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Dynamics Around Supermassive Black Holes: Extreme-mass-ratio Inspirals as Gravitational-wave Sources

  • Authors: Barak Rom, Itai Linial, Karamveer Kaur, Re'em Sari

Barak Rom et al 2024 The Astrophysical Journal 977 .

  • Provider: AAS Journals

Caption: Figure 5.

Characteristic strain of EMRIs as a function of the observed frequency. The black line is the LISA sensitivity curve (T. Robson et al. 2019) and the colored lines present contours of the observed source numbers, between 1 and 105, in a logarithmic frequency bin. The dashed lines present an analytical estimation at z ≪ 1 (Equation (40)), scaling as f 1/60 at low frequencies and f −19/60 at high frequencies. The color bar presents the source-frame SMBH mass that corresponds to the average redshift of the observed sources. The purple dotted line depicts the average SMBH mass M z= 105 M .

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