GW170823

 An ini file for running H1, L1, V1, and H1L1V1 searches for GW170823 from its graceDB id
gracedb = G298936
label = GW170823
detectors = [H1, L1, V1]
coherence-test = True
duration = 16
psd-duration = 1024
outdir = results_GW170823
create-summary = True
sampler = dynesty
sampler-kwargs = {'nlive': 2048}
channel-names = [H1:DCH-CLEAN_STRAIN_C02, L1:DCH-CLEAN_STRAIN_C02, V1:Hrec_hoft_V1O2Repro2A_16384Hz]
query-types = [H1_CLEANED_HOFT_C02, L1_CLEANED_HOFT_C02, V1O2Repro2A]
prior-file = GW170823.prior
reference-frequency = 20
create-summary = True
create-output = True
accounting = ligo.dev.o3.cbc.pe.lalinference

# These are the priors for analysing GW170823.
chirp_mass = Uniform(name='chirp_mass', minimum=10, maximum=50, unit='$M_{\\odot}$')
mass_ratio = Uniform(name='mass_ratio', minimum=0.125, maximum=1)
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)
phi_jl =  Uniform(name='phi_jl', minimum=0, maximum=2 * np.pi)
# Here we use a luminosity distance consistent with LAL analyses for comparison.
luminosity_distance = bilby.core.prior.PowerLaw(alpha=2, name='luminosity_distance', minimum=100, maximum=3000, unit='Mpc', latex_label='$d_L$')
dec =  Cosine(name='dec')
ra =  Uniform(name='ra', minimum=0, maximum=2 * np.pi)
iota =  Sine(name='iota')
psi =  Uniform(name='psi', minimum=0, maximum=np.pi)
phase =  Uniform(name='phase', minimum=0, maximum=2 * np.pi)