bilby/gw/prior_files/aligned_spins_waveform_tides_off.prior

-chirp_mass = Uniform(name='chirp_mass', minimum=3.56, maximum=3.68)
-mass_ratio = Uniform(name='mass_ratio', minimum=0.05, maximum=1)
-mass_1 = Constraint(name='mass_1', minimum=1.00, maximum=22.0)
-mass_2 = Constraint(name='mass_2', minimum=1.00, maximum=2.95)
-chi_1 = bilby.gw.prior.AlignedSpin(name='chi_1', a_prior=Uniform(minimum=0, maximum=0.5))
-chi_2 = bilby.gw.prior.AlignedSpin(name='chi_2', a_prior=Uniform(minimum=0, maximum=0.05))
-luminosity_distance = bilby.core.prior.PowerLaw(alpha=2, name='luminosity_distance', minimum=1, maximum=750, unit='Mpc')
-ra = Uniform(minimum=0, maximum=2 * np.pi, name='ra',  boundary='periodic')
-dec = Cosine(name='dec')
-theta_jn = Sine(name='theta_jn')
-psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
-phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')

test/prior_files/precessing_spins_binary_black_holes.prior → bilby/gw/prior_files/precessing_spins_bbh.prior

@@ -6,15 +6,15 @@ mass_1 = Constraint(name='mass_1', minimum=5, maximum=100)
 mass_2 = Constraint(name='mass_2', minimum=5, maximum=100)
 mass_ratio = Uniform(name='mass_ratio', minimum=0.125, maximum=1)
 chirp_mass = Uniform(name='chirp_mass', minimum=25, maximum=100)
-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')
 luminosity_distance = bilby.gw.prior.UniformSourceFrame(name='luminosity_distance', minimum=1e2, maximum=5e3)
 dec = Cosine(name='dec')
 ra = Uniform(name='ra', minimum=0, maximum=2 * np.pi, boundary='periodic')
 theta_jn = Sine(name='theta_jn')
 psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
 phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')
+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')

bilby/gw/prior_files/precessing_spins_waveform_tides_on.prior → bilby/gw/prior_files/precessing_spins_bbh_tides_on.prior

-chirp_mass = Uniform(name='chirp_mass', minimum=3.56, maximum=3.68)
-mass_ratio = Uniform(name='mass_ratio', minimum=0.05, maximum=1)
-mass_1 = Constraint(name='mass_1', minimum=1.00, maximum=22.0)
-mass_2 = Constraint(name='mass_2', minimum=1.00, maximum=22.0)
-a_1 = Uniform(name='a_1', minimum=0, maximum=0.89)
-a_2 = Uniform(name='a_2', minimum=0, maximum=0.05)
-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')
-luminosity_distance = bilby.gw.prior.UniformComovingVolume(name='luminosity_distance', minimum=1, maximum=750, unit='Mpc')
-ra = Uniform(minimum=0, maximum=2 * np.pi, name='ra',  boundary='periodic')
+# These are the default priors we use for BBH systems.
+# Note that you may wish to use more specific mass and distance parameters.
+# These commands are all known to bilby.gw.prior.
+# Lines beginning "#" are ignored.
+mass_1 = Constraint(name='mass_1', minimum=5, maximum=100)
+mass_2 = Constraint(name='mass_2', minimum=5, maximum=100)
+mass_ratio = Uniform(name='mass_ratio', minimum=0.125, maximum=1)
+chirp_mass = Uniform(name='chirp_mass', minimum=25, maximum=100)
+luminosity_distance = bilby.gw.prior.UniformSourceFrame(name='luminosity_distance', minimum=1e2, maximum=5e3)
 dec = Cosine(name='dec')
+ra = Uniform(name='ra', minimum=0, maximum=2 * np.pi, boundary='periodic')
 theta_jn = Sine(name='theta_jn')
 psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
 phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')
-lambda_1 = Uniform(name='lambda_2', minimum=0, maximum=5000)
+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')
+lambda_1 = Uniform(name='lambda_1', minimum=0, maximum=5000)
 lambda_2 = Uniform(name='lambda_2', minimum=0, maximum=5000)

