Пример #1
0
def generate(ngen,
             surveyList=None,
             age_max=1.0E9,
             pDistPars=[.3, .15],
             bFieldPars=[12.65, 0.55],
             birthVPars=[0.0, 180.],
             siDistPars=[-1.6, 0.35],
             alignModel='orthogonal',
             lumDistType='fk06',
             lumDistPars=[-1.5, 0.5],
             alignTime=None,
             spinModel='fk06',
             beamModel='tm98',
             birthVModel='gaussian',
             electronModel='ne2001',
             braking_index=0,
             zscale=0.05,
             duty=5.,
             nodeathline=False,
             efficiencycut=None,
             nostdout=False,
             nospiralarms=False,
             keepdead=False):

    pop = Population()

    # set the parameters in the population object
    pop.pmean, pop.psigma = pDistPars
    pop.bmean, pop.bsigma = bFieldPars

    if lumDistType == 'pow':
        try:
            pop.lummin, pop.lummax, pop.lumpow = \
                lumDistPars[0], lumDistPars[1], lumDistPars[2]
        except ValueError:
            raise EvolveException('Not enough lum distn parameters for "pow"')

    elif lumDistType == 'fk06':
        pop.lumPar1, pop.lumPar2 = lumDistPars[0], lumDistPars[1]
        if len(lumDistPars) == 3:
            pop.lumPar3 = lumDistPars[2]
        else:
            pop.lumPar3 = 0.18

    else:
        pop.lumPar1, pop.lumPar2 = lumDistPars

    pop.simean, pop.sisigma = siDistPars
    pop.birthvmean, pop.birthvsigma = birthVPars

    pop.alignModel = alignModel
    pop.alignTime = alignTime
    pop.spinModel = spinModel
    pop.beamModel = beamModel
    pop.birthVModel = birthVModel
    pop.electronModel = electronModel

    pop.braking_index = braking_index
    pop.deathline = not nodeathline
    pop.nospiralarms = nospiralarms

    pop.zscale = zscale

    if not nostdout:
        print "\tGenerating evolved pulsars with parameters:"
        print "\t\tngen = {0}".format(ngen)
        print "\t\tUsing electron distn model {0}".format(pop.electronModel)
        print "\n\t\tPeriod mean, sigma = {0}, {1}".format(
            pop.pmean, pop.psigma)
        print "\t\tLuminosity mean, sigma = {0}, {1}".format(
            pop.lummean, pop.lumsigma)
        print "\t\tSpectral index mean, sigma = {0}, {1}".format(
            pop.simean, pop.sisigma)
        print "\t\tGalactic z scale height = {0} kpc".format(pop.zscale)

        print "\t\tWidth {0}% ".format(duty)

        # set up progress bar for fun :)
        prog = ProgressBar(min_value=0,
                           max_value=ngen,
                           width=65,
                           mode='dynamic')

    # create survey objects here and put them in a list
    if surveyList is not None:
        surveys = [Survey(s) for s in surveyList]
    else:
        # make an empty list here - makes some code just a little
        # simpler - can still loop over an empty list (ie zero times)
        surveys = []

    # initialise these counters to zero
    for surv in surveys:
        surv.ndet = 0  # number detected
        surv.nout = 0  # number outside survey region
        surv.nsmear = 0  # number smeared out
        surv.ntf = 0  # number too faint

    # this is the nitty-gritty loop for generating the pulsars
    while pop.ndet < ngen:
        pulsar = Pulsar()

        # initial age for pulsar
        pulsar.age = random.random() * age_max

        # initial period
        pulsar.p0 = -1.
        while pulsar.p0 <= 0.:
            pulsar.p0 = random.gauss(pop.pmean, pop.psigma)

        # initial magnetic field (in Gauss)
        pulsar.bfield_init = 10**random.gauss(pop.bmean, pop.bsigma)

        # aligment angle
        alignpulsar(pulsar, pop)

        # braking index
        if pop.braking_index == 0:
            pulsar.braking_index = 2.5 + 0.5 * random.random()
        else:
            pulsar.braking_index = float(pop.braking_index)

        #apply relevant spin down model
        pulsar.dead = False  # pulsar should start alive!

        if pop.spinModel == 'fk06':
            spindown_fk06(pulsar)

            # apply deathline if relevant
            if pop.deathline:
                bhattacharya_deathperiod_92(pulsar)

        elif pop.spinModel == 'cs06':
            # contopoulos and spitkovsky
            spindown_cs06(pulsar, pop)

        # define pulse width (default = 6% = 18 degrees)
        width = (float(duty) / 100.) * pulsar.period**0.9
        width = math.log10(width)
        width = dists.drawlnorm(width, 0.3)
        pulsar.width_degree = 360. * width / pulsar.period

        # plough on - only if the pulsar isn't dead!
        if not pulsar.dead or keepdead:
            # is the pulsar beaming?
            pulsar_beaming(pulsar, pop.beamModel)
            # if not, then skip onto next pulsar
            if not pulsar.beaming:
                continue

            # position of the pulsar
            galacticDistribute(pulsar, pop)
            # birthvelocity
            birthVelocity(pulsar, pop)

