bilby.gw.utils
Functions
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Calculate the ASD from the frequency domain output of gaussian_noise() |
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Leading-order calculation of the time to merger from frequency |
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Converts inputs to floats, returns a list in the same order as the input |
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Get the merger time for known GW events using the gwosc package |
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Download information about a trigger from GraceDb and create cache files for finding gravitational-wave strain data. |
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A function which accesses the open strain data |
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Calculate the position of the IFO vertex in geocentric coordinates in meters. |
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Script to download a GraceDB candidate |
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Builds a gw_data_find call and process output |
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Calculate the inner product defined in the matched filter statistic |
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Safely call lalsimulation.SimInspiralChooseFDWaveform |
Safely call lalsimulation.SimInspiralChooseFDWaveformSequence |
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Safely call lalsimulation.SimInspiralFD |
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A numerically stable method to evaluate ln(I_0) a modified Bessel function of order 0 used in the phase-marginalized likelihood. |
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Calculate the _complex_ matched filter snr of a signal. |
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Calculate the noise weighted inner product between two arrays. |
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Compute the square of the optimal matched filter SNR for the provided signal. |
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Compute the overlap between two signals |
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Plot calibration posterior estimates for a spline model in log space. |
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Calculate the PSD from the frequency domain output of gaussian_noise() Calls asd_from_freq_series() and squares the output |
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A function which accesses the open strain data |
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Returns the angle in degrees corresponding to the spline calibration parameters delta_psi. |
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Convert from the 'detector frame' to the Earth frame. |
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Convert from the 'detector frame' to the Earth frame. |