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Observation of gravitational waves from a binary black hole merger

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Figure

FIG. 1.The gravitational-wave event GW150914 observed by the LIGO Hanford (H1, left column panels) and Livingston (L1, rightdetector in the 35recovered from GW150914amount and inverted (to account for the detectorscolumn panels) detectors
FIG. 2.Top:post-Newtonian parameter Estimated gravitational-wave strain amplitudefrom GW150914 projected onto H1
FIG. 3.Simplified diagram of an Advanced LIGO detector (not to scale). A gravitational wave propagating orthogonally to theorientation of the LIGO detectors at Hanford, WA (H1) and Livingston, LA (L1).the time of the signal detection; this is an amplitude
FIG. 4.Search results from the generic transient search (left) and the binary coalescence search (right)
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