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! pip install nrsur_catalog
Looking in indexes: https://pypi.org/simple, https://packagecloud.io/eugeny/tabby/pypi/simple
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GW190413_134308#
Below are some plots for GW190413_134308 from the NRSurrogate Catalog.
from nrsur_catalog import NRsurResult
nrsur_result = NRsurResult.load("GW190413_134308", cache_dir=".nrsur_catalog_cache")
# you can specify a `cache_dir`: folder where data will be downloaded
Summary#
nrsur_result.summary()
Parameter |
Posterior 90% CI |
Prior |
|---|---|---|
\(\chi_1\) |
\({0.59}_{-0.38}^{+0.29}\) |
\(\text{Uniform} [0, 0.99]\) |
\(\chi_2\) |
\({0.50}_{-0.34}^{+0.33}\) |
\(\text{Uniform} [0, 0.99]\) |
\(\phi\) |
\({2.25}_{-0.14}^{+0.29}\) |
\(\text{Uniform} [0, 6.28]\) |
\(\mathcal{M}_{c}^{\rm det}\ [M_{\odot}]\) |
\({58.79}_{-6.01}^{+5.47}\) |
\(\text{UniformInComponentsChirpMass} [12, 400]\) |
\(t_c\ [s]\) |
\({1239198206.71}_{-0.00}^{+0.00}\) |
\(\text{Uniform} [1239198206.64, 1239198206.84]\) |
\(d_L\ [Mpc]\) |
\({4635.32}_{-1461.27}^{+1481.59}\) |
\(\text{UniformSourceFrame} [100.0, 10000.0]\) |
\(q\) |
\({0.70}_{-0.21}^{+0.20}\) |
\(\text{UniformInComponentsMassRatio} [0.17, 1]\) |
\(\phi\) |
\({3.87}_{-2.80}^{+1.63}\) |
\(\text{Uniform} [0, 6.28]\) |
\(\phi_{12}\) |
\({3.04}_{-2.02}^{+2.16}\) |
\(\text{Uniform} [0, 6.28]\) |
\(\phi_{\mathrm{JL}}\) |
\({3.15}_{-2.14}^{+2.03}\) |
\(\text{Uniform} [0, 6.28]\) |
\(\psi\) |
\({1.42}_{-0.98}^{+1.26}\) |
\(\text{Uniform} [0, 3.14]\) |
\(\theta_{\mathrm{JN}}\) |
\({1.58}_{-1.05}^{+1.04}\) |
\(\text{Sine} [0, 3.14]\) |
\(\theta_1\) |
\({1.52}_{-0.55}^{+0.54}\) |
\(\text{Sine} [0, 3.14]\) |
\(\theta_2\) |
\({1.64}_{-0.72}^{+0.69}\) |
\(\text{Sine} [0, 3.14]\) |
\({M}^{\rm det}\ [M_{\odot}]\) |
\({139.22}_{-11.24}^{+11.60}\) |
\(\text{Constraint} [60, 400]\) |
\(\theta\) |
\({1.18}_{-0.05}^{+0.05}\) |
\(\text{Sine} [0, 3.14]\) |
\(m_1^{\rm src}\ [M_{\odot}]\) |
\({47.99}_{-6.86}^{+8.32}\) |
\(-\) |
\(m_2^{\rm src}\ [M_{\odot}]\) |
\({32.54}_{-7.08}^{+6.81}\) |
\(-\) |
\(\chi_{\mathrm{eff}}\) |
\({0.00}_{-0.17}^{+0.15}\) |
\(-\) |
\(\chi_{\mathrm{p}}\) |
\({0.57}_{-0.28}^{+0.25}\) |
\(-\) |
\(\alpha\) |
\({2.69}_{-0.14}^{+0.10}\) |
\(-\) |
\(\delta\) |
\({-0.52}_{-0.07}^{+0.30}\) |
\(-\) |
\(M_f^{\rm src}\ [M_{\odot}]\) |
\({132.84}_{-10.31}^{+10.59}\) |
\(-\) |
\(\chi_f\) |
\({0.69}_{-0.07}^{+0.06}\) |
\(-\) |
\(v_f\ [{\rm km/s}]\) |
\({767.68}_{-512.88}^{+778.61}\) |
\(-\) |
Note: For most events the kick inference is dominated by the prior itself, see Figs. 10 and 11 of Islam et al, 2023.