bilby/gw/prior_files/precessing_spins_bns.prior

+# These are the default priors we use for BNS systems.
+# Note that you may wish to use more specific mass and distance parameters.
+# These commands are all known to bilby.gw.prior.
+# Lines beginning "#" are ignored.
+mass_1 = Constraint(name='mass_1', minimum=0.5, maximum=5)
+mass_2 = Constraint(name='mass_2', minimum=0.5, maximum=5)
+mass_ratio = Uniform(name='mass_ratio', minimum=0.125, maximum=1)
+chirp_mass = Uniform(name='chirp_mass', minimum=0.4, maximum=4.4)
+luminosity_distance = bilby.gw.prior.UniformSourceFrame(name='luminosity_distance', minimum=1e2, maximum=5e3)
+dec = Cosine(name='dec')
+ra = Uniform(name='ra', minimum=0, maximum=2 * np.pi, boundary='periodic')
+theta_jn = Sine(name='theta_jn')
+psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
+phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')
+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')

bilby/gw/prior_files/precessing_spins_bns_tides_on.prior

+# These are the default priors we use for BNS systems.
+# Note that you may wish to use more specific mass and distance parameters.
+# These commands are all known to bilby.gw.prior.
+# Lines beginning "#" are ignored.
+mass_1 = Constraint(name='mass_1', minimum=0.5, maximum=5)
+mass_2 = Constraint(name='mass_2', minimum=0.5, maximum=5)
+mass_ratio = Uniform(name='mass_ratio', minimum=0.125, maximum=1)
+chirp_mass = Uniform(name='chirp_mass', minimum=0.4, maximum=4.4)
+luminosity_distance = bilby.gw.prior.UniformSourceFrame(name='luminosity_distance', minimum=1e2, maximum=5e3)
+dec = Cosine(name='dec')
+ra = Uniform(name='ra', minimum=0, maximum=2 * np.pi, boundary='periodic')
+theta_jn = Sine(name='theta_jn')
+psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
+phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')
+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')
+lambda_1 = Uniform(name='lambda_1', minimum=0, maximum=5000)
+lambda_2 = Uniform(name='lambda_2', minimum=0, maximum=5000)

bilby/gw/prior_files/precessing_spins_waveform_tides_off.prior

-chirp_mass = Uniform(name='chirp_mass', minimum=3.56, maximum=3.68)
-mass_ratio = Uniform(name='mass_ratio', minimum=0.05, maximum=1)
-mass_1 = Constraint(name='mass_1', minimum=1.00, maximum=22.0)
-mass_2 = Constraint(name='mass_2', minimum=1.00, maximum=22.0)
-a_1 = Uniform(name='a_1', minimum=0, maximum=0.89)
-a_2 = Uniform(name='a_2', minimum=0, maximum=0.05)
-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')
-luminosity_distance = bilby.gw.prior.UniformComovingVolume(name='luminosity_distance', minimum=1, maximum=750, unit='Mpc')
-ra = Uniform(minimum=0, maximum=2 * np.pi, name='ra',  boundary='periodic')
-dec = Cosine(name='dec')
-theta_jn = Sine(name='theta_jn')
-psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
-phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')

bilby/gw/waveform_generator.py

@@ -3,6 +3,7 @@ import numpy as np
 from ..core import utils
 from ..core.series import CoupledTimeAndFrequencySeries
 from .utils import PropertyAccessor
+from .conversion import convert_to_lal_binary_black_hole_parameters
 
 
 class WaveformGenerator(object):
@@ -57,7 +58,7 @@ class WaveformGenerator(object):
         self.time_domain_source_model = time_domain_source_model
         self.source_parameter_keys = self.__parameters_from_source_model()
         if parameter_conversion is None:
-            self.parameter_conversion = _default_parameter_conversion
+            self.parameter_conversion = convert_to_lal_binary_black_hole_parameters
         else:
             self.parameter_conversion = parameter_conversion
         if waveform_arguments is not None:
@@ -67,6 +68,15 @@ class WaveformGenerator(object):
         if isinstance(parameters, dict):
             self.parameters = parameters
         self._cache = dict(parameters=None, waveform=None, model=None)
+        utils.logger.info(
+            "Waveform generator initiated with\n"
+            "  frequency_domain_source_model: {}\n"
+            "  time_domain_source_model: {}\n"
+            "  parameter_conversion: {}"
+            .format(utils.get_function_path(self.frequency_domain_source_model),
+                    utils.get_function_path(self.time_domain_source_model),
+                    utils.get_function_path(self.parameter_conversion))
+        )
 
