Duncan A. Brown1,2
1Department of Physics, Syracuse University, Syracuse, NY 13244, USA
2DARK, Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, 2100 Copenhagen, Denmark
This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version.
This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details.
You should have received a copy of the GNU General Public License along with this program. If not, see http://www.gnu.org/licenses/.
This notebook demonstrates using the pycbc_inspiral program to find the triggers from the LIGO Hanford and Livingston observatories corresponding to GW150914 event. This notebook uses the publically available frame data from the LIGO Open Science Center (LOSC), input files from the PyCBC Configuration GitHub repository, and code from the PyCBC GitHub repository.
This notebook can be run from the PyCBC Docker container, or a machine with PyCBC installed. Instructions for downloading the docker container are available from the PyCBC home page. To start a container with instance of Jupyter notebook, run the commands
docker pull pycbc/pycbc-el7:v1.7.5
docker run -p 8888:8888 --name pycbc_notebook -it pycbc/pycbc-el7:v1.7.5 /bin/bash -l
Once the container has started, this notebook can be downloaded with the command:
curl -L https://raw.githubusercontent.com/ligo-cbc/pycbc/master/examples/gw150914/PyCBCInspiral.ipynb > PyCBCInspiral.ipynb
The notebook server can be started inside the container with the command:
jupyter notebook --ip 0.0.0.0 --no-browser
You can then connect to the notebook at the URL printed by jupyter.
There are several (arbitrary) choices that can be made when constructing a matched filter for binary mergers, including the overall normalization of the signal-to-noise ratio, the reference time in the waveform for which the search reports the arrival time, and a scale factor to keep numerical quantites close to unity to prevent round-off error. Understanding these choices is essential for interpreting the reported time, phase, and amplitude needed to construct the best-fit waveform for a signal.
pycbc_inspiral used the FindChirp algorithm for matched filtering. For details of the choices made by the algorithm used here, see chapter 4 of Duncan Brown's PhD thesis and the FindChirp paper in Phys Rev D.
In [1]:
% matplotlib inline
% config InlineBackend.figure_format = 'retina'
from matplotlib import rcParams
rcParams['figure.figsize']=(14,5)
import numpy as np
import matplotlib.pyplot as plt
import pycbc.types
import pycbc.fft
import pycbc.io.hdf
import pycbc.waveform
from pycbc import DYN_RANGE_FAC
In [2]:
!if [ ! -f H-H1_LOSC_16_V2-1126257414-4096.gwf ] ; then curl https://losc.ligo.org/s/events/GW150914/H-H1_LOSC_16_V2-1126257414-4096.gwf > H-H1_LOSC_16_V2-1126257414-4096.gwf ; fi
!if [ ! -f L-L1_LOSC_16_V2-1126257414-4096.gwf ] ; then curl https://losc.ligo.org/s/events/GW150914/L-L1_LOSC_16_V2-1126257414-4096.gwf > L-L1_LOSC_16_V2-1126257414-4096.gwf ; fi
These files are used to window out times when there are large delta function glitches in the input strain data that are identified by the Omicron burst search. This proceedure for identifying and removing these times from the search is described in the paper GW150914: First results from the search for binary black hole coalescence with Advanced LIGO.
In [3]:
!if [ ! -f H1-gating_C01_SNR300-1126051217-1129383017.txt.gz ] ; then curl -L https://raw.githubusercontent.com/ligo-cbc/pycbc-config/1e9aee13ebf85e916136afc4a9ae57f5b2d5bc64/O1/dq/H1-gating_C01_SNR300-1126051217-1129383017.txt.gz > H1-gating_C01_SNR300-1126051217-1129383017.txt.gz ; fi
!if [ ! -f L1-gating_C01_SNR300-1126051217-1129383017.txt.gz ] ; then curl -L https://raw.githubusercontent.com/ligo-cbc/pycbc-config/1e9aee13ebf85e916136afc4a9ae57f5b2d5bc64/O1/dq/L1-gating_C01_SNR300-1126051217-1129383017.txt.gz > L1-gating_C01_SNR300-1126051217-1129383017.txt.gz ; fi
A bank of template parameters is needed as input to pycbc_inspiral. The code will search over each template in the bank for a matching signal in the input strain data. The full template bank used in the GW150914 search contains approximately 250,000 templates. Since we are only going to look at GW150914, we download a template bank containing only the template that best matches GW150915. This is the template indicated by a circle in Figure 1 of the paper GW150914: First results from the search for binary black hole coalescence with Advanced LIGO.
In [4]:
!if [ ! -f H1L1-GW150914_BANK-1126051217-3331800.xml ] ; then curl -L https://raw.githubusercontent.com/ligo-cbc/pycbc-config/master/O1/bank/H1L1-GW150914_BANK-1126051217-3331800.xml > H1L1-GW150914_BANK-1126051217-3331800.xml ; fi
In order to use the template bank with the PyCBC trigger processing tools, we convert the XML format bank to HDF5.
In [5]:
!rm -f H1L1-GW150914_BANK-1126051217-3331800.hdf
!pycbc_coinc_bank2hdf --verbose --bank-file H1L1-GW150914_BANK-1126051217-3331800.xml --output H1L1-GW150914_BANK-1126051217-3331800.hdf
The following cells are based on downloading pycbc_inspiral from the v1.7.5 release of PyCBC. The production GW150914 search used the v1.3.2 release of PyCBC. PyCBC's Travis CI build and test suite ensures that the results of the code have not changed since this v1.3.2 release, when the code is run with the same parameters used to report the detection of GW150914 in the discovery PRL.
pycbc_inspiral is a stand-alone program that is designed to be run from the command line. To run it within an IPython notebook, we first download it with the %load command. We then modify the code to place the main program in the function
def findchirp(subtract_waveform=None):
# main pycbc_inspiral code goes here
return [snr, norm, corr, idx, snrv], bank, segments, gwstrain
This allows us to run the code with the findchirp() function in this notebook and access the internal data structures of the code.
The argument subtract_waveform allows us to pass a pycbc.types.TimeSeries that is subtracted from the strain data prior to filtering. To do this, we add the lines
if subtract_waveform:
logging.info('Removing waveform from input strain data')
gwstrain -= subtract_waveform
after reading in the gwstrain using strain.from_cli().
Other than these modifications, the code is identical to the production filtering code.
In [6]:
# %load https://raw.githubusercontent.com/ligo-cbc/pycbc/v1.7.5/bin/pycbc_inspiral
#!/usr/bin/env python
# Copyright (C) 2014 Alex Nitz
#
# This program is free software; you can redistribute it and/or modify it
# under the terms of the GNU General Public License as published by the
# Free Software Foundation; either version 3 of the License, or (at your
# option) any later version.
#
# This program is distributed in the hope that it will be useful, but
# WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General
# Public License for more details.
#
# You should have received a copy of the GNU General Public License along
# with this program; if not, write to the Free Software Foundation, Inc.,
# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
import sys
import logging, argparse, numpy, itertools
import pycbc
import pycbc.version
from pycbc import vetoes, psd, waveform, strain, scheme, fft, DYN_RANGE_FAC, events
from pycbc.vetoes.sgchisq import SingleDetSGChisq
from pycbc.filter import MatchedFilterControl, make_frequency_series, qtransform
from pycbc.types import TimeSeries, FrequencySeries, zeros, float32, complex64
import pycbc.fft.fftw, pycbc.version
import pycbc.opt
import pycbc.inject
import time
last_progress_update = -1.0
def update_progress(p,u,n):
""" updates a file 'progress.txt' with a value 0 .. 1.0 when enough (filtering) progress was made
"""
global last_progress_update
if p > last_progress_update + u:
f = open(n,"w")
if f:
f.write("%.4f" % p)
f.close()
last_progress_update = p
def findchirp(subtract_waveform=None):
global last_progress_update
tstart = time.time()
parser = argparse.ArgumentParser(usage='',
description="Find single detector gravitational-wave triggers.")
