• [1]

    M. Armanoet al., Phys. Rev. Lett.116, 231101 (2016)

  • [2]

    P. Amaro-Seoaneet al. (LISA),Laser Interferometer Space Antenna, (2017), arXiv: 1702.00786[astroph.IM]

  • [3]

    P. Amaro Seoaneet al. (LISA), Living Rev. Rel.26, 2 (2023), arXiv:2203.06016[gr-qc]

  • [4]

    L. Barack and C. Cutler, Phys. Rev. D70, 122002 (2004), arXiv:gr-qc/0409010

  • [5]

    T. Robson, Neil J. Cornish, and Chang Liu, Class. Quant. Grav.36, 105011 (2019), arXiv:1803.01944[astroph.HE]

  • [6]

    N. Cornish and T. Robson, J. Phys. Conf. Ser.840, 012024 (2017), arXiv:1703.09858[astro-ph.IM]

  • [7]

    Z. C. Chen, F. Huang, and Q. G. Huang, Astrophys. J.871, 97 (2019), arXiv:1809.10360[gr-qc]

  • [8]

    G. Agazieet al. (NANOGrav), Astrophys. J. Lett.951, L8 (2023), arXiv:2306.16213[astro-ph.HE]

  • [9]

    G. Agazieet al. (NANOGrav), Astrophys. J. Lett.951, L9 (2023), arXiv:2306.16217[astro-ph.HE]

  • [10]

    A. Afzalet al. (NANOGrav), Astrophys. J. Lett.951, L11 (2023), arXiv:2306.16219[astroph.HE]

  • [11]

    J. Antoniadiset al. (EPTA, InPTA:), Astron. Astrophys.678, A50 (2023), arXiv:2306.16214[astro-ph.HE]

  • [12]

    J. Antoniadiset al. (EPTA), Astron. Astrophys.678, A48 (2023), arXiv:2306.16224[astro-ph.HE]

  • [13]

    D. J. Reardonet al., Astrophys. J. Lett.951, L6 (2023), arXiv:2306.16215[astro-ph.HE]

  • [14]

    A. Zicet al.,The Parkes Pulsar Timing Array Third Data Release, (2023), arXiv: 2306.16230[astroph.HE]

  • [15]

    R. D. Nan, D. Li, C. J. Jinet al., Int. J. Mod. Phys. D20, 989 (2011), arXiv:1105.3794[astro-ph.IM]

  • [16]

    H. Xuet al., Res. Astron. Astrophys.23, 075024 (2023), arXiv:2306.16216[astro-ph.HE]

  • [17]

    G. Agazieet al. (NANOGrav), Astrophys. J. Lett.952, L37 (2023), arXiv:2306.16220[astro-ph.HE]

  • [18]

    J. Antoniadiset al. (EPTA),The second data release from the European Pulsar Timing Array: V. Implications for massive black holes, dark matter and the early Universe, (2023), arXiv: 2306.16227[astro-ph.CO]

  • [19]

    Y. C. Bi, Y. M. Wu, Z. C. Chenet al., Sci. China Phys. Mech. Astron.66, 120402 (2023), arXiv:2307.00722[astro-ph.CO]

  • [20]

    J. Ellis, M. Fairbairn, G. Francioliniet al.,What is the source of the PTA GW signal? (2023), arXiv: 2308.08546[astro-ph.CO]

  • [21]

    Z. C. Li, Z. Jiang, X. L. Fanet al., Mon. Not. Roy. Astron. Soc.527, 3 (2024), arXiv:2304.08333[gr-qc]

  • [22]

    S. Y. Chen, Alberto Sesana, and Christopher J. Conselice, Mon. Not. Roy. Astron. Soc.488, 401 (2019), arXiv:1810.04184[astro-ph.GA]

  • [23]

    P. Ajithet al., Phys. Rev. D77, 104017 (2008), arXiv:0710.2335[gr-qc]

  • [24]

    X. J. Zhu, E. Howell, T. Regimbauet al., Astrophys. J.739, 86 (2011), arXiv:1104.3565[gr-qc]

  • [25]

    E. S. Phinney,A Practical theorem on gravitational wave backgrounds, (2001), arXiv: astro-ph/0108028

  • [26]

    N. Aghanimet al. (Planck), Astron. Astrophys.641, A6 (2020) [Erratum: Astron. Astrophys.652, C4 (2021)], arXiv: 1807.06209[astro-ph.CO]

  • [27]

    J. Kormendy and L. C. Ho, Ann. Rev. Astron. Astrophys.51, 511 (2013), arXiv:1304.7762[astro-ph.CO]

  • [28]

    C. Pitte, Q. Baghi, S. Marsatet al., Phys. Rev. D108, 044053 (2023), arXiv:2304.03142[gr-qc]

  • [29]

    S. Babaket al. (Mock LISA Data Challenge Task Force), Class. Quant. Grav.27, 084009 (2010), arXiv:0912.0548[gr-qc]

  • [30]

    S. Sachdev, T. Regimbau, and B. S. Sathyaprakash, Phys. Rev. D102, 024051 (2020), arXiv:2002.05365[gr-qc]

  • [31]

    B. Zhou, L. Reali, E. Bertiet al.Compact Binary Foreground Subtraction in Next-Generation Ground-Based Observatories, (2022), arXiv: 2209.01221[gr-qc]

  • [32]

    D. S. Bellie, S. Banagiri, Z. Doctoret al.,The unresolved stochastic background from compact binary mergers detectable by nextgeneration ground-based gravitational-wave observatories, (2023), arXiv: 2310.02517[gr-qc]

  • [33]

    A. J. K. Chua, C. J. Moore, and J. R. Gair, Phys. Rev. D96, 044005 (2017), arXiv:1705.04259[gr-qc]

  • [34]

    T. Kupferet al.,LISA Galactic binaries with astrometry from Gaia DR3, (2023), arXiv: 2302.12719[astro-ph.SR]

  • [35]

    T. Kupferet al.,Lisa verification binaries, (2023)

  • [36]

    M. Volonteri, Astron. Astrophys. Rev.18, 279 (2010), arXiv:1003.4404[astro-ph.CO]

  • [37]

    A. Sesana, F. Haardt, P. Madauet al., Astrophys. J.611, 623 (2004), arXiv:astro-ph/0401543

  • [38]

    A. Kleinet al., Phys. Rev. D93, 024003 (2016), arXiv:1511.05581[grqc]

  • [39]

    S. Toonen, G. Nelemans, and S. P. Zwart, Astron. Astrophys.546, A70 (2012), arXiv:1208.6446[astro-ph.HE]

  • [40]

    T. Kupfer, V. Korol, S. Shahet al., Mon. Not. Roy. Astron. Soc.480, 302 (2018), arXiv:1805.00482[astro-ph.SR]

  • [41]

    S. Babak, H. Fang, J. R. Gairet al., Phys. Rev. D75, 024005 (2007), arXiv:gr-qc/0607007

  • [42]

    P. Amaro-Seoane, J. R. Gair, M. Freitaget al., Class. Quant. Grav.24, R113 (2007), arXiv:astro-ph/0703495

  • [43]

    Z. Luo, Y. Wang, Y. L. Wuet al.,The Taiji program: A concise overview, Progress of Theoretical and Experimental Physics2021(5), 05A108 (2020)

  • [44]

    J. Luoet al. (TianQin), Class. Quant. Grav.33, 035010 (2016), arXiv:1512.02076[astro-ph.IM]

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