     def __repr__(self):
         if self.frequency_domain_source_model is not None:
@@ -77,7 +87,7 @@ class WaveformGenerator(object):
             tdsm_name = self.time_domain_source_model.__name__
         else:
             tdsm_name = None
-        if self.parameter_conversion.__name__ == '_default_parameter_conversion':
+        if self.parameter_conversion is None:
             param_conv_name = None
         else:
             param_conv_name = self.parameter_conversion.__name__
@@ -237,7 +247,3 @@ class WaveformGenerator(object):
             raise AttributeError('Either time or frequency domain source '
                                  'model must be provided.')
         return set(utils.infer_parameters_from_function(model))
-
-
-def _default_parameter_conversion(parmeters):
-    return parmeters, list()

cli_bilby/bilby_result.py

@@ -41,6 +41,10 @@ def setup_command_line_args():
                         help="Convert all results.", default=False)
     parser.add_argument("-m", "--merge", action='store_true',
                         help="Merge the set of runs, output saved using the outdir and label")
+    parser.add_argument("-e", "--extension", type=str, choices=["json", "hdf5"],
+                        default=True, help="Use given extension for the merged output file.")
+    parser.add_argument("-g", "--gzip", action="store_true",
+                        help="Gzip the merged output results file if using JSON format.")
     parser.add_argument("-o", "--outdir", type=str, default=None,
                         help="Output directory.")
     parser.add_argument("-l", "--label", type=str, default=None,
@@ -131,4 +135,6 @@ def main():
             result.label = args.label
         if args.outdir is not None:
             result.outdir = args.outdir
-        result.save_to_file()
+
+        extension = args.extension
+        result.save_to_file(gzip=args.gzip, extension=extension)

docs/gw_eos.txt

+.. gw_eos:
+
+====================================================
+Neutron Star Equation of State Modeling and Sampling
+====================================================
+
+Base class for EOS objects. Initialized with energy-density pressure data from either an 2D array or file. Includes plotting routines for common representations of EOS:
+
+.. autoclass:: bilby.gw.eos.TabularEOS
+   :members:
+
+Spectral decomposition parameterized EOS from Lindblom, 2010 (ArXiv: 1009.0738):
+
+.. autoclass:: bilby.gw.eos.SpectralDecompositionEOS
+   :members:
+
+A Neutron star EOS 'Family'. Constructing this object maps the passed EOS object to its corresponding mass-radius relationship by solving the TOV equations. Also includes plotting routines for mass-radius and several equivalent representations of NS Family:
+
+.. autoclass:: bilby.gw.eos.EOSFamily
+   :members:

examples/gw_examples/injection_examples/binary_neutron_star_example.py

@@ -70,8 +70,7 @@ priors = bilby.gw.prior.BNSPriorDict()
 for key in ['psi', 'geocent_time', 'ra', 'dec', 'chi_1', 'chi_2',
             'theta_jn', 'luminosity_distance', 'phase']:
     priors[key] = injection_parameters[key]
-priors.pop('mass_1')
-priors.pop('mass_2')
+priors.pop('mass_ratio')
 priors.pop('lambda_1')
 priors.pop('lambda_2')
 priors['chirp_mass'] = bilby.core.prior.Gaussian(

examples/gw_examples/injection_examples/fast_tutorial.py

@@ -42,6 +42,7 @@ waveform_arguments = dict(waveform_approximant='IMRPhenomPv2',
 waveform_generator = bilby.gw.WaveformGenerator(
     duration=duration, sampling_frequency=sampling_frequency,
     frequency_domain_source_model=bilby.gw.source.lal_binary_black_hole,
+    parameter_conversion=bilby.gw.conversion.convert_to_lal_binary_black_hole_parameters,
     waveform_arguments=waveform_arguments)
 
 # Set up interferometers.  In this case we'll use two interferometers

sampler_requirements.txt

@@ -7,4 +7,4 @@ pymc3==3.6; python_version <= '2.7'
 pymc3>=3.6; python_version > '3.4'
 pymultinest
 kombine
-ultranest
+ultranest>=2.2.1

setup.py

@@ -39,7 +39,7 @@ def write_version_file(version):
     except Exception as e:
         print("Unable to obtain git version information, exception: {}"
               .format(e))
-        git_status = ''
+        git_status = 'release'
 
     version_file = '.version'
     if os.path.isfile(version_file) is False:
@@ -64,7 +64,7 @@ def readfile(filename):
     return filecontents
 
