コード例 #1
0
ファイル: lightcurve.py プロジェクト: jefemagril/fermipy
def _process_lc_bin(itime, name, config, basedir, workdir, diff_sources, const_spectrum, roi, lck_params,
                    **kwargs):
    i, time = itime

    roi = copy.deepcopy(roi)

    config = copy.deepcopy(config)
    config['selection']['tmin'] = time[0]
    config['selection']['tmax'] = time[1]

    # create output directories labeled in MET vals
    outdir = basedir + 'lightcurve_%.0f_%.0f' % (time[0], time[1])
    config['fileio']['outdir'] = os.path.join(workdir, outdir)
    config['logging']['prefix'] = 'lightcurve_%.0f_%.0f ' % (time[0], time[1])
    config['fileio']['logfile'] = os.path.join(config['fileio']['outdir'],
                                               'fermipy.log')
    utils.mkdir(config['fileio']['outdir'])

    yaml.dump(utils.tolist(config),
              open(os.path.join(config['fileio']['outdir'],
                                'config.yaml'), 'w'))

    xmlfile = os.path.join(config['fileio']['outdir'], 'base.xml')

    try:
        from fermipy.gtanalysis import GTAnalysis
        gta = GTAnalysis(config, roi, loglevel=logging.DEBUG)
        gta.logger.info('Fitting time range %i %i' % (time[0], time[1]))
        gta.setup()
    except:
        print('Analysis failed in time range %i %i' %
              (time[0], time[1]))
        print(sys.exc_info()[0])
        raise
        return {}

    gta._lck_params = lck_params
    # Recompute source map for source of interest and sources within 3 deg
    if gta.config['gtlike']['use_scaled_srcmap']:
        names = [s.name for s in
                 gta.roi.get_sources(distance=3.0, skydir=gta.roi[name].skydir)
                 if not s.diffuse]
        gta.reload_sources(names)

    # Write the current model
    gta.write_xml(xmlfile)

    # Optimize the model
    gta.optimize(skip=diff_sources,
                 shape_ts_threshold=kwargs.get('shape_ts_threshold'))

    fit_results = _fit_lc(gta, name, **kwargs)
    gta.write_xml('fit_model_final.xml')
    srcmodel = copy.deepcopy(gta.get_src_model(name))
    numfree = gta.get_free_param_vector().count(True)

    max_ts_thresholds = [None, 4, 9]
    for max_ts in max_ts_thresholds:
        if max_ts is not None:
            gta.free_sources(minmax_ts=[None, max_ts], free=False, exclude=[name])

        # rerun fit using params from full time (constant) fit using same
        # param vector as the successful fit to get loglike
        specname, spectrum = const_spectrum
        gta.set_source_spectrum(name, spectrum_type=specname,
                                spectrum_pars=spectrum,
                                update_source=False)
        gta.free_source(name, free=False)
        const_fit_results = gta.fit()
        if not const_fit_results['fit_success']:
            continue
        const_srcmodel = gta.get_src_model(name)

        # rerun using shape fixed to full time fit
        # for the fixed-shape lightcurve
        gta.free_source(name, pars='norm')
        fixed_fit_results = gta.fit()
        if not fixed_fit_results['fit_success']:
            continue
        fixed_srcmodel = gta.get_src_model(name)
        break
    
    # special lc output
    o = {'flux_const': const_srcmodel['flux'],
         'loglike_const': const_fit_results['loglike'],
         'fit_success': fit_results['fit_success'],
         'fit_success_fixed': fixed_fit_results['fit_success'],
         'fit_quality': fit_results['fit_quality'],
         'fit_status': fit_results['fit_status'],
         'num_free_params': numfree,
         'config': config}

    # full flux output
    if fit_results['fit_success'] == 1:
        for k in defaults.source_flux_output.keys():
            if not k in srcmodel:
                continue
            o[k] = srcmodel[k]
            o[k+'_fixed'] = fixed_srcmodel[k]

    gta.logger.info('Finished time range %i %i' % (time[0], time[1]))
    return o
コード例 #2
0
def _process_lc_bin(itime, name, config, basedir, workdir, diff_sources, const_spectrum, roi, lck_params,
                    **kwargs):
    i, time = itime

    roi = copy.deepcopy(roi)

    config = copy.deepcopy(config)
    config['selection']['tmin'] = time[0]
    config['selection']['tmax'] = time[1]