parser.add_argument('--version', action=pycbc.version.Version)
parser.add_argument("-V", "--verbose", action="store_true",
help="print extra debugging information", default=False )
parser.add_argument("--update-progress",
help="updates a file 'progress.txt' with a value 0 .. 1.0 when this amount of (filtering) progress was made",
type=float, default=0)
parser.add_argument("--update-progress-file",
help="name of the file to write the amount of (filtering) progress to",
type=str, default="progress.txt")
parser.add_argument("--output", type=str, help="FIXME: ADD")
parser.add_argument("--bank-file", type=str, help="FIXME: ADD")
parser.add_argument("--snr-threshold",
help="SNR threshold for trigger generation", type=float)
parser.add_argument("--newsnr-threshold", type=float, metavar='THRESHOLD',
help="Cut triggers with NewSNR less than THRESHOLD")
parser.add_argument("--low-frequency-cutoff", type=float,
help="The low frequency cutoff to use for filtering (Hz)")
parser.add_argument("--enable-bank-start-frequency", action='store_true',
help="Read the starting frequency of template waveforms"
" from the template bank.")
parser.add_argument("--max-template-length", type=float,
help="The maximum length of a template is seconds. The "
"starting frequency of the template is modified to "
"ensure the proper length")
parser.add_argument("--enable-q-transform", action='store_true',
help="compute the q-transform for each segment of a "
"given analysis run. (default = False)")
# add approximant arg
pycbc.waveform.bank.add_approximant_arg(parser)
parser.add_argument("--order", type=int,
help="The integer half-PN order at which to generate"
" the approximant. Default is -1 which indicates to use"
" approximant defined default.", default=-1,
choices = numpy.arange(-1, 9, 1))
taper_choices = ["start","end","startend"]
parser.add_argument("--taper-template", choices=taper_choices,
help="For time-domain approximants, taper the start and/or"
" end of the waveform before FFTing.")
parser.add_argument("--cluster-method", choices=["template", "window"],
help="FIXME: ADD")
parser.add_argument("--cluster-function", choices=["findchirp", "symmetric"],
help="How to cluster together triggers within a window. "
"'findchirp' uses a forward sliding window; 'symmetric' "
"will compare each window to the one before and after, keeping "
"only a local maximum.", default="findchirp")
parser.add_argument("--cluster-window", type=float, default = -1,
help="Length of clustering window in seconds."
" Set to 0 to disable clustering.")
parser.add_argument("--maximization-interval", type=float, default=0,
help="Maximize triggers over the template bank (ms)")
parser.add_argument("--bank-veto-bank-file", type=str, help="FIXME: ADD")
parser.add_argument("--chisq-snr-threshold", type=float,
help="Minimum SNR to calculate the power chisq")
parser.add_argument("--chisq-bins", default=0, help=
"Number of frequency bins to use for power chisq. Specify"
" an integer for a constant number of bins, or a function "
"of template attributes. Math functions are "
"allowed, ex. "
"'10./math.sqrt((params.mass1+params.mass2)/100.)'. "
"Non-integer values will be rounded down.")
parser.add_argument("--chisq-threshold", type=float, default=0,
help="FIXME: ADD")
parser.add_argument("--chisq-delta", type=float, default=0, help="FIXME: ADD")
parser.add_argument("--autochi-number-points", type=int, default=0,
help="The number of points to use, in both directions if"
"doing a two-sided auto-chisq, to calculate the"
"auto-chisq statistic.")
parser.add_argument("--autochi-stride", type=int, default=0,
help="The gap, in sample points, between the points at"
"which to calculate auto-chisq.")
parser.add_argument("--autochi-two-phase", action="store_true",
default=False,
help="If given auto-chisq will be calculated by testing "
"against both phases of the SNR time-series. "
"If not given, only the phase matching the trigger "
"will be used.")
parser.add_argument("--autochi-onesided", action='store', default=None,
choices=['left','right'],
help="Decide whether to calculate auto-chisq using"
"points on both sides of the trigger or only on one"
"side. If not given points on both sides will be"
"used. If given, with either 'left' or 'right',"
"only points on that side (right = forward in time,"
"left = back in time) will be used.")
parser.add_argument("--autochi-reverse-template", action="store_true",
default=False,
help="If given, time-reverse the template before"
"calculating the auto-chisq statistic. This will"
"come at additional computational cost as the SNR"
"time-series will need recomputing for the time-"
"reversed template.")
parser.add_argument("--autochi-max-valued", action="store_true",
default=False,
help="If given, store only the maximum value of the auto-"
"chisq over all points tested. A disadvantage of this "
"is that the mean value will not be known "
"analytically.")
parser.add_argument("--autochi-max-valued-dof", action="store", metavar="INT",
type=int,
help="If using --autochi-max-valued this value denotes "
"the pre-calculated mean value that will be stored "
"as the auto-chisq degrees-of-freedom value.")
parser.add_argument("--downsample-factor", type=int,
help="Factor that determines the interval between the "
"initial SNR sampling. If not set (or 1) no sparse sample "
"is created, and the standard full SNR is calculated.", default=1)
parser.add_argument("--upsample-threshold", type=float,
help="The fraction of the SNR threshold to check the sparse SNR sample.")
parser.add_argument("--upsample-method", choices=["pruned_fft"],
help="The method to find the SNR points between the sparse SNR sample.",
default='pruned_fft')
parser.add_argument("--user-tag", type=str, metavar="TAG", help="""
This is used to identify FULL_DATA jobs for
compatibility with pipedown post-processing.
Option will be removed when no longer needed.""")
parser.add_argument("--keep-loudest-interval", type=float,
help="Window in seconds to maximize triggers over bank")
parser.add_argument("--keep-loudest-num", type=int,
help="Number of triggers to keep from each maximization interval")
parser.add_argument("--gpu-callback-method", default='none')
parser.add_argument("--use-compressed-waveforms", action="store_true", default=False,
help='Use compressed waveforms from the bank file.')
parser.add_argument("--waveform-decompression-method", action='store', default=None,
help='Method to be used decompress waveforms from the bank file.')
