def likelihood_function(right_ascension, declination, t_ref, phi_orb,
                            inclination, psi, distance):

        P.phi = right_ascension  # right ascension
        P.theta = declination  # declination
        P.tref = t_ref + fiducial_epoch  # ref. time (rel to epoch for data taking)
        P.phiref = phi_orb  # ref. orbital phase
        P.incl = inclination  # inclination
        P.psi = psi  # polarization angle
        P.dist = distance * 1.e6 * lal.PC_SI  # luminosity distance

        lnL = factored_likelihood.factored_log_likelihood(
            P, rholms_intp, cross_terms, opts.l_max)

        return numpy.exp(lnL)
 def likelihood_function(right_ascension, declination, t_ref, phi_orb, inclination, psi, distance):
     # use EXTREMELY many bits
     lnL = numpy.zeros(right_ascension.shape,dtype=numpy.float128)
     i = 0
     for ph, th, tr, phr, ic, ps, di in zip(right_ascension, declination,
             t_ref, phi_orb, inclination, psi, distance):
         P.phi = ph # right ascension
         P.theta = th # declination
         P.tref = fiducial_epoch + tr # ref. time (rel to epoch for data taking)
         P.phiref = phr # ref. orbital phase
         P.incl = ic # inclination
         P.psi = ps # polarization angle
         P.dist = di* 1.e6 * lal.PC_SI # luminosity distance
 
         lnL[i] = factored_likelihood.factored_log_likelihood(P, rholms_intp, cross_terms, opts.l_max)
         i+=1
 
     return numpy.exp(lnL)
 def likelihood_function(right_ascension, declination, t_ref, phi_orb, inclination, psi, distance):
     # use EXTREMELY many bits
     lnL = numpy.zeros(right_ascension.shape,dtype=numpy.float128)
     i = 0
     for ph, th, tr, phr, ic, ps, di in zip(right_ascension, declination,
             t_ref, phi_orb, inclination, psi, distance):
         P.phi = ph # right ascension
         P.theta = th # declination
         P.tref = fiducial_epoch + tr # ref. time (rel to epoch for data taking)
         P.phiref = phr # ref. orbital phase
         P.incl = ic # inclination
         P.psi = ps # polarization angle
         P.dist = di* 1.e6 * lal.PC_SI # luminosity distance
 
         lnL[i] = factored_likelihood.factored_log_likelihood(P, rholms_intp, cross_terms, opts.l_max)
         i+=1
 
     return numpy.exp(lnL)
t_window = 0.15
rholms_intp, cross_terms, rholms = factored_likelihood.precompute_likelihood_terms(fiducial_epoch, t_window, P, data_dict, psd_dict, opts.l_max, fmax, False, inv_spec_trunc_Q, T_spec)

if opts.pin_to_sim and not opts.zero_noise:
    P.copy_lsctables_sim_inspiral(sim_row)
    print "Pinned parameters from sim_inspiral"
    print "\tRA", P.phi, sim_row.longitude 
    print "\tdec", P.theta, sim_row.latitude 
    print "\tt ref %d.%d" % (P.tref.gpsSeconds, P.tref.gpsNanoSeconds), sim_row.get_time_geocent()
    print "\torb phase", P.phiref, sim_row.coa_phase # ref. orbital phase
    print "\tinclination", P.incl, sim_row.inclination # inclination
    print "\tpsi", P.psi, sim_row.polarization # polarization angle
    print "\tdistance", P.dist/(1e6 * lal.PC_SI), sim_row.distance  # luminosity distance