            # model the xyz velocity
            go.vxyz(pulsar)

            # luminosity
            if lumDistType == 'fk06':
                luminosity_fk06(pulsar,
                                alpha=pop.lumPar1,
                                beta=pop.lumPar2,
                                gamma=pop.lumPar3)

            elif lumDistType == 'lnorm':
                pulsar.lum_1400 = dists.drawlnorm(pop.lumPar1, pop.lumPar2)

            elif lumDistType == 'pow':
                pulsar.lum_1400 = dists.powerlaw(pop.lummin, pop.lummax,
                                                 pop.lumpow)
            else:
                # something's wrong!
                raise EvolveException('Invalid luminosity distn selected')

            # apply efficiency cutoff
            if efficiencycut is not None:
                if pulsar.efficiency() > efficiencycut:
                    pulsar.dead = True
                    if not keepdead:
                        continue

            # spectral index
            pulsar.spindex = random.gauss(pop.simean, pop.sisigma)

            # calculate galactic coords and distance
            pulsar.gl, pulsar.gb = go.xyz_to_lb(pulsar.galCoords)
            pulsar.dtrue = go.calc_dtrue(pulsar.galCoords)

            # then calc DM  using fortran libs
            if pop.electronModel == 'ne2001':
                pulsar.dm = go.ne2001_dist_to_dm(pulsar.dtrue, pulsar.gl,
                                                 pulsar.gb)
            elif pop.electronModel == 'lmt85':
                pulsar.dm = go.lmt85_dist_to_dm(pulsar.dtrue, pulsar.gl,
                                                pulsar.gb)
            else:
                raise EvolveException('Invalid electron dist model selected')

            # if surveys are given, check if pulsar detected or not
            # in ANY of the surveys
            if surveyList is not None:
                detect_int = 0  # just a flag if pulsar is detected
                for surv in surveys:
                    SNR = surv.SNRcalc(pulsar, pop)

                    if SNR > surv.SNRlimit:
                        # SNR is over threshold
                        # increment the flag
                        # and survey ndetected
                        detect_int += 1
                        surv.ndet += 1
                        continue

                    elif SNR == -1:
                        # pulse is smeared out
                        surv.nsmear += 1
                        continue

                    elif SNR == -2:
                        # pulsar is outside survey region
                        surv.nout += 1
                        continue

                    else:
                        #pulsar is just too faint
                        surv.ntf += 1
                        continue

                # if detected, increment ndet (for whole population)
                # and redraw the progress bar
                if detect_int:
                    pop.ndet += 1
                    # update the counter
                    if not nostdout:
                        prog.increment_amount()
                        print prog, '\r',
                        sys.stdout.flush()

            else:
                # no survey list, just add the pulsar to population,
                # and increment number of pulsars
                pop.ndet += 1
                # update the counter
                if not nostdout:
                    prog.increment_amount()
                    print prog, '\r',
                    sys.stdout.flush()

            # pulsar isn't dead, add to population!
            pop.population.append(pulsar)

        else:
            # pulsar is dead. If no survey list,
            # just increment number of pulsars
            if surveyList is None:
                pop.ndet += 1
                # update the counter
                if not nostdout:
                    prog.increment_amount()
                    print prog, '\r',
                    sys.stdout.flush()

    if not nostdout:
        print "\n\n"
        print "  Total pulsars = {0}".format(len(pop.population))
        print "  Total detected = {0}".format(pop.ndet)

        for surv in surveys:
            print "\n  Results for survey '{0}'".format(surv.surveyName)
            print "    Number detected = {0}".format(surv.ndet)
            print "    Number too faint = {0}".format(surv.ntf)
            print "    Number smeared = {0}".format(surv.nsmear)
            print "    Number outside survey area = {0}".format(surv.nout)

    # save list of arguments into the pop
    argspec = inspect.getargspec(generate)
    key_values = [(arg, locals()[arg]) for arg in argspec.args]
    pop.arguments = {key: value for (key, value) in key_values}

    return pop
Пример #2
0
def generate(ngen,
             surveyList=None,
             age_max=1.0E9,
             pDistPars=[.3, .15],
             bFieldPars=[12.65, 0.55],
             birthVPars=[0.0, 180.],
             siDistPars=[-1.6, 0.35],
             alignModel='orthogonal',
             lumDistType='fk06',
             lumDistPars=[-1.5, 0.5],
             alignTime=None,
             spinModel='fk06',
             beamModel='tm98',
             birthVModel='gaussian',
             electronModel='ne2001',
             braking_index=0,
             zscale=0.05,
             duty=5.,
             scindex=-3.86,
             widthModel=None,
             nodeathline=False,
             efficiencycut=None,
             nostdout=False,
             nospiralarms=False,
             keepdead=False):

    pop = Population()

    # set the parameters in the population object
    pop.pmean, pop.psigma = pDistPars
    pop.bmean, pop.bsigma = bFieldPars

    if lumDistType == 'pow':
        try:
            pop.lummin, pop.lummax, pop.lumpow = \
                lumDistPars[0], lumDistPars[1], lumDistPars[2]
        except ValueError:
            raise EvolveException('Not enough lum distn parameters for "pow"')

    elif lumDistType == 'fk06':
        pop.lumPar1, pop.lumPar2 = lumDistPars[0], lumDistPars[1]
        if len(lumDistPars) == 3:
            pop.lumPar3 = lumDistPars[2]
        else:
            pop.lumPar3 = 0.18

    else:
        pop.lumPar1, pop.lumPar2 = lumDistPars

    pop.simean, pop.sisigma = siDistPars
    pop.birthvmean, pop.birthvsigma = birthVPars