Lets make some plots!
Show code cell source
# NRSurrogate corner plots
import os
param_sets = dict(
mass=["mass_1_source", "mass_2_source", "mass_ratio"],
spin=["a_1", "a_2", "tilt_1", "tilt_2"],
effective_spin=["mass_ratio", "chi_eff", "chi_p"],
sky_localisation=["luminosity_distance", "ra", "dec"],
remnant=["final_mass", "final_spin", "final_kick"],
)
for name, params in param_sets.items():
fname = f"GW190413_134308_{name}_corner.png"
if not os.path.isfile(fname):
fig = nrsur_result.plot_corner(params)
fig.savefig(fname)
if name == "remnant":
continue
# LVK-Comparison plots
fname = f"GW190413_134308_compare_{name}_corner.png"
if not os.path.isfile(fname):
fig = nrsur_result.plot_lvk_comparison_corner(params)
fig.savefig(fname)
Corner Plots#
Corner plots of the NRSurCat-1 posteriors. The plots along the diagonal display the 1D marginalized posteriors, with the median values and the central \(1\sigma\) credible regions indicated as text. The contour plots display the joint 2D posteriors at the \(1,2,3\sigma\) regions. The LVK posteriors are plotted using the IMRPhenomXPHM samples obtained from the the GWTC-2.1 and GWTC-3 zenodo releases.
Mass#
Posterior corner plots for the component masses, and mass-ratio (\(m_1^{\rm src}, m_2^{\rm src}, q\)). Component masses are shown in the source frame.
Spin#
Posterior corner plots for the component spin magnitudes (\(\chi_1, \chi_2\)) and tilt angles (\(\theta_1, \theta_2\)).
Effective Spin#
Posterior corner plots for the mass-ratio \(q\), effective spin \(\chi_{\rm eff}\) and the transverse spin precession parameters \(\chi_p\).
Sky-localisation#
Posterior corner plots for the luminosity distance, ra and dec (\(d_L, \alpha, \delta\)).
Remnant#
Posterior corner plots for the remnant mass, remnant spin magnitude and kick (\(M_f^{\rm src}, \chi_f, v_f\)).
Animations#
Here are some animations of the posterior.
Spin |
|---|
Posterior samples for the dimensionless spin vectors (\(\chi_1, \chi_2\)) of the component black holes. Each purple marker indicates a posterior sample; an arrow drawn from the origin to the marker would show the spin vector. The outer radii of the spheres correspond to the maximum spin magnitude of 1. The spins are shown in the “wave frame” defined at a reference frequency of 20 Hz. The x-axis (orange) and y-axis (green) are shown as arrows near the origin; the x-y plane is orthogonal to the orbital angular momentum direction. The color reflects posterior probability density.
Remnant |
|---|
Posterior samples for the dimensionless spin vector \(\chi_f\) and the recoil kick velocity \(v_f\), (units of km/s). Each purple marker indicates a posterior sample; an arrow drawn from the origin to the marker would show the spin or kick vector. For the spin, the outer radii of the spheres correspond to the maximum spin magnitude of 1. For the kick, the outer radius of the sphere corresponds to a kick magnitude of 2500 km/s. The remnant spin and kick are shown in the “wave frame” defined at a reference time of -100 \(M^{\rm det}\ [M_{\odot}]\) before the peak waveform amplitude, where \(M^{\rm det}\) is the detector frame total mass.
