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Gravitational wave data analysis for the advanced detector era

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Academic year: 2020

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Figure

Figure 1.1: The Gaussian density distribution for the known pulsars contained in the ATNF Pulsar Catalogue (Hobbs et al., 2004).
Figure 1.2: The gaussian density distribution for the known pulsars contained in the ATNF Pulsar Catalogue (Hobbs et al., 2004), younger
Figure 1.3: Noise strain amplitude spectral density (ASD) curves of LIGO Hanford (H1) and Livingston (L1) for O2 averaged over 1800s
Figure 1.4: This figure shows h 90% 0 from eq.(1.59) for di↵erent values of T coh and f with a fixed T obs = 3months
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