    pop.alignModel = alignModel
    pop.alignTime = alignTime
    pop.spinModel = spinModel
    pop.beamModel = beamModel
    pop.birthVModel = birthVModel
    pop.electronModel = electronModel

    pop.braking_index = braking_index
    pop.deathline = not nodeathline
    pop.nospiralarms = nospiralarms

    pop.zscale = zscale

    if widthModel == 'kj07':
        print "\tLoading KJ07 models...."
        kj_p_vals, kj_pdot_vals, kj_dists = beammodels.load_kj2007_models()
        print "\tDone\n"

    if not nostdout:
        print "\tGenerating evolved pulsars with parameters:"
        print "\t\tngen = {0}".format(ngen)
        print "\t\tUsing electron distn model {0}".format(
                                        pop.electronModel)
        print "\n\t\tPeriod mean, sigma = {0}, {1}".format(
                                                    pop.pmean,
                                                    pop.psigma)
        print "\t\tLuminosity mean, sigma = {0}, {1}".format(
                                                    pop.lummean,
                                                    pop.lumsigma)
        print "\t\tSpectral index mean, sigma = {0}, {1}".format(
                                                    pop.simean,
                                                    pop.sisigma)
        print "\t\tGalactic z scale height = {0} kpc".format(
                                                    pop.zscale)
        if widthModel is None:
            print "\t\tWidth {0}% ".format(duty)
        else:
            print "\t\tUsing Karastergiou & Johnston beam width model"

        # set up progress bar for fun :)
        prog = ProgressBar(min_value=0,
                           max_value=ngen,
                           width=65,
                           mode='dynamic')

    # create survey objects here and put them in a list
    if surveyList is not None:
        surveys = [Survey(s) for s in surveyList]
    else:
        # make an empty list here - makes some code just a little
        # simpler - can still loop over an empty list (ie zero times)
        surveys = []

    # initialise these counters to zero
    for surv in surveys:
        surv.ndet = 0  # number detected
        surv.nout = 0  # number outside survey region
        surv.nsmear = 0  # number smeared out
        surv.ntf = 0  # number too faint

    # this is the nitty-gritty loop for generating the pulsars
    while pop.ndet < ngen:
        pulsar = Pulsar()

        # initial age for pulsar
        pulsar.age = random.random() * age_max

        # initial period
        pulsar.p0 = -1.
        while pulsar.p0 <= 0.:
            pulsar.p0 = random.gauss(pop.pmean, pop.psigma)

        # initial magnetic field (in Gauss)
        pulsar.bfield_init = 10**random.gauss(pop.bmean, pop.bsigma)

        # aligment angle
        alignpulsar(pulsar, pop)

        # braking index
        if pop.braking_index == 0:
            pulsar.braking_index = 2.5 + 0.5 * random.random()
        else:
            pulsar.braking_index = float(pop.braking_index)

        # apply relevant spin down model
        pulsar.dead = False  # pulsar should start alive!

        if pop.spinModel == 'fk06':
            spindown_fk06(pulsar)

            # apply deathline if relevant
            if pop.deathline:
                bhattacharya_deathperiod_92(pulsar)

        elif pop.spinModel == 'cs06':
            # contopoulos and spitkovsky
            spindown_cs06(pulsar, pop)

        # if period > 10 seconds, just try a new one
        if pulsar.period > 10000.0 or pulsar.period < 10.:
            continue
        # cut on pdot too - this doesn't help
        if pulsar.pdot > 1.e-11 or pulsar.pdot < 1.e-18:
            continue

        # define pulse width (default = 6% = 18 degrees)
        if widthModel is None:
            width = (float(duty)/100.) * pulsar.period**0.9
            width = math.log10(width)
            width = dists.drawlnorm(width, 0.3)
        elif widthModel == 'kj07':
            # Karastergiou & Johnston beam model

            # find closest p, pdot in the kj lists
            logp = math.log10(pulsar.period)
            logpdot = math.log10(pulsar.pdot)

            p_idx = (np.abs(kj_p_vals - logp)).argmin()
            pd_idx = (np.abs(kj_pdot_vals - logpdot)).argmin()

            # pick a width from relevant model
            dist = kj_dists[p_idx][pd_idx][2]
            width = np.random.choice(dist)

            """
            width = beammodels.kj2007_width(pulsar)
            no_width = 0
            while width  == 0.0:
                no_width+=1
                width = beammodels.kj2007_width(pulsar)

                # if we get to five, then try a new pulsar
                if no_width == 5:
                    no_width = 0
                    continue
            """

        else:
            print "Undefined width model!"
            sys.exit()
        # print width
        # print pulsar.period, width, pulsar.pdot
        if width == 0.0:
            # some kj2007 models make many zero-width sources. Skip!
            continue
        pulsar.width_degree = 360. * width / pulsar.period

        # plough on - only if the pulsar isn't dead!
        if not pulsar.dead or keepdead:
            # is the pulsar beaming?
            pulsar_beaming(pulsar, pop.beamModel)
            # if not, then skip onto next pulsar
            if not pulsar.beaming:
                continue

            # position of the pulsar
            galacticDistribute(pulsar, pop)
            # birthvelocity
            birthVelocity(pulsar, pop)