 
-VERSION = '0.6.9'
+VERSION = '1.0.0'
 version_file = write_version_file(VERSION)
 long_description = get_long_description()
 

test/gw_plot_test.py

@@ -117,7 +117,6 @@ class TestCBCResult(unittest.TestCase):
 
         expected_keys = {
             "HISTORY",
-            "build_date",
             "creator",
             "distmean",
             "diststd",
@@ -126,7 +125,6 @@ class TestCBCResult(unittest.TestCase):
             "nest",
             "objid",
             "origin",
-            "vcs_revision",
             "vcs_version",
             "instruments",
         }

test/gw_prior_test.py

@@ -26,7 +26,7 @@ class TestBBHPriorDict(unittest.TestCase):
         )
         self.filename = os.path.join(
             os.path.dirname(os.path.realpath(__file__)),
-            "prior_files/precessing_spins_binary_black_holes.prior",
+            "prior_files/precessing_spins_bbh.prior",
         )
         self.bbh_prior_dict = bilby.gw.prior.BBHPriorDict(filename=self.filename)
         for key, value in self.bbh_prior_dict.items():
@@ -267,13 +267,13 @@ class TestPackagedPriors(unittest.TestCase):
     """ Test that the prepackaged priors load """
 
     def test_aligned(self):
-        filename = "aligned_spins_binary_black_holes.prior"
+        filename = "aligned_spins_bbh.prior"
         prior_dict = bilby.gw.prior.BBHPriorDict(filename=filename)
         self.assertTrue("chi_1" in prior_dict)
         self.assertTrue("chi_2" in prior_dict)
 
     def test_binary_black_holes(self):
-        filename = "precessing_spins_binary_black_holes.prior"
+        filename = "precessing_spins_bbh.prior"
         prior_dict = bilby.gw.prior.BBHPriorDict(filename=filename)
         self.assertTrue("a_1" in prior_dict)
 
@@ -298,7 +298,7 @@ class TestBNSPriorDict(unittest.TestCase):
         )
         self.filename = os.path.join(
             os.path.dirname(os.path.realpath(__file__)),
-            "prior_files/aligned_spins_waveform_tides_on.prior",
+            "prior_files/aligned_spins_bns_tides_on.prior",
         )
         self.bns_prior_dict = bilby.gw.prior.BNSPriorDict(filename=self.filename)
         for key, value in self.bns_prior_dict.items():

test/prior_files/aligned_spins_bbh.prior

+# These are the default priors we use for BBH systems.
+# Note that you may wish to use more specific mass and distance parameters.
+# These commands are all known to bilby.gw.prior.
+# Lines beginning "#" are ignored.
+mass_1 = Constraint(name='mass_1', minimum=5, maximum=100)
+mass_2 = Constraint(name='mass_2', minimum=5, maximum=100)
+mass_ratio = Uniform(name='mass_ratio', minimum=0.125, maximum=1)
+chirp_mass = Uniform(name='chirp_mass', minimum=25, maximum=100)
+luminosity_distance = bilby.gw.prior.UniformSourceFrame(name='luminosity_distance', minimum=1e2, maximum=5e3)
+dec = Cosine(name='dec')
+ra = Uniform(name='ra', minimum=0, maximum=2 * np.pi, boundary='periodic')
+theta_jn = Sine(name='theta_jn')
+psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
+phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')
+chi_1 = bilby.gw.prior.AlignedSpin(name='chi_1', a_prior=Uniform(minimum=0, maximum=0.99))
+chi_2 = bilby.gw.prior.AlignedSpin(name='chi_2', a_prior=Uniform(minimum=0, maximum=0.99))

test/prior_files/aligned_spins_bbh_tides_on.prior

+# These are the default priors we use for BBH systems.
+# Note that you may wish to use more specific mass and distance parameters.
+# These commands are all known to bilby.gw.prior.
+# Lines beginning "#" are ignored.
+mass_1 = Constraint(name='mass_1', minimum=5, maximum=100)
+mass_2 = Constraint(name='mass_2', minimum=5, maximum=100)
+mass_ratio = Uniform(name='mass_ratio', minimum=0.125, maximum=1)
+chirp_mass = Uniform(name='chirp_mass', minimum=25, maximum=100)
+luminosity_distance = bilby.gw.prior.UniformSourceFrame(name='luminosity_distance', minimum=1e2, maximum=5e3)
+dec = Cosine(name='dec')
+ra = Uniform(name='ra', minimum=0, maximum=2 * np.pi, boundary='periodic')
+theta_jn = Sine(name='theta_jn')
+psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
+phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')
+chi_1 = bilby.gw.prior.AlignedSpin(name='chi_1', a_prior=Uniform(minimum=0, maximum=0.99))
+chi_2 = bilby.gw.prior.AlignedSpin(name='chi_2', a_prior=Uniform(minimum=0, maximum=0.99))
+lambda_1 = Uniform(name='lambda_1', minimum=0, maximum=5000)
+lambda_2 = Uniform(name='lambda_2', minimum=0, maximum=5000)