    logL = factored_likelihood.factored_log_likelihood(P, rholms_intp, cross_terms, opts.l_max)
    print "Pinned log likelihood: %g, (%g in \"SNR\")" % (logL, numpy.sqrt(2*logL))
    tref = float(P.tref)
    tvals = numpy.arange(tref-0.01, tref+0.01, 0.00001)
    logLs = []
    for t in tvals:
        P.tref = lal.LIGOTimeGPS(t)
        logLs.append(factored_likelihood.factored_log_likelihood(P, rholms_intp, cross_terms, opts.l_max))
    import matplotlib
    matplotlib.use("Agg")
    from matplotlib import pyplot
    print "Maximum logL is %g, (%g in \"SNR\")" % (max(logLs), numpy.sqrt(2*max(logLs)))
    print "Which occurs at sample", numpy.argmax(logLs)
    print "This corresponds to time %.20g" % tvals[numpy.argmax(logLs)]
    print "The data event time is:  %.20g" % sim_row.get_time_geocent()
    print "Difference from geocenter t_ref is %.20g" %\
示例#5
0
if opts.pin_to_sim:
    P.copy_lsctables_sim_inspiral(sim_row)
    print "Pinned parameters from sim_inspiral"
    print "\tRA", P.phi, sim_row.longitude
    print "\tdec", P.theta, sim_row.latitude
    print "\tt ref %d.%d" % (
        P.tref.gpsSeconds, P.tref.gpsNanoSeconds), sim_row.get_time_geocent()
    print "\torb phase", P.phiref, sim_row.coa_phase  # ref. orbital phase
    print "\tinclination", P.incl, sim_row.inclination  # inclination
    print "\tpsi", P.psi, sim_row.polarization  # polarization angle
    print "\tdistance", P.dist / (
        1e6 * lal.PC_SI), sim_row.distance  # luminosity distance

    logL = factored_likelihood.factored_log_likelihood(P, rholms_intp,
                                                       cross_termsU,
                                                       opts.l_max)
    print "Pinned log likelihood: %g, (%g in \"SNR\")" % (logL,
                                                          numpy.sqrt(2 * logL))
    tref = float(P.tref)
    tvals = numpy.arange(tref - 0.01, tref + 0.01, 0.00001)
    logLs = []
    for t in tvals:
        P.tref = lal.LIGOTimeGPS(t)
        logLs.append(
            factored_likelihood.factored_log_likelihood(
                P, rholms_intp, cross_termsU, opts.l_max))
    import matplotlib
    matplotlib.use("Agg")
    from matplotlib import pyplot
    print "Maximum logL is %g, (%g in \"SNR\")" % (max(logLs),
t_window = 0.15
rholms_intp, cross_terms, rholms = factored_likelihood.precompute_likelihood_terms(fiducial_epoch, t_window, P, data_dict, psd_dict, opts.l_max, fmax, False, inv_spec_trunc_Q, T_spec)

if opts.pin_to_sim and not opts.zero_noise:
    P.copy_lsctables_sim_inspiral(sim_row)
    print "Pinned parameters from sim_inspiral"
    print "\tRA", P.phi, sim_row.longitude 
    print "\tdec", P.theta, sim_row.latitude 
    print "\tt ref %d.%d" % (P.tref.gpsSeconds, P.tref.gpsNanoSeconds), sim_row.get_time_geocent()
    print "\torb phase", P.phiref, sim_row.coa_phase # ref. orbital phase
    print "\tinclination", P.incl, sim_row.inclination # inclination
    print "\tpsi", P.psi, sim_row.polarization # polarization angle
    print "\tdistance", P.dist/(1e6 * lal.PC_SI), sim_row.distance  # luminosity distance

    logL = factored_likelihood.factored_log_likelihood(P, rholms_intp, cross_terms, opts.l_max)
    print "Pinned log likelihood: %g, (%g in \"SNR\")" % (logL, numpy.sqrt(2*logL))
    tref = float(P.tref)
    tvals = numpy.arange(tref-0.01, tref+0.01, 0.00001)
    logLs = []
    for t in tvals:
        P.tref = lal.LIGOTimeGPS(t)
        logLs.append(factored_likelihood.factored_log_likelihood(P, rholms_intp, cross_terms, opts.l_max))
    import matplotlib
    matplotlib.use("Agg")
    from matplotlib import pyplot
    print "Maximum logL is %g, (%g in \"SNR\")" % (max(logLs), numpy.sqrt(2*max(logLs)))
    print "Which occurs at sample", numpy.argmax(logLs)
    print "This corresponds to time %.20g" % tvals[numpy.argmax(logLs)]
    print "The data event time is:  %.20g" % sim_row.get_time_geocent()
    print "Difference from geocenter t_ref is %.20g" %\