Analysis configs#
Below are the configs used for the analysis of this job.
nrsur_result.print_configs()
Tmax: 10000
accounting: None
accounting_user: None
adapt: False
allow_tape: True
analysis_executable: None
analysis_executable_parser: None
autocorr_c: 5.0
autocorr_tol: 50.0
bilby_zero_likelihood_mode: False
burn_in_nact: 50.0
calibration_model: CubicSpline
calibration_prior_boundary: reflective
catch_waveform_errors: True
channel_dict: {H1:DCS-CALIB_STRAIN_CLEAN_SUB60HZ_C01, L1:DCS-CALIB_STRAIN_CLEAN_SUB60HZ_C01_T1700406_v4, V1:Hrec_hoft_16384Hz}
check_point_deltaT: 3600
clean: False
coherence_test: False
conda_env: None
condor_job_priority: 0
conversion_function: None
create_summary: True
data_dict: {H1:/anvil/projects/x-phy990007n/vvarma/Work/Projects/Current/NRSurCatalog/runs/GWTC/Data/GW190413_134308/H1_data.gwf, L1:/anvil/projects/x-phy990007n/vvarma/Work/Projects/Current/NRSurCatalog/runs/GWTC/Data/GW190413_134308/L1_data.gwf, V1:/anvil/projects/x-phy990007n/vvarma/Work/Projects/Current/NRSurCatalog/runs/GWTC/Data/GW190413_134308/V1_data.gwf}
data_dump_file: None
data_format: None
default_prior: BBHPriorDict
deltaT: 0.2
desired_sites: None
detectors: ['H1', 'L1', 'V1']
distance_marginalization: True
distance_marginalization_lookup_table: None
dlogz: 0.1
do_not_save_bounds_in_resume: False
duration: 4.0
dynesty_bound: multi
dynesty_sample: rwalk
email: None
enforce_signal_duration: False
enlarge: 1.5
existing_dir: None
extra_likelihood_kwargs: None
extra_lines: job-name=GW190413_134308 mail-user=sfield@umassd.edu mail-type=END
facc: 0.5
fast_mpi: False
final_result: True
final_result_nsamples: 20000
frac_threshold: 0.01
frequency_domain_source_model: lal_binary_black_hole
gaussian_noise: False
generation_function: None
generation_seed: None
gps_file: None
gps_tuple: None
idx: 0
ignore_gwpy_data_quality_check: True
ini: GW190413_134308_config.ini
injection: False
injection_dict: None
injection_file: None
injection_numbers: None
injection_waveform_approximant: None
injection_waveform_arguments: None
jitter_time: True
label: GW190413_134308_NRSur7dq4
likelihood_type: GravitationalWaveTransient
local: False
local_generation: False
local_plot: False
log_directory: None
max_iterations: 100000
max_its: 10000000000
max_run_time: 10000000000.0
maximum_frequency: 448.000000
maxmcmc: 5000
mem_per_cpu: None
min_eff: 10
min_tau: 30
minimum_frequency: {H1:20.000000, L1:20.000000, V1:20.000000, waveform: 0}
mode_array: None
mpi_timing: False
mpi_timing_interval: 0
n_check_point: 100
n_effective: inf
n_parallel: 4
n_simulation: 0
nact: 50
ncheck: 500
nestcheck: False
nfrac: 5
nlive: 2000
no_plot: False
nodes: 1
notification: Never
nsamples: 10000
ntasks_per_node: 128
ntemps: 20
numerical_relativity_file: None
nwalkers: 100
online_pe: False
osg: False
outdir: NRSur7dq4_run
overwrite_outdir: False
periodic_restart_time: 28800
phase_marginalization: False
plot_calibration: False
plot_corner: False
plot_data: True
plot_format: png
plot_injection: True
plot_marginal: False
plot_skymap: False
plot_spectrogram: True
plot_trace: True
plot_waveform: False
pn_amplitude_order: 0
pn_phase_order: -1
pn_spin_order: -1
pn_tidal_order: -1
post_trigger_duration: 2.0
postprocessing_arguments: None
postprocessing_executable: None