test/prior_files/aligned_spins_bns.prior

+# These are the default priors we use for BNS systems.
+# Note that you may wish to use more specific mass and distance parameters.
+# These commands are all known to bilby.gw.prior.
+# Lines beginning "#" are ignored.
+mass_1 = Constraint(name='mass_1', minimum=0.5, maximum=5)
+mass_2 = Constraint(name='mass_2', minimum=0.5, maximum=5)
+mass_ratio = Uniform(name='mass_ratio', minimum=0.125, maximum=1)
+chirp_mass = Uniform(name='chirp_mass', minimum=0.4, maximum=4.4)
+luminosity_distance = bilby.gw.prior.UniformSourceFrame(name='luminosity_distance', minimum=1e2, maximum=5e3)
+dec = Cosine(name='dec')
+ra = Uniform(name='ra', minimum=0, maximum=2 * np.pi, boundary='periodic')
+theta_jn = Sine(name='theta_jn')
+psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
+phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')
+chi_1 = bilby.gw.prior.AlignedSpin(name='chi_1', a_prior=Uniform(minimum=0, maximum=0.99))
+chi_2 = bilby.gw.prior.AlignedSpin(name='chi_2', a_prior=Uniform(minimum=0, maximum=0.99))

test/prior_files/aligned_spins_bns_tides_on.prior

+# These are the default priors we use for BNS systems.
+# Note that you may wish to use more specific mass and distance parameters.
+# These commands are all known to bilby.gw.prior.
+# Lines beginning "#" are ignored.
+mass_1 = Constraint(name='mass_1', minimum=0.5, maximum=5)
+mass_2 = Constraint(name='mass_2', minimum=0.5, maximum=5)
+mass_ratio = Uniform(name='mass_ratio', minimum=0.125, maximum=1)
+chirp_mass = Uniform(name='chirp_mass', minimum=0.4, maximum=4.4)
+luminosity_distance = bilby.gw.prior.UniformSourceFrame(name='luminosity_distance', minimum=1e2, maximum=5e3)
+dec = Cosine(name='dec')
+ra = Uniform(name='ra', minimum=0, maximum=2 * np.pi, boundary='periodic')
+theta_jn = Sine(name='theta_jn')
+psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
+phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')
+chi_1 = bilby.gw.prior.AlignedSpin(name='chi_1', a_prior=Uniform(minimum=0, maximum=0.99))
+chi_2 = bilby.gw.prior.AlignedSpin(name='chi_2', a_prior=Uniform(minimum=0, maximum=0.99))
+lambda_1 = Uniform(name='lambda_1', minimum=0, maximum=5000)
+lambda_2 = Uniform(name='lambda_2', minimum=0, maximum=5000)

test/prior_files/aligned_spins_waveform_tides_on.prior

-chirp_mass = Uniform(name='chirp_mass', minimum=3.56, maximum=3.68)
-mass_ratio = Uniform(name='mass_ratio', minimum=0.05, maximum=1)
-mass_1 = Constraint(name='mass_1', minimum=1.00, maximum=22.0)
-mass_2 = Constraint(name='mass_2', minimum=1.00, maximum=2.95)
-chi_1 = bilby.gw.prior.AlignedSpin(name='chi_1', a_prior=Uniform(minimum=0, maximum=0.5))
-chi_2 = bilby.gw.prior.AlignedSpin(name='chi_2', a_prior=Uniform(minimum=0, maximum=0.05))
-luminosity_distance = bilby.core.prior.PowerLaw(alpha=2, name='luminosity_distance', minimum=1, maximum=750, unit='Mpc')
-ra = Uniform(minimum=0, maximum=2 * np.pi, name='ra',  boundary='periodic')
-dec = Cosine(name='dec')
-theta_jn = Sine(name='theta_jn')
-psi = Uniform(name='psi', minimum=0, maximum=np.pi, boundary='periodic')
-phase = Uniform(name='phase', minimum=0, maximum=2 * np.pi, boundary='periodic')
-lambda_1 = Uniform(name='lambda_2', minimum=0, maximum=5000)
-lambda_2 = Uniform(name='lambda_2', minimum=0, maximum=5000)