# Add options groups
psd.insert_psd_option_group(parser)
strain.insert_strain_option_group(parser)
strain.StrainSegments.insert_segment_option_group(parser)
scheme.insert_processing_option_group(parser)
fft.insert_fft_option_group(parser)
pycbc.opt.insert_optimization_option_group(parser)
pycbc.inject.insert_injfilterrejector_option_group(parser)
SingleDetSGChisq.insert_option_group(parser)
opt = parser.parse_args()
# Check that the values returned for the options make sense
psd.verify_psd_options(opt, parser)
strain.verify_strain_options(opt, parser)
strain.StrainSegments.verify_segment_options(opt, parser)
scheme.verify_processing_options(opt, parser)
fft.verify_fft_options(opt,parser)
pycbc.opt.verify_optimization_options(opt, parser)
pycbc.init_logging(opt.verbose)
inj_filter_rejector = pycbc.inject.InjFilterRejector.from_cli(opt)
ctx = scheme.from_cli(opt)
gwstrain = strain.from_cli(opt, dyn_range_fac=DYN_RANGE_FAC,
inj_filter_rejector=inj_filter_rejector)
# Add code to subtract a waveform from the input time series
if subtract_waveform:
logging.info('Removing waveform from input strain data')
gwstrain -= subtract_waveform
strain_segments = strain.StrainSegments.from_cli(opt, gwstrain)
with ctx:
fft.from_cli(opt)
flow = opt.low_frequency_cutoff
flen = strain_segments.freq_len
tlen = strain_segments.time_len
delta_f = strain_segments.delta_f
logging.info("Making frequency-domain data segments")
segments = strain_segments.fourier_segments()
psd.associate_psds_to_segments(opt, segments, gwstrain, flen, delta_f,
flow, dyn_range_factor=DYN_RANGE_FAC, precision='single')
# storage for values and types to be passed to event manager
out_types = {
'time_index' : int,
'snr' : complex64,
'chisq' : float32,
'chisq_dof' : int,
'bank_chisq' : float32,
'bank_chisq_dof' : int,
'cont_chisq' : float32,
}
out_types.update(SingleDetSGChisq.returns)
out_vals = {key: None for key in out_types}
names = sorted(out_vals.keys())
if len(strain_segments.segment_slices) == 0:
logging.info("--filter-inj-only specified and no injections in analysis time")
event_mgr = events.EventManager(
opt, names, [out_types[n] for n in names], psd=None,
gating_info=gwstrain.gating_info)
event_mgr.finalize_template_events()
event_mgr.write_events(opt.output)
logging.info("Finished")
sys.exit(0)
if opt.enable_q_transform:
logging.info("Performing q-transform on analysis segments")
q_trans = qtransform.inspiral_qtransform_generator(segments)
else:
q_trans = {}
# FIXME: Maybe we should use the PSD corresponding to each trigger
event_mgr = events.EventManager(
opt, names, [out_types[n] for n in names], psd=segments[0].psd,
gating_info=gwstrain.gating_info, q_trans=q_trans)
template_mem = zeros(tlen, dtype = complex64)
cluster_window = int(opt.cluster_window * gwstrain.sample_rate)
if opt.cluster_window == 0.0:
use_cluster = False
else:
use_cluster = True
if hasattr(ctx, "num_threads"):
ncores = ctx.num_threads
else:
ncores = 1
matched_filter = MatchedFilterControl(opt.low_frequency_cutoff, None,
opt.snr_threshold, tlen, delta_f, complex64,
segments, template_mem, use_cluster,
downsample_factor=opt.downsample_factor,
upsample_threshold=opt.upsample_threshold,
upsample_method=opt.upsample_method,
gpu_callback_method=opt.gpu_callback_method,
cluster_function=opt.cluster_function)
bank_chisq = vetoes.SingleDetBankVeto(opt.bank_veto_bank_file,
flen, delta_f, flow, complex64,
phase_order=opt.order,
approximant=opt.approximant)
power_chisq = vetoes.SingleDetPowerChisq(opt.chisq_bins, opt.chisq_snr_threshold)
autochisq = vetoes.SingleDetAutoChisq(opt.autochi_stride,
opt.autochi_number_points,
onesided=opt.autochi_onesided,
twophase=opt.autochi_two_phase,
reverse_template=opt.autochi_reverse_template,
take_maximum_value=opt.autochi_max_valued,
maximal_value_dof=opt.autochi_max_valued_dof)
logging.info("Overwhitening frequency-domain data segments")
for seg in segments:
seg /= seg.psd
logging.info("Read in template bank")
bank = waveform.FilterBank(opt.bank_file, flen, delta_f,
low_frequency_cutoff=None if opt.enable_bank_start_frequency else flow,
dtype=complex64, phase_order=opt.order,
taper=opt.taper_template, approximant=opt.approximant,
out=template_mem, max_template_length=opt.max_template_length,
enable_compressed_waveforms=True if opt.use_compressed_waveforms else False,
waveform_decompression_method=
opt.waveform_decompression_method if opt.use_compressed_waveforms else None)
sg_chisq = SingleDetSGChisq.from_cli(opt, bank, opt.chisq_bins)
ntemplates = len(bank)
nfilters = 0
logging.info("Full template bank size: %s", ntemplates)
bank.template_thinning(inj_filter_rejector)
if not len(bank) == ntemplates:
logging.info("Template bank size after thinning: %s", len(bank))
tsetup = time.time() - tstart
# Note: in the class-based approach used now, 'template' is not explicitly used
# within the loop. Rather, the iteration simply fills the memory specifed in
# the 'template_mem' argument to MatchedFilterControl with the next template
# from the bank.
for t_num in xrange(len(bank)):
tmplt_generated = False
for s_num, stilde in enumerate(segments):
# Filter check checks the 'inj_filter_rejector' options to
# determine whether
# to filter this template/segment if injections are present.
if not inj_filter_rejector.template_segment_checker(
bank, t_num, stilde, opt.gps_start_time):
continue
if not tmplt_generated:
template = bank[t_num]
event_mgr.new_template(tmplt=template.params,
sigmasq=template.sigmasq(segments[0].psd))
tmplt_generated = True
if opt.cluster_method == "window":
cluster_window = int(opt.cluster_window * gwstrain.sample_rate)
if opt.cluster_method == "template":
cluster_window = \
int(template.chirp_length * gwstrain.sample_rate)
if opt.update_progress:
update_progress((t_num + (s_num / float(len(segments))) ) / len(bank),
opt.update_progress, opt.update_progress_file)
logging.info("Filtering template %d/%d segment %d/%d" %
(t_num + 1, len(bank), s_num + 1, len(segments)))
nfilters = nfilters + 1
snr, norm, corr, idx, snrv = \
matched_filter.matched_filter_and_cluster(s_num,
template.sigmasq(stilde.psd),
cluster_window,
epoch=stilde._epoch)
if not len(idx):
continue
out_vals['bank_chisq'], out_vals['bank_chisq_dof'] = \
bank_chisq.values(template, stilde.psd, stilde, snrv, norm,
idx+stilde.analyze.start)
out_vals['chisq'], out_vals['chisq_dof'] = \
power_chisq.values(corr, snrv, norm, stilde.psd,
idx+stilde.analyze.start, template)
out_vals['sg_chisq'] = sg_chisq.values(stilde, template, stilde.psd,
snrv, norm,
out_vals['chisq'],
out_vals['chisq_dof'],
idx+stilde.analyze.start)
out_vals['cont_chisq'] = \
autochisq.values(snr, idx+stilde.analyze.start, template,
stilde.psd, norm, stilde=stilde,
low_frequency_cutoff=flow)
idx += stilde.cumulative_index
out_vals['time_index'] = idx
out_vals['snr'] = snrv * norm
event_mgr.add_template_events(names, [out_vals[n] for n in names])
event_mgr.cluster_template_events("time_index", "snr", cluster_window)
event_mgr.finalize_template_events()
logging.info("Found %s triggers" % str(len(event_mgr.events)))
if opt.chisq_threshold and opt.chisq_bins:
logging.info("Removing triggers with poor chisq")
event_mgr.chisq_threshold(opt.chisq_threshold, opt.chisq_bins,
opt.chisq_delta)
logging.info("%d remaining triggers" % len(event_mgr.events))
if opt.newsnr_threshold and opt.chisq_bins:
logging.info("Removing triggers with NewSNR below threshold")
event_mgr.newsnr_threshold(opt.newsnr_threshold)
logging.info("%d remaining triggers" % len(event_mgr.events))
if opt.keep_loudest_interval:
logging.info("Removing triggers that are not within the top %s loudest"
" of a %s second interval" % (opt.keep_loudest_num,
opt.keep_loudest_interval))
event_mgr.keep_loudest_in_interval(opt.keep_loudest_interval * opt.sample_rate,
opt.keep_loudest_num)
logging.info("%d remaining triggers" % len(event_mgr.events))
if opt.injection_window and hasattr(gwstrain, 'injections'):
logging.info("Keeping triggers within %s seconds of injection" % opt.injection_window)
event_mgr.keep_near_injection(opt.injection_window, gwstrain.injections)
logging.info("%d remaining triggers" % len(event_mgr.events))
if opt.maximization_interval:
logging.info("Maximizing triggers over %s ms window" % opt.maximization_interval)
window = int(opt.maximization_interval * gwstrain.sample_rate / 1000)
event_mgr.maximize_over_bank("time_index", "snr", window)
logging.info("%d remaining triggers" % len(event_mgr.events))
tstop = time.time()
run_time = tstop - tstart
event_mgr.save_performance(ncores, nfilters, ntemplates, run_time, tsetup)
logging.info("Writing out triggers")
event_mgr.write_events(opt.output)
if opt.fftw_output_float_wisdom_file:
fft.fftw.export_single_wisdom_to_filename(opt.fftw_output_float_wisdom_file)
if opt.fftw_output_double_wisdom_file:
fft.fftw.export_double_wisdom_to_filename(opt.fftw_output_double_wisdom_file)
logging.info("Finished")
return [snr * 1, norm, corr * 1, idx, snrv], bank, segments, gwstrain
To run the code, we first set up the command line arguments for pycbc_inspiral before calling the findchirp() function. The command line arguments below are taken from the production analysis for the GW150914 result. We first run the code for the LIGO Hanford detector, and then for the LIGO Livingston detector.