prior_dict: {mass-ratio: bilby.gw.prior.UniformInComponentsMassRatio(name='mass_ratio', minimum= 0.167 , maximum=1), chirp_mass = bilby.gw.prior.UniformInComponentsChirpMass(name='chirp_mass', minimum=12, maximum=400), total_mass = Constraint(name='total_mass', minimum=60, maximum=400), a_1 = Uniform(name='a_1', minimum=0, maximum=0.99), a_2 = Uniform(name='a_2', minimum=0, maximum=0.99), tilt_1 = Sine(name='tilt_1'), tilt_2 = Sine(name='tilt_2'), phi_12 = Uniform(name='phi_12', minimum=0, maximum=2 * np.pi, boundary='periodic'), phi_jl = Uniform(name='phi_jl', minimum=0, maximum=2 * np.pi, boundary='periodic'), dec = Cosine(name='dec'), ra = Uniform(name='ra', minimum=0, maximum=2 * np.pi, boundary='periodic'), theta_jn = Sine(name='theta_jn'), luminosity_distance = bilby.gw.prior.UniformSourceFrame(name='luminosity_distance', minimum=100.0, maximum=10000.0), psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic'), phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')}
prior_file: None
psd_dict: {H1:/anvil/projects/x-phy990007n/vvarma/Work/Projects/Current/NRSurCatalog/runs/GWTC/Data/GW190413_134308/H1_PSD.dat, L1:/anvil/projects/x-phy990007n/vvarma/Work/Projects/Current/NRSurCatalog/runs/GWTC/Data/GW190413_134308/L1_PSD.dat, V1:/anvil/projects/x-phy990007n/vvarma/Work/Projects/Current/NRSurCatalog/runs/GWTC/Data/GW190413_134308/V1_PSD.dat}
psd_fractional_overlap: 0.5
psd_length: 32
psd_maximum_duration: 1024
psd_method: median
psd_start_time: None
reference_frame: H1L1
reference_frequency: 20.0
request_cpus: 1
request_disk: 1.0
request_memory: 4.0
request_memory_generation: None
resampling_method: lal
result_format: hdf5
roq_folder: None
roq_scale_factor: 1
roq_weights: None
rotate_checkpoints: False
safety: 1.0
sampler: dynesty
sampler_kwargs: Default
sampling_frequency: 1024.0
sampling_seed: None
scheduler: condor
scheduler_analysis_time: 7-00:00:00
scheduler_args: None
scheduler_env: None
scheduler_module: None
single_postprocessing_arguments: None
single_postprocessing_executable: None
slurm_extra_lines: partition=wholenode account=phy990002
spline_calibration_amplitude_uncertainty_dict: None
spline_calibration_envelope_dict: {H1:/anvil/projects/x-phy990007n/vvarma/Work/Projects/Current/NRSurCatalog/runs/GWTC/Data/GW190413_134308/H1_CalEnv.dat, L1:/anvil/projects/x-phy990007n/vvarma/Work/Projects/Current/NRSurCatalog/runs/GWTC/Data/GW190413_134308/L1_CalEnv.dat, V1:/anvil/projects/x-phy990007n/vvarma/Work/Projects/Current/NRSurCatalog/runs/GWTC/Data/GW190413_134308/V1_CalEnv.dat}
spline_calibration_nodes: 10
spline_calibration_phase_uncertainty_dict: None
submit: True
summarypages_arguments: {'nsamples_for_skymap': 5000, 'multi_process':8}
thin_by_nact: 1.0
time: 42:00:00
time_marginalization: False
time_reference: geocent
timeslide_dict: None
timeslide_file: None
transfer_files: True
trigger_time: 1239198206.741211
tukey_roll_off: 0.4
verbose: False
vol_check: 8
vol_dec: 0.5
walks: 100
waveform_approximant: NRSur7dq4
waveform_arguments_dict: None
waveform_generator: bilby.gw.waveform_generator.WaveformGenerator
webdir: summary
weight_file: None
zero_noise: False
Comments#
This has been made with
nrsur_catalogversion 0.0.5. If you used this data, please cite this work.Leave a comment in this issue.