            # model the xyz velocity
            go.vxyz(pulsar)

            # luminosity
            if lumDistType == 'fk06':
                luminosity_fk06(pulsar,
                                alpha=pop.lumPar1,
                                beta=pop.lumPar2,
                                gamma=pop.lumPar3)

            elif lumDistType == 'lnorm':
                pulsar.lum_1400 = dists.drawlnorm(pop.lumPar1, pop.lumPar2)

            elif lumDistType == 'pow':
                pulsar.lum_1400 = dists.powerlaw(pop.lummin,
                                                 pop.lummax,
                                                 pop.lumpow)
            else:
                # something's wrong!
                raise EvolveException('Invalid luminosity distn selected')

            # apply efficiency cutoff
            if efficiencycut is not None:
                if pulsar.efficiency() > efficiencycut:
                    pulsar.dead = True
                    if not keepdead:
                        continue

            # spectral index
            pulsar.spindex = random.gauss(pop.simean, pop.sisigma)

            # calculate galactic coords and distance
            pulsar.gl, pulsar.gb = go.xyz_to_lb(pulsar.galCoords)
            pulsar.dtrue = go.calc_dtrue(pulsar.galCoords)

            # then calc DM  using fortran libs
            if pop.electronModel == 'ne2001':
                pulsar.dm = go.ne2001_dist_to_dm(pulsar.dtrue,
                                                 pulsar.gl,
                                                 pulsar.gb)
            elif pop.electronModel == 'lmt85':
                pulsar.dm = go.lmt85_dist_to_dm(pulsar.dtrue,
                                                pulsar.gl,
                                                pulsar.gb)
            else:
                raise EvolveException('Invalid electron dist model selected')

            pulsar.scindex = scindex
            pulsar.t_scatter = go.scatter_bhat(pulsar.dm,
                                               pulsar.scindex)

            # if surveys are given, check if pulsar detected or not
            # in ANY of the surveys
            if surveyList is not None:
                detect_int = 0  # just a flag if pulsar is detected
                for surv in surveys:
                    SNR = surv.SNRcalc(pulsar, pop)

                    if SNR > surv.SNRlimit:
                        # SNR is over threshold
                        # increment the flag
                        # and survey ndetected
                        detect_int += 1
                        surv.ndet += 1
                        continue

                    elif SNR == -1:
                        # pulse is smeared out
                        surv.nsmear += 1
                        continue

                    elif SNR == -2:
                        # pulsar is outside survey region
                        surv.nout += 1
                        continue

                    else:
                        # pulsar is just too faint
                        surv.ntf += 1
                        continue

                # if detected, increment ndet (for whole population)
                # and redraw the progress bar
                if detect_int:
                    pop.ndet += 1
                    # update the counter
                    if not nostdout:
                        prog.increment_amount()
                        print prog, '\r',
                        sys.stdout.flush()

            else:
                # no survey list, just add the pulsar to population,
                # and increment number of pulsars
                pop.ndet += 1
                # update the counter
                if not nostdout:
                    prog.increment_amount()
                    print prog, '\r',
                    sys.stdout.flush()

            # pulsar isn't dead, add to population!
            pop.population.append(pulsar)

        else:
            # pulsar is dead. If no survey list,
            # just increment number of pulsars
            if surveyList is None:
                pop.ndet += 1
                # update the counter
                if not nostdout:
                    prog.increment_amount()
                    print prog, '\r',
                    sys.stdout.flush()

    if not nostdout:
        print "\n\n"
        print "  Total pulsars = {0}".format(len(pop.population))
        print "  Total detected = {0}".format(pop.ndet)

        for surv in surveys:
            print "\n  Results for survey '{0}'".format(surv.surveyName)
            print "    Number detected = {0}".format(surv.ndet)
            print "    Number too faint = {0}".format(surv.ntf)
            print "    Number smeared = {0}".format(surv.nsmear)
            print "    Number outside survey area = {0}".format(surv.nout)

    # save list of arguments into the pop
    try:
        argspec = inspect.getargspec(generate)
        key_values = [(arg, locals()[arg]) for arg in argspec.args]
        pop.arguments = {key: value for (key, value) in key_values}
    except SyntaxError:
        pass

    return pop
Пример #3
0
def generate(ngen,
             surveyList=None,
             age_max=1.0E9,
             pDistPars=[0.3, 0.15],
             pDistType = 'norm' ,           # P distirbution for MSPs (Lorimer et al. 2015)
             bFieldPars=[12.65, 0.55],
             birthVPars=[0.0, 180.],
             siDistPars=[-1.6, 0.35],
             alignModel='orthogonal',
             lumDistType='fk06',
             lumDistPars=[-1.5, 0.5],
             alignTime=None,
             spinModel='fk06',
             beamModel='tm98',
             birthVModel='gaussian',
             electronModel='ne2001',
             braking_index=0,
             zscale=0.05,
             duty=5.,
             scindex=-3.86,
             widthModel=None,
             nodeathline=False,
             efficiencycut=None,
             nostdout=False,
             nospiralarms=False,
             keepdead=False,
             dosurveyList = None,
             makepop=False):

    pop = Population()