The only difference between the command line arguments and the production arguments used in the discovery PRL are:
--trig-start-time and --trig-end-time arguments that determine how much data will be searched for triggers are set to a 64 second interval centered the GPS time of GW150914 (1126259462) to avoid unncessary computation.SEONBRv2 time-domain template, rather than the SEOBNRv2_DoubleSpinROM frequency-domain template, as the using a time-domain waveform makes this notebook slightly simpler.
In [7]:
search_f_low = 25.0
argv = ['pycbc_inspiral', '--verbose',
'--approximant=SEOBNRv2', '--order=-1', '--taper-template=start',
'--bank-file=H1L1-GW150914_BANK-1126051217-3331800.xml',
'--pad-data=8', '--sample-rate=4096', '--strain-high-pass=20',
'--segment-length=256', '--segment-start-pad=112', '--segment-end-pad=16',
'--psd-estimation=median', '--psd-segment-stride=8', '--psd-segment-length=16', '--psd-inverse-length=16',
'--low-frequency-cutoff={}'.format(search_f_low),
'--trig-start-time=1126259430', '--trig-end-time=1126259494',
"--chisq-bins=0.4*get_freq('fSEOBNRv2Peak',params.mass1,params.mass2,params.spin1z,params.spin2z)**(2./3.)",
'--snr-threshold=5.5', '--newsnr-threshold=5',
'--cluster-method=window', '--cluster-window=4', '--cluster-function=symmetric',
'--injection-window=4.5', '--filter-inj-only',
'--processing-scheme=cpu']
In [8]:
argv_h1_data = ['--frame-files=H-H1_LOSC_16_V2-1126257414-4096.gwf', '--channel-name=H1:LOSC-STRAIN',
'--gps-start-time=1126257636', '--gps-end-time=1126259684',
'--gating-file=H1-gating_C01_SNR300-1126051217-1129383017.txt.gz'
]
In [9]:
argv_h1_out = ['--output=H1-INSPIRAL_FULL_DATA_JOB0-1126257771-1837.hdf']
In [10]:
argv_h1 = argv + argv_h1_data + argv_h1_out
sys.argv = argv_h1
In [11]:
!rm -f H1-INSPIRAL_FULL_DATA_JOB0-1126257771-1837.hdf
h1_result = findchirp()
In [12]:
argv_l1_data = ['--frame-files=L-L1_LOSC_16_V2-1126257414-4096.gwf', '--channel-name=L1:LOSC-STRAIN',
'--gps-start-time=1126258108', '--gps-end-time=1126260156',
'--gating-file=L1-gating_C01_SNR300-1126051217-1129383017.txt.gz'
]
In [13]:
argv_l1_out = ['--output=L1-INSPIRAL_FULL_DATA_JOB0-1126258302-1591.hdf']
In [14]:
argv_l1 = argv + argv_l1_data + argv_l1_out
sys.argv = argv_l1
In [15]:
!rm -f L1-INSPIRAL_FULL_DATA_JOB0-1126258302-1591.hdf
l1_result = findchirp()
In [16]:
h1_triggers = pycbc.io.hdf.SingleDetTriggers(
'H1-INSPIRAL_FULL_DATA_JOB0-1126257771-1837.hdf',
'H1L1-GW150914_BANK-1126051217-3331800.hdf',
None, None, None, 'H1'
)
l1_triggers = pycbc.io.hdf.SingleDetTriggers(
'L1-INSPIRAL_FULL_DATA_JOB0-1126258302-1591.hdf',
'H1L1-GW150914_BANK-1126051217-3331800.hdf',
None, None, None, 'L1'
)
imax = np.argmax(h1_triggers.snr)
t_h1 = h1_triggers.end_time[imax]
t_idx_h1 = h1_result[0][3][np.argmax(np.abs(h1_result[0][4]))]
snr_h1 = h1_triggers.snr[imax]
sigmasq = h1_triggers.get_column('sigmasq')[0]
eff_distance_h1 = (sigmasq)**0.5 / snr_h1
imax = np.argmax(l1_triggers.snr)
t_l1 = l1_triggers.end_time[imax]
t_idx_l1 = l1_result[0][3][np.argmax(np.abs(l1_result[0][4]))]
snr_l1 = l1_triggers.snr[imax]
sigmasq = l1_triggers.get_column('sigmasq')[0]
eff_distance_l1 = (sigmasq)**0.5 / snr_l1
We print the arrival time, signal-to-noise ratio, and time delay for the H1 and L1 triggers. We also print the effective distance measured by the search code, as this is needed to scale the amplitude of the best-fit template.
pycbc_inspiral records the sample index of the trigger, relative to the start of the strain time series that is read in. We save this arrival time offset as it will be used later to set the arrival time of the best-fit template.
In [17]:
print "H1 Time of event is {} with signal-to-noise ratio {}".format(t_h1, snr_h1)
print "L1 Time of event is {} with signal-to-noise ratio {}".format(t_l1, snr_l1)
print "HL arrival time difference = {} ms".format(t_h1-t_l1)
print "H1 Effective distance = {} Mpc, L1 effective distance = {} Mpc".format(eff_distance_h1, eff_distance_l1)
print "H1 arrival time offset = {}, L1 arrival time offset = {}".format(t_idx_h1,t_idx_l1)
Now we plot the signal-to-noise ratio time series for each detector. The filtering function used by pycbc_inspiral generates the complex signal-to-noise ratio time series. In our code, this is returned in the array h1_result[0][0]. The complex signal-to-noise ratio is scaled by a normalization factor stored in h1_result[0][1]. We plot the absolute value of the complex signal-to-noise, relative to GPS time 1126259462. For comparison, we draw vertical lines at the time of the GW150914 trigger. It can be seen that the signal-to-noise ratio time series peaks at the time of the trigger, as expected. We also store the array index of this peak, as we will use this to compute the phase of the best-fit template.
