Reference on kuibit.sensitivity_curves¶
The sensitivity_curves
module contains the power spectral
distribution of the noise of known detectors. The available ones are:
- kuibit.sensitivity_curves.Sn_CE1(freqs)[source]¶
Return the average power spectral density noise for Einstein Telescope in 1/Hz.
Note
The data was downloaded from https://cosmicexplorer.org/data/CE1_strain.txt and has range
fmin=3
,fmax=10000
(Hz).The resampling to the requested frequencies is done considering the values of the nearest neighbors.
- Parameters
freqs (1d NumPy array) – Frequencies in Hz over which to evaluate the sensitivity curve.
- Returns
CE1 sensitivity curve in 1/Hz.
- Return type
- kuibit.sensitivity_curves.Sn_CE2(freqs)[source]¶
Return the average power spectral density noise for Einstein Telescope in 1/Hz.
Note
The data was downloaded from https://cosmicexplorer.org/data/CE2_strain.txt and has range
fmin=3
,fmax=10000
(Hz).The resampling to the requested frequencies is done considering the values of the nearest neighbors.
- Parameters
freqs (1d NumPy array) – Frequencies in Hz over which to evaluate the sensitivity curve.
- Returns
CE2 sensitivity curve in 1/Hz.
- Return type
- kuibit.sensitivity_curves.Sn_ET_B(freqs)[source]¶
Return the average power spectral density noise for Einstein Telescope (variant B) in 1/Hz.
Note
The data was downloaded from https://apps.et-gw.eu/tds/?content=3&r=14323 and has range
fmin=1
,fmax=10000
(Hz).- Parameters
freqs (1d NumPy array) – Frequencies in Hz over which to evaluate the sensitivity curve.
- Returns
ET-B sensitivity curve in 1/Hz.
- Return type
- kuibit.sensitivity_curves.Sn_KAGRA_D(freqs)[source]¶
Return the average power spectral density noise for KAGRA in 1/Hz.
Note
The data was downloaded from https://granite.phys.s.u-tokyo.ac.jp/svn/LCGT/trunk/sensitivity/spectrum/BW2009_VRSED.dat and has range
fmin=1.00231
,fmax=10000
(Hz).The resampling to the requested frequencies is done considering the values of the nearest neighbors.
- Parameters
freqs (1d NumPy array) – Frequencies in Hz over to evaluate the sensitivity curve.
- Returns
KAGRA sensitivity curve in 1/Hz.
- Return type
- kuibit.sensitivity_curves.Sn_LISA(freqs, arms_length=2500000000.0)[source]¶
Return the average power spectral density noise for LISA in 1/Hz.
The expression implemented is Equation (13) in https://arxiv.org/abs/1803.01944.
- Parameters
freqs (1d NumPy array) – Frequencies in Hz over which to evaluate the sensitivity curve.
arms_length (float) – Length of the detector’s arms in meters.
- Returns
LISA sensitivity curve in 1/Hz.
- Return type
- kuibit.sensitivity_curves.Sn_aLIGO(freqs)[source]¶
Return the average power spectral density noise for advanced LIGO in 1/Hz. This is the Zero-Detuned-High-Power noise curve.
Note
The data was downloaded from https://dcc.ligo.org/LIGO-T1500293-v11/public and has range
fmin=9
,fmax=8192
(Hz).The resampling to the requested frequencies is done considering the values of the nearest neighbors.
- Parameters
freqs (1d NumPy array) – Frequencies in Hz over to evaluate the sensitivity curve.
- Returns
Advanced LIGO Zero-Detuned High-Power sensitivity curve in 1/Hz.
- Return type
- kuibit.sensitivity_curves.Sn_aLIGO_plus(freqs)[source]¶
Return the average power spectral density noise for Advanced LIGO + in 1/Hz.
Note
The data was downloaded from https://dcc.ligo.org/public/0149/T1800042/005/AplusDesign.txt and has range
fmin=5
,fmax=5000
(Hz).The resampling to the requested frequencies is done considering the values of the nearest neighbors.
- Parameters
freqs (1d NumPy array) – Frequencies in Hz over to evaluate the sensitivity curve.
- Returns
aLIGO+ sensitivity curve in 1/Hz.
- Return type
- kuibit.sensitivity_curves.Sn_voyager(freqs)[source]¶
Return the average power spectral density noise for voyager in 1/Hz.
Note
The data was downloaded from https://dcc.ligo.org/LIGO-T1500293-v11/public and has range
fmin=5
,fmax=10000
(Hz).The resampling to the requested frequencies is done considering the values of the nearest neighbors.
- Parameters
freqs (1d NumPy array) – Frequencies in Hz over to evaluate the sensitivity curve.
- Returns
Voyager sensitivity curve in 1/Hz.
- Return type