Gravitational-wave astronomy requires population-informed parameter estimation. Mould, M., Tenorio, R., & Gerosa, D. \prd, 114(2):L021302, July, 2026.
doi  bibtex   
@ARTICLE{2026PhRvD.114b1302M,
       author = {{Mould}, Matthew and {Tenorio}, Rodrigo and {Gerosa}, Davide},
        title = "{Gravitational-wave astronomy requires population-informed parameter estimation}",
      journal = {\prd},
     keywords = {General Relativity and Quantum Cosmology, High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics, Data Analysis, Statistics and Probability},
         year = 2026,
        month = jul,
       volume = {114},
       number = {2},
          eid = {L021302},
        pages = {L021302},
          doi = {10.1103/blhd-ktbf},
archivePrefix = {arXiv},
       eprint = {2604.15885},
 primaryClass = {gr-qc},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2026PhRvD.114b1302M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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