    # set the parameters in the population object

    pop.pmean, pop.psigma = pDistPars
    pop.bmean, pop.bsigma = bFieldPars

    if lumDistType == 'pow':
        try:
            pop.lummin, pop.lummax, pop.lumpow = \
                lumDistPars[0], lumDistPars[1], lumDistPars[2]
        except ValueError:
            raise EvolveException('Not enough lum distn parameters for "pow"')

    elif lumDistType == 'fk06':
        pop.lumPar1, pop.lumPar2 = lumDistPars[0], lumDistPars[1]
        if len(lumDistPars) == 3:
            pop.lumPar3 = lumDistPars[2]
        else:
            pop.lumPar3 = 0.18

    else:
        pop.lumPar1, pop.lumPar2 = lumDistPars

    pop.simean, pop.sisigma = siDistPars
    pop.birthvmean, pop.birthvsigma = birthVPars

    pop.alignModel = alignModel
    pop.alignTime = alignTime
    pop.spinModel = spinModel
    pop.beamModel = beamModel
    pop.birthVModel = birthVModel
    pop.electronModel = electronModel

    pop.braking_index = braking_index
    pop.deathline = not nodeathline
    pop.nospiralarms = nospiralarms

    pop.zscale = zscale

    if widthModel == 'kj07':
        print "\tLoading KJ07 models...."
        kj_p_vals, kj_pdot_vals, kj_dists = beammodels.load_kj2007_models()
        print "\tDone\n"

    if not nostdout:
        print "\tGenerating evolved pulsars with parameters:"
        print "\t\tngen = {0}".format(ngen)
        print "\t\tUsing electron distn model {0}".format(
                                        pop.electronModel)
        print "\n\t\tPeriod mean, sigma = {0}, {1}".format(
                                                    pop.pmean,
                                                    pop.psigma)
        print "\t\tLuminosity mean, sigma = {0}, {1}".format(
                                                    pop.lummean,
                                                    pop.lumsigma)
        print "\t\tSpectral index mean, sigma = {0}, {1}".format(
                                                    pop.simean,
                                                    pop.sisigma)
        print "\t\tGalactic z scale height = {0} kpc".format(
                                                    pop.zscale)
        if widthModel is None:
            print "\t\tWidth {0}% ".format(duty)
        else:
            print "\t\tUsing Karastergiou & Johnston beam width model"

        # set up progress bar for fun :)
        prog = ProgressBar(min_value=0,
                           max_value=ngen,
                           width=65,
                           mode='dynamic')

    # create survey objects here and put them in a list
    if surveyList is not None:
        surveys = [Survey(s) for s in surveyList]
    else:
        # make an empty list here - makes some code just a little
        # simpler - can still loop over an empty list (ie zero times)
        surveys = []

    # initialise these counters to zero
    for surv in surveys:
        surv.ndet = 0  # number detected
        surv.nout = 0  # number outside survey region
        surv.nsmear = 0  # number smeared out
        surv.ntf = 0  # number too faint

    # create dosurvey objects here and put them in a list
    if dosurveyList is not None:
        dosurveys = [Survey(s) for s in dosurveyList]
        # initialise these counters to zero
        for surv in dosurveys:
            surv.ndet = 0  # number detected
            surv.nout = 0  # number outside survey region
            surv.nsmear = 0  # number smeared out
            surv.ntf = 0  # number too faint

            # surv.gainpat=pattern
    else:
        # make an empty list here - makes some code just a little
        # simpler - can still loop over an empty list (ie zero times)
        dosurveys = []

    # this is the nitty-gritty loop for generating the pulsars
    ntot = 0   #total number of pulsars generated by the while loop (including dead, and the ones not beaming towards us)
    n_alive = 0  #total number of pulsars which are alive (beaming + not beaming towards Earth)
    n_alive_beam = 0 #total number of alive pulsars beaming towards Earth    
    while pop.ndet < ngen:
        pulsar = Pulsar()

        # initial age for pulsar
        pulsar.age = random.random() * age_max
        # initial period
        pulsar.p0 = -1.
        while (pulsar.p0 <= 0.):
          if(pDistType == 'norm'):
            pulsar.p0 = random.gauss(pop.pmean, pop.psigma)
          elif(pDistType == 'drl15'):
            L_p0 = np.random.lognormal(mean = pop.pmean, sigma = pop.psigma)  
            pulsar.p0 = np.exp(L_p0)/1000         # period in seconds
        # initial magnetic field (in Gauss)
        pulsar.bfield_init = 10**random.gauss(pop.bmean, pop.bsigma)

        # aligment angle
        alignpulsar(pulsar, pop)

        # braking index
        if pop.braking_index == 0:
            pulsar.braking_index = 2.5 + 0.5 * random.random()
        else:
            pulsar.braking_index = float(pop.braking_index)

        # apply relevant spin down model
        pulsar.dead = False  # pulsar should start alive!

        if pop.spinModel == 'fk06':
            spindown_fk06(pulsar)

            # apply deathline if relevant
            if pop.deathline:
                bhattacharya_deathperiod_92(pulsar)

        elif pop.spinModel == 'tk01':
            spindown_tk01(pulsar)

            # apply deathline if relevant
            if pop.deathline:
                bhattacharya_deathperiod_92(pulsar)
 
        elif pop.spinModel == 'cs06':
            # contopoulos and spitkovsky
            spindown_cs06(pulsar, pop)

        # if period > 10 seconds, just try a new one
        if pulsar.period > 10000.0 or pulsar.period < 1.5:
            continue
        # cut on pdot too - this doesn't help
        if pulsar.pdot > 1.e-11 or pulsar.pdot < 1.e-21:
            continue