In [18]:
h1_complex_snr = h1_result[0][0] * h1_result[0][1]
h1_complex_snr.start_time -= 1126259462
h1_complex_snr = h1_complex_snr.time_slice(0.3, 0.5)
h1_snr_data = abs(h1_complex_snr)
h1_imax = h1_snr_data.abs_arg_max()
l1_complex_snr = l1_result[0][0] * l1_result[0][1]
l1_complex_snr.start_time -= 1126259462
l1_complex_snr = l1_complex_snr.time_slice(0.3, 0.5)
l1_snr_data = abs(l1_complex_snr)
l1_imax = l1_snr_data.abs_arg_max()
plt.plot(h1_snr_data.sample_times, h1_snr_data, color='r', label="H1")
plt.axvline(t_h1 - 1126259462, color='r', linestyle=':')
plt.plot(l1_snr_data.sample_times, l1_snr_data, color='g', label="L1")
plt.axvline(t_l1 - 1126259462, color='g', linestyle=':')
plt.legend(loc='best')
plt.xlim([0.3,0.5])
plt.ylim([0,20])
plt.xlabel("Time from 1126259462 (seconds)")
plt.ylabel("Signal-to-noise ratio")
Out[18]:
In [19]:
phase_h1 = np.angle(h1_complex_snr[h1_imax])
phase_l1 = np.angle(l1_complex_snr[l1_imax])
print "H1 Coalescence phase = {} radians, L1 Coalescence phase = {} radians".format(phase_h1, phase_l1)
For visual comparison, we plot the template used in the search compared to an SEOBNRv2 waveform directly generated with the template parameters. pycbc_inspiral stores templates in the frequency domain, so we convert the template to the time domain for plotting with the command:
template = h1_bank[0].to_timeseries()
The waveforms are computed for a signal at a distance of 1 Mpc. pycbc_inspiral applies an internal scaling of approximately 6e20 to scale these quanties up to order unity (the exact scaling is stored in the constant pycbc.DYN_RANGE_FAC). We divide the amplitude of the template by DYN_RANGE_FAC so that it has the correct amplitude.
The FindChirp algorithm expects the peak time of the template to be at t = 0 in the time domain so that the signal-to-noise ratio time series is time-stamped reference to the peak (coalescence) time of the waveform. Since the FFT is periodic, this means that the signal prior to the merger is at the end of the time-domain template and the merger-ringdown waveform is at the start of the time-domain template. We use the roll function to shift the sample points of the template so that it is contiguous and can be plotted against the result of calling pycbc.waveform.get_td_waveform() to generate the SEOBNRv2 waveform.
Notice that the only difference between the template waveform and the reference SEOBNRv2 waveform is that the search template is windowed at the start to prevent Gibbs ringing when it is transformed into the frequency domain.
In [20]:
h1_bank = h1_result[1]
l1_bank = l1_result[1]
In [21]:
hp, hc = pycbc.waveform.get_td_waveform(
approximant="SEOBNRv2",
mass1=h1_bank.table['mass1'][0],
mass2=h1_bank.table['mass2'][0],
spin1z=h1_bank.table['spin1z'][0],
spin2z=h1_bank.table['spin2z'][0],
f_lower=search_f_low,
delta_t=h1_bank.delta_t)
template = h1_bank[0].to_timeseries() / DYN_RANGE_FAC
template.roll(int(-template.start_time / template.delta_t))
plt.plot(template.sample_times, template,
color='r',label='Search template')
plt.plot(hp.sample_times, hp, linestyle=':', label='SEOBNRv2')
np.savetxt('SearchTemplate_hp.txt', np.c_[template.sample_times.numpy(),
template.numpy()])
plt.xlim([-0.3,0.05])
plt.title('Search template at 1 Mpc')
plt.legend(loc='best')
plt.ylabel('Strain'.format(DYN_RANGE_FAC))
plt.xlabel('Time from waveform peak (seconds)')
Out[21]:
In [22]:
h1_best_fit_waveform = (h1_bank[0] * np.exp(1.0j * phase_h1)).to_timeseries()
h1_best_fit_waveform /= eff_distance_h1
l1_best_fit_waveform = (l1_bank[0] * np.exp(1.0j * phase_l1)).to_timeseries()
l1_best_fit_waveform /= eff_distance_l1
Using the measured arrival index we place the template at the correct location in the time series created in the previous cell.
When this cell is evaluated, the time series h1_remove and l1_remove will contain the correctly time, phase, and amplitude shifted waveform.
In [23]:
h1_strain = h1_result[3]
l1_strain = l1_result[3]
h1_remove = h1_best_fit_waveform * 1
h1_remove.roll(-500)
h1_remove.resize(len(h1_strain))
h1_remove.roll(t_idx_h1 + 500 - len(h1_best_fit_waveform))
h1_remove.start_time = h1_strain.start_time
l1_remove = l1_best_fit_waveform * 1
l1_remove.roll(-500)
l1_remove.resize(len(l1_strain))
l1_remove.roll(t_idx_l1 + 500 - len(l1_best_fit_waveform))
l1_remove.start_time = l1_strain.start_time
We now compare the best-fit template to the raw numerical relavity data shown in Figure 2 of the PRL, and the filtered NR waveform shown Figure 1 of the PRL.
The LOSC NR data is scalled by a factor of 1e21. We undo this scaling when we plot the data for comparison to the best-fit waveform.
In [24]:
!if [ ! -f fig2-unfiltered-waveform-H.txt ] ; then curl -L "https://losc.ligo.org/s/events/GW150914/P150914/fig2-unfiltered-waveform-H.txt" > fig2-unfiltered-waveform-H.txt ; fi
!if [ ! -f fig2-unfiltered-waveform-L.txt ] ; then curl -L "https://losc.ligo.org/s/events/GW150914/P150914/fig2-unfiltered-waveform-L.txt" > fig2-unfiltered-waveform-L.txt ; fi
!if [ ! -f fig1-waveform-H.txt ] ; then curl -L "https://losc.ligo.org/s/events/GW150914/P150914/fig1-waveform-H.txt" > fig1-waveform-H.txt ; fi
!if [ ! -f fig1-waveform-L.txt ] ; then curl -L "https://losc.ligo.org/s/events/GW150914/P150914/fig1-waveform-L.txt" > fig1-waveform-L.txt ; fi
In [25]:
nr_filt_data = np.loadtxt("fig1-waveform-H.txt")
dt = nr_filt_data[1,0] - nr_filt_data[0,0]
h1_nr_filt_hp = pycbc.types.TimeSeries(nr_filt_data[:,1], delta_t=dt, epoch=nr_filt_data[0,0])
nr_data = np.loadtxt("fig2-unfiltered-waveform-H.txt")
dt=nr_data[1,0]-nr_data[0,0]
h1_nr_hp = pycbc.types.TimeSeries(nr_data[:,1], delta_t=dt, epoch=nr_data[0,0])
nr_filt_data = np.loadtxt("fig1-waveform-L.txt")
dt= nr_filt_data[1,0] - nr_filt_data[0,0]
l1_nr_filt_hp = pycbc.types.TimeSeries(nr_filt_data[:,1], delta_t=dt, epoch=nr_filt_data[0,0])
nr_data = np.loadtxt("fig2-unfiltered-waveform-L.txt")
dt = nr_data[1,0] - nr_data[0,0]
l1_nr_hp = pycbc.types.TimeSeries(nr_data[:,1], delta_t=dt, epoch=nr_data[0,0])
In [26]:
h1_bf = h1_remove.time_slice(1126259462-2, 1126259462+2)
l1_bf = l1_remove.time_slice(1126259462-2, 1126259462+2)
h1_bf.save('H1BestFitTemplate.txt')
l1_bf.save('L1BestFitTemplate.txt')
We plot the best-fit waveform from the search and compare it to the data from Figure 1 of the PRL. The L1 raw NR waveform is shifted by 0.007 s and multiplied by -1, as described in the caption of Figure 1.
