Detectors¶
GW detectors description
Earth detectors¶
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class
gwtoolbox.detectors_earth.
LigoLike
(det)[source]¶ This class describes LIGO-like detectors
Parameters: det (int) – detector ID (0 - Virgo, 1 - LIGO, -1 - LIGO-like) -
ante_pattern
(theta, varphi, psi)[source]¶ The Antenna Pattern of LIGO-like (two arms with 90 deg) Gravitational Waves (GW) Observatories.
Parameters: Returns: size=2, [Fplus, Fcross]
Return type: (array of dtype float)
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noise_curve
(pars=None)[source]¶ The Noise power spectrum of LIGO-like GW observatories.
Parameters: pars (Optional[list of floats]) – which defines the configuration of the LIGO-like detector, this list of parameters will be passed to FINESSE Returns: noise vs. frequency, size=(,2), the 0-th column are frequencies, and 1-st column are corresponding noise power Return type: (array of dtype float)
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class
gwtoolbox.detectors_earth.
ETLike
(det)[source]¶ This class describes ET-like detectors
Parameters: det (int) – detector ID (2 - ET, -2 - ET-like) -
ante_pattern
(theta, varphi, psi, Nnest=3)[source]¶ The Antenna Pattern of ET-like (multiple detectors nested, each has two arms with 60 deg) Gravitational Waves (GW) Observatories.
Parameters: Returns: size=(Nnext,2). The i-th row are the Antenna Patterns [Fplus,Fcross] of the i-th nested detector
Return type: (array of dtype float)
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noise_curve
(pars=None)[source]¶ The Noise power spectrum of ET-like GW observatories.
Parameters: pars (Optional[list of floats]) – define the configuration of the ET-like detector, this list of parameters will be passed to FINESSE ??? Returns: noise vs. frequency, size=(,2), the 0-th column are frequencies, and 1-st column are corresponding noise power Return type: (array of dtype float)
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Simulate LIGO-like detector¶
Space detectors¶
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class
gwtoolbox.detectors_space.
LisaLike
(det)[source]¶ This class describes LISA-like detectors
Parameters: det (int) – detector ID (3 - LISA, -3 - LISA-like) -
ante_pattern
()[source]¶ The Antenna Pattern of LISA-like Gravitational Waves Observatories.
Parameters:
Returns: antenna pattern Return type: (array of dtype float)
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noise_curve
(pars=None)[source]¶ The Noise power spectrum of LISA-like GW observatories.
Parameters: pars (Optional[list of floats]) – which defines the configuration of the LISA-like detector Returns: noise vs. frequency, size=(,2), the 0-th column are frequencies, and 1-st column are corresponding noise power Return type: (array of dtype float)
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