        # define pulse width (default = 6% = 18 degrees)
        if widthModel is None:
            width = (float(duty)/100.) * pulsar.period**0.9
            width = math.log10(width)
            width = dists.drawlnorm(width, 0.3)
        elif widthModel == 'kj07':
            # Karastergiou & Johnston beam model

            # find closest p, pdot in the kj lists
            logp = math.log10(pulsar.period)
            logpdot = math.log10(pulsar.pdot)

            p_idx = (np.abs(kj_p_vals - logp)).argmin()
            pd_idx = (np.abs(kj_pdot_vals - logpdot)).argmin()

            # pick a width from relevant model
            dist = kj_dists[p_idx][pd_idx][2]
            width = np.random.choice(dist)

            """
            width = beammodels.kj2007_width(pulsar)
            no_width = 0
            while width  == 0.0:
                no_width+=1
                width = beammodels.kj2007_width(pulsar)

                # if we get to five, then try a new pulsar
                if no_width == 5:
                    no_width = 0
                    continue
            """

        else:
            print "Undefined width model!"
            sys.exit()
        # print width
        # print pulsar.period, width, pulsar.pdot
        if width == 0.0:
            # some kj2007 models make many zero-width sources. Skip!
            continue
        pulsar.width_degree = 360. * width / pulsar.period

        # incrementing the total number of physical pulsars generated by
        # the model after the unphysical ones are removed
        ntot += 1
        # plough on - only if the pulsar isn't dead!
        if not pulsar.dead or keepdead:
            n_alive+=1
            # is the pulsar beaming?
            pulsar_beaming(pulsar, pop.beamModel)
            # if not, then skip onto next pulsar
            if not pulsar.beaming:
                continue

            # position of the pulsar
            galacticDistribute(pulsar, pop)
            # birthvelocity
            birthVelocity(pulsar, pop)

            # model the xyz velocity
            go.vxyz(pulsar)

            # luminosity
            if lumDistType == 'fk06':
                luminosity_fk06(pulsar,
                                alpha=pop.lumPar1,
                                beta=pop.lumPar2,
                                gamma=pop.lumPar3)

            elif lumDistType == 'lnorm':
                pulsar.lum_1400 = dists.drawlnorm(pop.lumPar1, pop.lumPar2)

            elif lumDistType == 'pow':
                pulsar.lum_1400 = dists.powerlaw(pop.lummin,
                                                 pop.lummax,
                                                 pop.lumpow)
            else:
                # something's wrong!
                raise EvolveException('Invalid luminosity distn selected')

            # apply efficiency cutoff
            if efficiencycut is not None:
                if pulsar.efficiency() > efficiencycut:
                    pulsar.dead = True
                    if not keepdead:
                        continue

            # spectral index
            pulsar.spindex = random.gauss(pop.simean, pop.sisigma)

            # calculate galactic coords and distance
            pulsar.gl, pulsar.gb = go.xyz_to_lb(pulsar.galCoords)
            pulsar.dtrue = go.calc_dtrue(pulsar.galCoords)

            # then calc DM  using fortran libs
            if pop.electronModel == 'ne2001':
                pulsar.dm = go.ne2001_dist_to_dm(pulsar.dtrue,
                                                 pulsar.gl,
                                                 pulsar.gb)
            elif pop.electronModel == 'lmt85':
                pulsar.dm = go.lmt85_dist_to_dm(pulsar.dtrue,
                                                pulsar.gl,
                                                pulsar.gb)
            else:
                raise EvolveException('Invalid electron dist model selected')

            pulsar.scindex = scindex
            pulsar.t_scatter = go.scatter_bhat(pulsar.dm,
                                               pulsar.scindex)

            # if surveys are given, check if pulsar detected or not
            # in ANY of the surveys
            if surveyList is not None:
                detect_int = 0  # just a flag if pulsar is detected
                for surv in surveys:
                    SNR = surv.SNRcalc(pulsar, pop)

                    if SNR > surv.SNRlimit:
                        # SNR is over threshold
                        # increment the flag
                        # and survey ndetected
                        detect_int += 1
                        surv.ndet += 1
                        continue

                    elif SNR == -1:
                        # pulse is smeared out
                        surv.nsmear += 1
                        continue

                    elif SNR == -2:
                        # pulsar is outside survey region
                        surv.nout += 1
                        continue

                    else:
                        # pulsar is just too faint
                        surv.ntf += 1
                        continue

                # if detected, increment ndet (for whole population)
                # and redraw the progress bar
                if detect_int:
                    pop.ndet += 1
                    # update the counter
                    if not nostdout:
                        prog.increment_amount()
                        print prog, '\r',
                        sys.stdout.flush()

            else:
                # no survey list, just add the pulsar to population,
                # and increment number of pulsars
                pop.ndet += 1
                # update the counter
                if not nostdout:
                    prog.increment_amount()
                    print prog, '\r',
                    sys.stdout.flush()

            # increment the total number of alive pulsars beaming towards Earth
            # should be different from n_alive (as the loop was stopped if pulsar
            # was found to not beam towards Earth)
            # is incremented only when pulsar was beaming towards us
            n_alive_beam += 1            
            
            # pulsar isn't dead, and makepop True, add the pulsar to population!
            if makepop == True:
                pop.population.append(pulsar)