Notice that in both of these plots there is a phase shift between the raw NR waveform and the filtered NR waveform. This is beacuse the filters used in Figure 1 of the PRL are not phase preserving.
In [27]:
plt.plot(h1_nr_filt_hp.sample_times, h1_nr_filt_hp*1e-21,
color='b', label='Fig 1 NR waveform', linestyle=':')
plt.plot(h1_nr_hp.sample_times, h1_nr_hp*1e-21 ,color='g', label='SXS:BBH:0305')
plt.plot(h1_bf.sample_times-1126259462, h1_bf/DYN_RANGE_FAC, color='r', label='Best fit template')
np.savetxt('BestFitTemplateH1_Fig1.txt', np.c_[h1_bf.sample_times-1126259462,h1_bf/DYN_RANGE_FAC])
plt.xlim([0.25, 0.45])
plt.ylim([-1.4e-21, 1.4e-21])
plt.title('LIGO Hanford Detector')
plt.legend(loc='best')
plt.ylabel('Strain $\\times$ {0:.1e}'.format(DYN_RANGE_FAC))
plt.xlabel('Time from 1126259462 (seconds)')
Out[27]:
In [28]:
plt.plot(l1_nr_filt_hp.sample_times, l1_nr_filt_hp*1e-21,
color='b', label='Fig 1 NR waveform', linestyle=':')
plt.plot(l1_nr_hp.sample_times-0.007, l1_nr_hp*-1e-21, color='g', label='SXS:BBH:0305')
plt.plot(l1_bf.sample_times-1126259462, l1_bf/DYN_RANGE_FAC, color='r', label='Best fit template')
np.savetxt('BestFitTemplateL1_Fig1.txt', np.c_[l1_bf.sample_times-1126259462,l1_bf/DYN_RANGE_FAC])
plt.xlim([0.3,0.45])
plt.ylim([-1.4e-21,1.4e-21])
plt.title('LIGO Livingston Detector')
plt.legend(loc='best')
plt.ylabel('Strain')
plt.xlabel('Time from 1126259462 (seconds)')
Out[28]:
We now re-run pycbc_inspiral but this time we pass the best-fit waveform to the findchip() function so that it is removed from the data prior to the matched filter.
Since we have removed the GW150914 signal, the search code should not find any triggers. In the case where no triggers are found pycbc_inspiral's filtering function does not return any data. To force the code to return the signal-to-noise ratio time series, we set the SNR and newSNR thresholds to unity before running it.
In [29]:
sys.argv = [a for a in argv_h1 if not (a.startswith('--snr-threshold') or a.startswith('--newsnr-threshold'))]
sys.argv += ['--snr-threshold=1', '--newsnr-threshold=1']
!rm -f H1-INSPIRAL_FULL_DATA_JOB0-1126257771-1837.hdf
h1_residual_result = findchirp(h1_remove)
In [30]:
sys.argv = [a for a in argv_l1 if not (a.startswith('--snr-threshold') or a.startswith('--newsnr-threshold'))]
sys.argv += ['--snr-threshold=1', '--newsnr-threshold=1']
!rm -f L1-INSPIRAL_FULL_DATA_JOB0-1126258302-1591.hdf
l1_residual_result = findchirp(l1_remove)
Now we plot the signal-to-noise ratio time series returned by the search for each detector, with vertial lines indicating the trigger times of GW150914.
Notice that there is no trigger corresponding to GW150914 in the output and the values of the SNR at the time of the GW150914 are consistent with noise.
In [31]:
h1_complex_snr = h1_residual_result[0][0] * h1_residual_result[0][1]
h1_complex_snr.start_time -= 1126259462
h1_complex_snr = h1_complex_snr.time_slice(0.3, 0.5)
h1_snr_data = abs(h1_complex_snr)
l1_complex_snr = l1_residual_result[0][0] * l1_residual_result[0][1]
l1_complex_snr.start_time -= 1126259462
l1_complex_snr = l1_complex_snr.time_slice(0.3, 0.5)
l1_snr_data = abs(l1_complex_snr)
plt.plot(h1_snr_data.sample_times, h1_snr_data, color='r', label="H1")
plt.axvline(t_h1 - 1126259462, color='r', linestyle=':')
plt.plot(l1_snr_data.sample_times, l1_snr_data, color='g', label="L1")
plt.axvline(t_l1 - 1126259462, color='g', linestyle=':')
plt.legend(loc='best')
plt.xlim([0.3,0.5])
plt.ylim([0,4])
plt.xlabel("Time from 1126259462 (seconds)")
plt.ylabel("Signal-to-noise ratio")
Out[31]:
The matched filter in pycbc_inspiral stores the overwhitened strain data. Data is overwhitened in the frequency domain by dividing by the time-truncated inverse power spectral density of the data, as described in the the FindChirp algorithm. To plot the whitened strain, we multiply the frequency-domain overwhitened data by the square root of the power spectral density used to overwhiten it, then use PyCBC's to_timeseries() function to transform back to the time domain.
Before plotting the strain data in the time domain, we plot the power spectral density of the data for each detector. The vertical lines show the frequencies that the original GW150914 LOSC tutorial* suggests should be notched out from the data.
In [32]:
plt.loglog(h1_result[2][0].psd.sample_frequencies, h1_result[2][0].psd, color='r')
for l in [14.0, 34.70, 35.30, 35.90, 36.70, 37.30, 40.95, 60.00,
120.00, 179.99, 304.99, 331.49, 510.02, 1009.99]:
plt.axvline(l,color='k',linestyle=':')
plt.xlim([25,2048])
plt.xlabel('Frequency (Hz)')
plt.ylabel('Power spectral density $\\times$ {0:.1e}'.format(DYN_RANGE_FAC*DYN_RANGE_FAC))
plt.title('LIGO Hanford Detector')
np.savetxt('PowerSpectrumH1.txt', np.c_[h1_result[2][0].psd.sample_frequencies,
h1_result[2][0].psd])
In [33]:
plt.loglog(l1_result[2][0].psd.sample_frequencies, l1_result[2][0].psd, color='g')
for l in [14.0, 34.70, 35.30, 35.90, 36.70, 37.30, 40.95, 60.00,
120.00, 179.99, 304.99, 331.49, 510.02, 1009.99]:
plt.axvline(l,color='k',linestyle=':')
plt.xlim([25,2048])
plt.xlabel('Frequency (Hz)')
plt.ylabel('Power spectral density $\\times$ {0:.1e}'.format(DYN_RANGE_FAC*DYN_RANGE_FAC))
plt.title('LIGO Livingston Detector')
np.savetxt('PowerSpectrumL1.txt', np.c_[l1_result[2][0].psd.sample_frequencies,
l1_result[2][0].psd])
In [34]:
whitened_strain_h1 = (h1_result[2][0] * (h1_result[2][0].psd**0.5)).to_timeseries()
whitened_strain_l1 = (l1_result[2][0] * (l1_result[2][0].psd**0.5)).to_timeseries()
whitened_residual_strain_h1 = (h1_residual_result[2][0] * (h1_residual_result[2][0].psd**0.5)).to_timeseries()
whitened_residual_strain_l1 = (l1_residual_result[2][0] * (l1_residual_result[2][0].psd**0.5)).to_timeseries()
We first plot the data used by the search. We offset the L1 data by the measured time of arrival difference, and multiply the Livingston strain by a factor of -1 to account for the relative orientations of the Hanford and Livingston detetectors. The GW150914 signal is clearly visible in the data. More high-frequency noise is visible here than in Figure 1, as only low-pass filter applied is the anti-aliasing filtered used to downsample the input data. This has a higher frequency cutoff than the Butterworth filter used to make Figure 1.
