125485NB-C21) funded by MCIN/AEI/10.13039/501100011033 and ERDF A way of making Europe, and by the European Union's Horizon 2020 research and innovation (RISE) programme H2020-MSCA-RISE-2017 Grant No. FunFiCO-777740 and by the European Horizon Europe staff exchange (SE) programme HORIZON-MSCA2021-SE-01 Grant No. NewFunFiCO-101086251. KC acknowledges the support through NSF grant numbers PHY-2207638, AST-2307147, PHY-2308886, and PHY-2309064. We acknowledge the use of IUCAA LDG cluster Sarathi for the computational/numerical work. The authors acknowledge computational resources provided by the CIT cluster of the LIGO Laboratory and supported by National Science Foundation Grants PHY-0757058 and PHY0823459; and the support of the NSF CIT cluster for the provision of computational resources for our parameter inference runs. This material is based upon work supported by NSF's LIGO Laboratory which is a major facility fully funded by the National Science Foundation. The analysed LIGO-Virgo data and the corresponding power spectral densities, in their strain versions, are publicly available at the online Gravitational-Wave Open Science Center [87, 88]. This research has made use of data or software obtained from the Gravitational Wave Open Science Center (gwosc.org), a service of LIGO Laboratory, the LIGO Scientific Collaboration, the Virgo Collaboration, and KAGRA. LIGO Laboratory and Advanced LIGO are funded by the United States National Science Foundation (NSF) as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. Virgo is funded, through the European Gravitational Observatory (EGO), by the French Centre National de Recherche Scientifique (CNRS), the Italian Istituto Nazionale di Fisica Nucleare (INFN) and the Dutch Nikhef, with contributions by institutions from Belgium, Germany, Greece, Hungary, Ireland, Japan, Monaco, Poland, Portugal, Spain. KAGRA is supported by Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan Society for the Promotion of Science (JSPS) in Japan; National Research Foundation (NRF) and Ministry of Science and ICT (MSIT) in Korea; Academia Sinica (AS) and National Science and Technology Council (NSTC) in Taiwan. This manuscript has LIGO DCC number P2400018.