            # if dosurveys are given, check if pulsar detected or not
            # in each of the surveys or any of the survey
            # just a flag to increment if pulsar is detected
            if dosurveyList is not None:
                for surv in dosurveys:
                    SNR = surv.SNRcalc(pulsar, pop)

                    if SNR > surv.SNRlimit:
                        # SNR is over threshold
                        # increment survey ndetected
                        surv.ndet += 1
                        continue

                    elif SNR == -1:
                        # pulse is smeared out
                        surv.nsmear += 1
                        continue

                    elif SNR == -2:
                        # pulsar is outside survey region
                        surv.nout += 1
                        continue

                    else:
                        # pulsar is just too faint
                        surv.ntf += 1
                        continue

        else:
            # pulsar is dead. If no survey list,
            # just increment number of pulsars
            if surveyList is None:
                pop.ndet = ntot 
                # update the counter
                if not nostdout:
                    prog.increment_amount()
                    print prog, '\r',
                    sys.stdout.flush()

    if not nostdout:
        print "\n\n"
#        print "  Total pulsars = {0}".format(len(pop.population))
#        print "  Total detected = {0}".format(pop.ndet)
        print "  Total pulsars generated = {0}".format(ntot)
        print "  Total living pulsars = {0}".format(n_alive)
        print "  Total living pulsars beaming towards Earth = {0}".format(n_alive_beam)

        if surveyList is not None:
            print "  Total detected by all surveys = {0}".format(pop.ndet)


        for surv in surveys:
            print "\n  Results for survey '{0}'".format(surv.surveyName)
            print "    Number detected = {0}".format(surv.ndet)
            print "    Number too faint = {0}".format(surv.ntf)
            print "    Number smeared = {0}".format(surv.nsmear)
            print "    Number outside survey area = {0}".format(surv.nout)

        for surv in dosurveys:
            print "\n  Dosurvey Results for survey '{0}'".format(surv.surveyName)
            print "    Number detected = {0}".format(surv.ndet)
            print "    Number too faint = {0}".format(surv.ntf)
            print "    Number smeared = {0}".format(surv.nsmear)
            print "    Number outside survey area = {0}".format(surv.nout)

    dosurvey_result = []
    for surv in dosurveys:
        dosurvey_result.append([surv.surveyName, surv.ndet, surv.ntf, surv.nsmear, surv.nout])

    # save list of arguments into the pop
    #try:
    #    argspec = inspect.getargspec(generate)
    #    key_values = [(arg, locals()[arg]) for arg in argspec.args]
    #    pop.arguments = {key: value for (key, value) in key_values}
    #except SyntaxError:
     #   pass

    return pop, dosurvey_result
Пример #4
0
def generate(ngen,
             surveyList=None,
             age_max=1.0E9,
             pDistPars=[.3, .15],
             bFieldPars=[12.65, 0.55],
             birthVPars=[0.0, 180.],
             siDistPars= [-1.6,0.35],
             alignModel='orthogonal',
             lumDistType='fk06',
             lumDistPars=[-1.5, 0.5],
             alignTime=None,
             spinModel = 'fk06',
             beamModel = 'tm98',
             birthVModel = 'gaussian',
             electronModel='ne2001',
             braking_index=0,
             zscale=0.33,
             duty=5.,
             nodeathline=False,
             nostdout=False,
             nospiralarms=False):


    pop = Population()

    # set the parameters in the population object
    pop.pmean, pop.psigma = pDistPars
    pop.bmean, pop.bsigma = bFieldPars
    if lumDistType=='pow':
        try:
            pop.lummin, pop.lummax, pop.lumpow = \
                lumDistPars[0], lumDistPars[1], lumDistPars[2]
        except ValueError:
            raise EvolveException('Not enough lum distn parameters')
    else:
        pop.lumPar1, pop.lumPar2 = lumDistPars

    pop.simean, pop.sisigma = siDistPars
    pop.birthvmean, pop.birthvsigma = birthVPars
    
    pop.alignModel = alignModel
    pop.alignTime= alignTime
    pop.spinModel = spinModel
    pop.beamModel = beamModel
    pop.birthVModel = birthVModel
    pop.electronModel = electronModel

    pop.braking_index = braking_index
    pop.nodeathline = nodeathline
    pop.nospiralarms = nospiralarms

    pop.zscale = zscale

    if not nostdout:
        print "\tGenerating evolved pulsars with parameters:"
        print "\t\tngen = {0}".format(ngen)
        print "\t\tUsing electron distn model {0}".format(
                                        pop.electronModel)
        print "\n\t\tPeriod mean, sigma = {0}, {1}".format(
                                                    pop.pmean,
                                                    pop.psigma)
        print "\t\tLuminosity mean, sigma = {0}, {1}".format(
                                                    pop.lummean,
                                                    pop.lumsigma)
        print "\t\tSpectral index mean, sigma = {0}, {1}".format(
                                                    pop.simean,
                                                    pop.sisigma)
        print "\t\tGalactic z scale height = {0} kpc".format(
                                                    pop.zscale)

        print "\t\tWidth {0}% ".format(duty)

        # set up progress bar for fun :)
        prog = ProgressBar(min_value = 0,
                           max_value=ngen,
                           width=65,
                           mode='dynamic')

    # create survey objects here and put them in a list
    if surveyList is not None:
        surveys = [Survey(s) for s in surveyList]
    else:
        # make an empty list here - makes some code just a little
        # simpler - can still loop over an empty list (ie zero times)
        surveys=[]