In [35]:
plt.plot(whitened_strain_h1.sample_times-1126259462, whitened_strain_h1, label='H1', color='r')
plt.plot(whitened_strain_l1.sample_times-1126259462+(t_h1-t_l1), -1.0*whitened_strain_l1, label='L1', color='g')
np.savetxt('WhitenedStrainH1.txt', np.c_[whitened_strain_h1.sample_times.numpy()-1126259462,
whitened_strain_h1.numpy()])
np.savetxt('WhitenedStrainL1.txt', np.c_[whitened_strain_l1.sample_times.numpy()-1126259462,
whitened_strain_l1.numpy()])
plt.xlim([0.3,0.45])
plt.ylim([-200,200])
plt.legend(loc='best')
plt.xlabel("Time from 1126259462 (seconds)")
plt.ylabel("Whitened strain")
Out[35]:
In [36]:
plt.plot(whitened_residual_strain_h1.sample_times-1126259462, whitened_residual_strain_h1, label='H1', color='r')
plt.plot(whitened_residual_strain_l1.sample_times-1126259462+(t_h1-t_l1),
-1.0*whitened_residual_strain_l1, label='L1', color='g')
np.savetxt('WhitenedResidualStrainH1.txt', np.c_[whitened_residual_strain_h1.sample_times.numpy()-1126259462,
whitened_residual_strain_h1.numpy()])
np.savetxt('WhitenedResidualStrainL1.txt', np.c_[whitened_residual_strain_l1.sample_times.numpy()-1126259462,
whitened_residual_strain_l1.numpy()])
plt.xlim([0.3,0.45])
plt.ylim([-200,200])
plt.legend(loc='best')
plt.xlabel("Time from 1126259462 (seconds)")
plt.ylabel("Whitened strain")
Out[36]:
We now look numerically for correllations in the above strain data.
To compute the correllation of the residuals, we use the code written by Creswell et al. This code, when run on the data from the Figure 1 of the PRL, reproduces the green curve in the lower right plot in Figure 7 of Creswell et al.
Here we run the code on the strain data used by the filtering code.
In [37]:
def cross_correllation(h1_res_times, h1_res_strain, l1_res_times, l1_res_strain):
fs = 1./(h1_res_times[1]-h1_res_times[0])
# Based on suggestion from Hao, changed this from 0.39 to 0.40
t = 0.40
w = 0.04
min_indxt = np.where(abs(h1_res_times-t) == abs(h1_res_times-t).min())[0][0]
max_indxt = np.where(abs(h1_res_times-(t+w)) == abs(h1_res_times-(t+w)).min())[0][0]
deltatau = 0.01
tauind_min = int(-deltatau*fs); tauind_max = int(+deltatau*fs)
tauind = np.arange(tauind_min,tauind_max)
tau = tauind/fs
corr = []
for i in tauind:
corr.append(np.corrcoef(h1_res_strain[min_indxt+abs(tauind_min)+i:max_indxt-abs(tauind_max)+i],l1_res_strain[min_indxt+abs(tauind_min):max_indxt-abs(tauind_max)])[0][1])
corr = np.array(corr)
imax = np.argmax(abs(corr))
plt.figure()
plt.plot(tau * 1000.,corr,'k',label="t="+str(t)+", w="+str(w))
plt.axvline(1000*tau[imax], color='k')
plt.xlim(-10,10)
plt.xlabel(r"$\tau$ [ms]")
plt.ylabel(r"$C(t,\tau,w)$")
plt.ylim(-1,1)
plt.legend(loc='best')
print('max |corr| = {:.2g} at tau = {:.3g} ms'.format(max(abs(corr)), 1000*tau[imax]))
In [38]:
cross_correllation(whitened_strain_h1.sample_times.numpy()-1126259462, whitened_strain_h1.numpy(),
whitened_strain_l1.sample_times.numpy()-1126259462, whitened_strain_l1.numpy())
In [39]:
cross_correllation(whitened_residual_strain_h1.sample_times.numpy()-1126259462, whitened_residual_strain_h1.numpy(),
whitened_residual_strain_l1.sample_times.numpy()-1126259462, whitened_residual_strain_l1.numpy())
In [40]:
from scipy.signal import butter, freqz, filtfilt
def butter_bandpass(lowcut, highcut, fs, order=4):
nyq = 0.5 * fs
low = lowcut / nyq
high = highcut / nyq
b, a = butter(order, [low, high], btype='band')
return b, a
def filter_data(data, coefs):
for coef in coefs:
b,a = coef
data = filtfilt(b, a, data)
return data
In [41]:
fs = 1.0/whitened_residual_strain_h1.delta_t
filter_coefs = []
bb, ab = butter_bandpass(35.0, 350.0, fs, order=4)
filter_coefs.append((bb, ab))
In [42]:
filterNumber = 0
for b,a in filter_coefs:
w,h = freqz(b,a,worN=100000)
if (filterNumber < 1): # first is bandpass...make thicker
plt.plot((fs * 0.5/np.pi) * w, abs(h),linewidth=3)
else:
plt.plot((fs * 0.5/np.pi) * w, abs(h))
filterNumber += 1
plt.xlabel('Frequency (Hz)')
plt.ylabel('Gain')
plt.loglog()
plt.xlim(8,2000)
plt.ylim(1e-3,2)
plt.grid(True)
plt.legend_ = None
In [43]:
bandpassed_whitened_strain_h1 = filter_data(whitened_strain_h1.numpy(), filter_coefs)
bandpassed_whitened_strain_l1 = filter_data(whitened_strain_l1.numpy(), filter_coefs)
bandpassed_whitened_residual_strain_h1 = filter_data(whitened_residual_strain_h1.numpy(), filter_coefs)
bandpassed_whitened_residual_strain_l1 = filter_data(whitened_residual_strain_l1.numpy(), filter_coefs)
In [44]:
plt.plot(whitened_strain_h1.sample_times-1126259462,bandpassed_whitened_strain_h1,
label='H1',color='r')
plt.plot(whitened_strain_l1.sample_times-1126259462+(t_h1-t_l1),-1.0*bandpassed_whitened_strain_l1,
label='L1',color='g')
plt.xlim([0.3,0.45])
plt.ylim([-200,200])
plt.legend(loc='best')
plt.xlabel("Time from 1126259462 (seconds)")
plt.ylabel("Bandpassed Whitened strain")
Out[44]:
We now compute the correllation for the band-passed whitened strain.
In [45]:
cross_correllation(whitened_strain_h1.sample_times.numpy()-1126259462,bandpassed_whitened_strain_h1,
whitened_strain_l1.sample_times.numpy()-1126259462,bandpassed_whitened_strain_l1)
In [46]:
plt.plot(whitened_strain_h1.sample_times-1126259462,bandpassed_whitened_residual_strain_h1,
label='H1',color='r')
plt.plot(whitened_strain_l1.sample_times-1126259462+(t_h1-t_l1),-1.0*bandpassed_whitened_residual_strain_l1,
label='L1',color='g')
plt.xlim([0.3,0.45])
plt.ylim([-200,200])
plt.legend(loc='best')
plt.xlabel("Time from 1126259462 (seconds)")
plt.ylabel("Bandpassed Whitened strain")
Out[46]:
We now compute the correllation for the band-passed whitened, waveform subtracted strain.
