-
[1]
M. Armano et al., Phys. Rev. Lett. 116, 231101 (2016)
-
[2]
P. Amaro-Seoane et al. (LISA), Laser Interferometer Space Antenna, (2017), arXiv: 1702.00786[astroph.IM]
-
[3]
P. Amaro Seoane et al. (LISA), Living Rev. Rel. 26, 2 (2023), arXiv:2203.06016[gr-qc]
-
[4]
L. Barack and C. Cutler, Phys. Rev. D 70, 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. Agazie et al. (NANOGrav), Astrophys. J. Lett. 951, L8 (2023), arXiv:2306.16213[astro-ph.HE]
-
[9]
G. Agazie et al. (NANOGrav), Astrophys. J. Lett. 951, L9 (2023), arXiv:2306.16217[astro-ph.HE]
-
[10]
A. Afzal et al. (NANOGrav), Astrophys. J. Lett. 951, L11 (2023), arXiv:2306.16219[astroph.HE]
-
[11]
J. Antoniadis et al. (EPTA, InPTA:), Astron. Astrophys. 678, A50 (2023), arXiv:2306.16214[astro-ph.HE]
-
[12]
J. Antoniadis et al. (EPTA), Astron. Astrophys. 678, A48 (2023), arXiv:2306.16224[astro-ph.HE]
-
[13]
D. J. Reardon et al., Astrophys. J. Lett. 951, L6 (2023), arXiv:2306.16215[astro-ph.HE]
-
[14]
A. Zic et al., The Parkes Pulsar Timing Array Third Data Release, (2023), arXiv: 2306.16230[astroph.HE]
-
[15]
R. D. Nan, D. Li, C. J. Jin et al., Int. J. Mod. Phys. D 20, 989 (2011), arXiv:1105.3794[astro-ph.IM]
-
[16]
H. Xu et al., Res. Astron. Astrophys. 23, 075024 (2023), arXiv:2306.16216[astro-ph.HE]
-
[17]
G. Agazie et al. (NANOGrav), Astrophys. J. Lett. 952, L37 (2023), arXiv:2306.16220[astro-ph.HE]
-
[18]
J. Antoniadis et 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. Chen et al., Sci. China Phys. Mech. Astron. 66, 120402 (2023), arXiv:2307.00722[astro-ph.CO]
-
[20]
J. Ellis, M. Fairbairn, G. Franciolini et 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. Fan et 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. Ajith et al., Phys. Rev. D 77, 104017 (2008), arXiv:0710.2335[gr-qc]
-
[24]
X. J. Zhu, E. Howell, T. Regimbau et 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. Aghanim et 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. Marsat et al., Phys. Rev. D 108, 044053 (2023), arXiv:2304.03142[gr-qc]
-
[29]
S. Babak et 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. D 102, 024051 (2020), arXiv:2002.05365[gr-qc]
-
[31]
B. Zhou, L. Reali, E. Berti et al. Compact Binary Foreground Subtraction in Next-Generation Ground-Based Observatories, (2022), arXiv: 2209.01221[gr-qc]
-
[32]
D. S. Bellie, S. Banagiri, Z. Doctor et 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. D 96, 044005 (2017), arXiv:1705.04259[gr-qc]
-
[34]
T. Kupfer et al., LISA Galactic binaries with astrometry from Gaia DR3, (2023), arXiv: 2302.12719[astro-ph.SR]
-
[35]
T. Kupfer et 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. Madau et al., Astrophys. J. 611, 623 (2004), arXiv:astro-ph/0401543
-
[38]
A. Klein et al., Phys. Rev. D 93, 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. Shah et al., Mon. Not. Roy. Astron. Soc. 480, 302 (2018), arXiv:1805.00482[astro-ph.SR]
-
[41]
S. Babak, H. Fang, J. R. Gair et al., Phys. Rev. D 75, 024005 (2007), arXiv:gr-qc/0607007
-
[42]
P. Amaro-Seoane, J. R. Gair, M. Freitag et al., Class. Quant. Grav. 24, R113 (2007), arXiv:astro-ph/0703495
-
[43]
Z. Luo, Y. Wang, Y. L. Wu et al., The Taiji program: A concise overview, Progress of Theoretical and Experimental Physics 2021 (5), 05A108 (2020)
-
[44]
J. Luo et al. (TianQin), Class. Quant. Grav. 33, 035010 (2016), arXiv:1512.02076[astro-ph.IM]