FrequencySeries
¶While gravitational-wave detectors are time-domain instruments, their sensitivity is frequency dependent and so is often measured as a power-spectral-density over the range of interesting gravitational-wave frequencies (~10-10,000 Hz). Additionally, the auxiliary channels used to sense and control instrumental operations each have their own frequency-domain characteristics, contributing to the overall sensitivity spectrum.
The FrequencySeries
object is used to represent any frequency series, including the power-spectral (and amplitude-spectral) density series describing instrument performance.
Analogously to the TimeSeries
, a new FrequencySeries
can be generated from any data sequence along with the minimal f0
and df
metadata:
>>> from gwpy.frequencyseries import FrequencySeries
>>> spec = FrequencySeries([1,2,3,4,5,6,7,8,9,10], f0=0, df=1)
>>> print(spec)
FrequencySeries([ 1 2 3 4 5 6 7 8 9 10],
name: None,
unit: None,
epoch: None,
channel: None,
f0: 0 Hz,
df: 1 Hz,
logf: False)
The full set of metadata that can be provided is as follows:
Name for this data set |
|
The physical unit of these data |
|
GPS epoch associated with these data |
|
Starting frequency for this |
|
Frequency spacing of this |
FrequencySeries
from a TimeSeries
¶The frequency-spectrum of a TimeSeries
can be calculated using either of the following methods:
Calculate the PSD |
|
Calculate the ASD |
In this example we expand upon plotting a TimeSeries
, by calculating the amplitude-spectral density of the gravitational-wave strain data from LHO:
>>> from gwpy.timeseries import TimeSeries
>>> gwdata = TimeSeries.get('H1:LDAS-STRAIN', 'September 16 2010 06:40',
... 'September 16 2010 06:50')
>>> spectrum = gwdata.asd(8, 4)
where the result is an average spectrum calculated using the Welch method.
FrequencySeries
¶Similary to the TimeSeries
, the FrequencySeries
object comes with its own plot()
method, which will quickly construct a Plot
:
>>> plot = spectrum.plot()
>>> ax = plot.gca()
>>> ax.set_xlim(40, 4000)
>>> ax.set_ylabel(r'GW strain ASD [strain$/\sqrt{\mathrm{Hz}}$]')
>>> ax.set_ylim(1e-23, 3e-20)
>>> plot.show()
(png)
FrequencySeries
applications¶FrequencySeries
reference¶A data array holding some metadata to represent a frequency series |
|
A 2-dimensional array containing the variance histogram of a frequency-series |