In [47]:
cross_correllation(whitened_strain_h1.sample_times.numpy()-1126259462,bandpassed_whitened_residual_strain_h1,
whitened_strain_l1.sample_times.numpy()-1126259462,bandpassed_whitened_residual_strain_l1)
In [48]:
from scipy.signal import iirdesign, zpk2tf, freqz
def iir_bandstops(fstops, fs, order=4):
"""ellip notch filter
fstops is a list of entries of the form [frequency (Hz), df, df2]
where df is the pass width and df2 is the stop width (narrower
than the pass width). Use caution if passing more than one freq at a time,
because the filter response might behave in ways you don't expect.
"""
nyq = 0.5 * fs
# Zeros zd, poles pd, and gain kd for the digital filter
zd = np.array([])
pd = np.array([])
kd = 1
# Notches
for fstopData in fstops:
fstop = fstopData[0]
df = fstopData[1]
df2 = fstopData[2]
low = (fstop - df) / nyq
high = (fstop + df) / nyq
low2 = (fstop - df2) / nyq
high2 = (fstop + df2) / nyq
z, p, k = iirdesign([low,high], [low2,high2], gpass=1, gstop=6,
ftype='ellip', output='zpk')
zd = np.append(zd,z)
pd = np.append(pd,p)
# Set gain to one at 100 Hz...better not notch there
bPrelim,aPrelim = zpk2tf(zd, pd, 1)
outFreq, outg0 = freqz(bPrelim, aPrelim, 100/nyq)
# Return the numerator and denominator of the digital filter
b,a = zpk2tf(zd,pd,k)
return b, a
##################################################
# Notches from the analog filter minima
notchesAbsolute = np.array(
[1.400069436086257468e+01,
3.469952395163710435e+01, 3.529747106409942603e+01,
3.589993517579549831e+01, 3.670149543090175825e+01,
3.729785276981694153e+01, 4.095285995922058930e+01,
6.000478656292731472e+01, 1.200021163564880027e+02,
1.799868042163590189e+02, 3.049881434406700009e+02,
3.314922032415910849e+02, 5.100176305752708572e+02,
1.009992518164026706e+03])
def get_filt_coefs(fs, lowcut, highcut, no_notches=False):
"""return filter coefficients for timeseries figure
return is a list of (b,a) coefficient tuples, starting with the
bandpass, followed by the notches.
"""
coefs = []
# bandpass
bb, ab = butter_bandpass(lowcut, highcut, fs, order=4)
coefs.append((bb, ab))
if no_notches:
return coefs
for notchf in notchesAbsolute: #use this if not using sectionBas
bn, an = iir_bandstops(np.array([[notchf,1,0.1]]), fs, order=4)
coefs.append((bn,an))
# Manually do a wider filter around 510 Hz etc.
bn, an = iir_bandstops(np.array([[510,200,20]]), fs, order=4)
coefs.append((bn, an))
bn, an = iir_bandstops(np.array([[3.314922032415910849e+02,10,1]]), fs, order=4)
coefs.append((bn, an))
return coefs
In [49]:
filter_coefs_notch = get_filt_coefs(fs, 35.0, 350.0)
In [50]:
filterNumber = 0
for b,a in filter_coefs_notch:
w,h = freqz(b,a,worN=100000)
if (filterNumber < 1): # first is bandpass...make thicker
plt.plot((fs * 0.5/np.pi) * w, abs(h),linewidth=3)
else:
plt.plot((fs * 0.5/np.pi) * w, abs(h))
filterNumber += 1
plt.xlabel('Frequency (Hz)')
plt.ylabel('Gain')
plt.loglog()
plt.xlim(8,2000)
plt.ylim(1e-3,2)
plt.grid(True)
plt.legend_ = None
In [51]:
bandpassed_notched_whitened_strain_h1 = filter_data(whitened_strain_h1.numpy(), filter_coefs_notch)
bandpassed_notched_whitened_strain_l1 = filter_data(whitened_strain_l1.numpy(), filter_coefs_notch)
bandpassed_notched_whitened_residual_strain_h1 = filter_data(whitened_residual_strain_h1.numpy(), filter_coefs_notch)
bandpassed_notched_whitened_residual_strain_l1 = filter_data(whitened_residual_strain_l1.numpy(), filter_coefs_notch)
In [52]:
plt.plot(whitened_strain_h1.sample_times-1126259462,bandpassed_notched_whitened_strain_h1,
label='H1',color='r')
plt.plot(whitened_strain_l1.sample_times-1126259462+(t_h1-t_l1),-1.0*bandpassed_notched_whitened_strain_l1,
label='L1',color='g')
plt.xlim([0.3,0.45])
plt.ylim([-200,200])
plt.legend(loc='best')
plt.xlabel("Time from 1126259462 (seconds)")
plt.ylabel("Bandpassed Whitened strain")
Out[52]:
We now compute the correllation for the band-passed and notched whitened strain.
In [53]:
cross_correllation(whitened_strain_h1.sample_times.numpy()-1126259462,bandpassed_notched_whitened_strain_h1,
whitened_strain_l1.sample_times.numpy()-1126259462,bandpassed_notched_whitened_strain_l1)
In [54]:
plt.plot(whitened_strain_h1.sample_times-1126259462,bandpassed_notched_whitened_residual_strain_h1,
label='H1',color='r')
plt.plot(whitened_strain_l1.sample_times-1126259462+(t_h1-t_l1),-1.0*bandpassed_notched_whitened_residual_strain_l1,
label='L1',color='g')
plt.xlim([0.3,0.45])
plt.ylim([-200,200])
plt.legend(loc='best')
plt.xlabel("Time from 1126259462 (seconds)")
plt.ylabel("Bandpassed Whitened strain")
Out[54]:
We now compute the correllation for the band-passed whitened and notched waveform subtracted strain.
In [55]:
cross_correllation(whitened_strain_h1.sample_times.numpy()-1126259462,bandpassed_notched_whitened_residual_strain_h1,
whitened_strain_l1.sample_times.numpy()-1126259462,bandpassed_notched_whitened_residual_strain_l1)
In [56]:
residual_strain_h1 = (h1_residual_result[2][0] * (h1_residual_result[2][0].psd)).to_timeseries()
residual_strain_l1 = (l1_residual_result[2][0] * (l1_residual_result[2][0].psd)).to_timeseries()
np.savetxt('ResidualStrainH1.txt', np.c_[residual_strain_h1.sample_times.numpy()-1126259462,
residual_strain_h1.numpy()/DYN_RANGE_FAC])
np.savetxt('ResidualStrainL1.txt', np.c_[residual_strain_l1.sample_times.numpy()-1126259462,
residual_strain_l1.numpy()/DYN_RANGE_FAC])
DAB thanks Jeandrew Brink, Jolien Creighton, Will Farr, Ben Farr, Jon Gair, Ian Harry, Daniel Holz, Andrew Jackson, Joey Key, Hao Liu, Andrew Lundgren, Jessica McIver, Pavel Naselsky, Alex Neilsen, and Alexander Nitz for helpful discussions. This work is supported by National Science Foundation award PHY-1707954. DAB thanks the Niels Bohr Institute for its hospitality while part of this work was completed, the Kavli Foundation and the DNRF for supporting the 2017 Kavli Summer Program.
In [57]:
sys.argv = ['pycbc_inspiral', '--version']
try:
findchirp()
except SystemExit:
pass