    # initialise these counters to zero 
    for surv in surveys:
        surv.ndet =0 # number detected
        surv.nout=0 # number outside survey region
        surv.nsmear=0 # number smeared out
        surv.ntf=0 # number too faint

    # this is the nitty-gritty loop for generating the pulsars
    while pop.ndet < ngen:
        pulsar = Pulsar()

        # initial age for pulsar
        pulsar.age = random.random() * age_max

        # initial period
        pulsar.p0 = -1.
        while pulsar.p0 <= 0.:
            pulsar.p0 = random.gauss(pop.pmean, pop.psigma)

        # initial magnetic field (in Gauss)
        pulsar.bfield_init = 10**random.gauss(pop.bmean, pop.bsigma)

        # aligment angle
        alignpulsar(pulsar, pop)

        # braking index
        if pop.braking_index == 0:
            pulsar.braking_index = 2.5 + 0.5 * random.random()
        else:
            pulsar.braking_index = float(pop.braking_index)

        #apply relevant spin down model
        pulsar.dead = False # pulsar should start alive! 

        if pop.spinModel == 'fk06':
            spindown_fk06(pulsar)

            # apply deathline if relevant
            if not pop.nodeathline:
                bhattacharya_deathperiod_92(pulsar)

        elif pop.spinModel == 'cs06':
            # contopoulos and spitkovsky
            spindown_cs06(pulsar, pop)

        # define pulse width (default = 5% = 18 degrees)
        pulsar.width_degree = 360. * duty /100.

        # plough on - only if the pulsar isn't dead!
        if not pulsar.dead:
            # is the pulsar beaming? 
            pulsar_beaming(pulsar, pop.beamModel)
            # if not, then skip onto next pulsar
            if not pulsar.beaming:
                continue

            # position of the pulsar       
            galacticDistribute(pulsar, pop)
            # birthvelocity
            birthVelocity(pulsar, pop)

            # model the xyz velocity
            go.vxyz(pulsar)

            # luminosity
            if lumDistType == 'fk06':
                luminosity_fk06(pulsar, alpha=pop.lumPar1, beta=pop.lumPar2)

            elif lumDistType == 'lnorm':
                pulsar.lum_1400 = populate._drawlnorm(pop.lumPar1, pop.lumPar2)

            elif lumDistType == 'pow':
                pulsar.lum_1400 = populate._powerlaw(pop.lummin,
                                                     pop.lummax,
                                                     pop.lumpow)
            else:
                # something's wrong!
                raise EvolveException('Invalid luminosity distn selected')

            # spectral index
            pulsar.spindex = random.gauss(pop.simean, pop.sisigma)

            # calculate galactic coords and distance
            pulsar.gl, pulsar.gb = go.xyz_to_lb(pulsar.galCoords)
            pulsar.dtrue = go.calc_dtrue(pulsar.galCoords)

            # then calc DM  using fortran libs
            if pop.electronModel == 'ne2001':
                pulsar.dm = go.ne2001_dist_to_dm(pulsar.dtrue,
                                                   pulsar.gl, 
                                                   pulsar.gb)
            elif pop.electronModel == 'lmt85':
                pulsar.dm = go.lmt85_dist_to_dm(pulsar.dtrue,
                                                  pulsar.gl, 
                                                  pulsar.gb)

            # if surveys are given, check if pulsar detected or not
            # in ANY of the surveys
            if surveyList is not None:
                detect_int = 0 # just a flag if pulsar is detected
                for surv in surveys:
                    SNR = surv.SNRcalc(pulsar, pop)

                    if SNR > surv.SNRlimit:
                        # SNR is over threshold
                        # increment the flag 
                        # and survey ndetected
                        detect_int += 1
                        surv.ndet += 1
                        continue

                    elif SNR == -1:
                        # pulse is smeared out
                        surv.nsmear += 1
                        continue

                    elif SNR == -2:
                        # pulsar is outside survey region
                        surv.nout += 1
                        continue

                    else:
                        #pulsar is just too faint
                        surv.ntf += 1
                        continue 
            
                # if detected, increment ndet (for whole population)
                # and redraw the progress bar
                if detect_int:
                    pop.ndet += 1
                    # update the counter
                    if not nostdout:
                        prog.increment_amount()
                        print prog, '\r',
                        sys.stdout.flush()

            else:
                # no survey list, just add the pulsar to population,
                # and increment number of pulsars
                pop.ndet +=1
                # update the counter
                if not nostdout:
                    prog.increment_amount()
                    print prog, '\r',
                    sys.stdout.flush()

            # pulsar isn't dead, add to population!
            pop.population.append(pulsar)

        else:
            # pulsar is dead. If no survey list, 
            # just increment number of pulsars
            if surveyList is None:
                pop.ndet += 1
                # update the counter
                if not nostdout:
                    prog.increment_amount()
                    print prog, '\r',
                    sys.stdout.flush()


    if not nostdout:
        print "\n\n"
        print "  Total pulsars = {0}".format(len(pop.population))
        print "  Total detected = {0}".format(pop.ndet)

        for surv in surveys:
            print "\n  Results for survey '{0}'".format(surv.surveyName)
            print "    Number detected = {0}".format(surv.ndet)
            print "    Number too faint = {0}".format(surv.ntf)
            print "    Number smeared = {0}".format(surv.nsmear)
            print "    Number outside survey area = {0}".format(surv.nout)

    return pop