    # create output directories labeled in MET vals
    outdir = basedir + 'lightcurve_%.0f_%.0f' % (time[0], time[1])
    config['fileio']['outdir'] = os.path.join(workdir, outdir)
    config['logging']['prefix'] = 'lightcurve_%.0f_%.0f ' % (time[0], time[1])
    config['fileio']['logfile'] = os.path.join(config['fileio']['outdir'],
                                               'fermipy.log')
    utils.mkdir(config['fileio']['outdir'])

    yaml.dump(utils.tolist(config),
              open(os.path.join(config['fileio']['outdir'],
                                'config.yaml'), 'w'))

    xmlfile = os.path.join(config['fileio']['outdir'], 'base.xml')

    try:
        from fermipy.gtanalysis import GTAnalysis
        gta = GTAnalysis(config, roi, loglevel=logging.DEBUG)
        gta.logger.info('Fitting time range %i %i' % (time[0], time[1]))
        gta.setup()
    except:
        print('Analysis failed in time range %i %i' %
              (time[0], time[1]))
        print(sys.exc_info()[0])
        raise
        return {}

    gta._lck_params = lck_params
    # Recompute source map for source of interest and sources within 3 deg
    if gta.config['gtlike']['use_scaled_srcmap']:
        names = [s.name for s in
                 gta.roi.get_sources(distance=3.0, skydir=gta.roi[name].skydir)
                 if not s.diffuse]
        gta.reload_sources(names)

    # Write the current model
    gta.write_xml(xmlfile)

    # Optimize the model
    gta.optimize(skip=diff_sources,
                 shape_ts_threshold=kwargs.get('shape_ts_threshold'))

    fit_results = _fit_lc(gta, name, **kwargs)
    gta.write_xml('fit_model_final.xml')
    srcmodel = copy.deepcopy(gta.get_src_model(name))
    numfree = gta.get_free_param_vector().count(True)
    
    const_srcmodel = gta.get_src_model(name).copy()
    fixed_fit_results = fit_results.copy()
    fixed_srcmodel = gta.get_src_model(name).copy()
    fixed_fit_results['fit_success'],fixed_srcmodel['fit_success'] = [False,False]
    fixed_fit_results['fit_quality'],fixed_srcmodel['fit_quality'] = [0,0]
    max_ts_thresholds = [None, 4, 9, 16, 25]
    for max_ts in max_ts_thresholds:
        if max_ts is not None:
            gta.free_sources(minmax_ts=[None, max_ts], free=False, exclude=[name])

        # rerun fit using params from full time (constant) fit using same
        # param vector as the successful fit to get loglike
        specname, spectrum = const_spectrum
        gta.set_source_spectrum(name, spectrum_type=specname,
                                spectrum_pars=spectrum,
                                update_source=False)
        gta.free_source(name, free=False)
        const_fit_results = gta.fit()
        if not const_fit_results['fit_success']:
            continue
        const_srcmodel = gta.get_src_model(name)
        # rerun using shape fixed to full time fit
        # for the fixed-shape lightcurve
        gta.free_source(name, pars='norm')
        fixed_fit_results = gta.fit()
	if not fixed_fit_results['fit_success']:
            continue
        fixed_srcmodel = gta.get_src_model(name)
        break
    
    # special lc output
    o = {'flux_const': const_srcmodel['flux'],
         'loglike_const': const_fit_results['loglike'],
         'fit_success': fit_results['fit_success'],
         'fit_success_fixed': fixed_fit_results['fit_success'],
         'fit_quality': fit_results['fit_quality'],
         'fit_status': fit_results['fit_status'],
         'num_free_params': numfree,
         'config': config}
    # full flux output
    if fit_results['fit_success'] == 1:
        for k in defaults.source_flux_output.keys():
            if not k in srcmodel:
                continue
            o[k] = srcmodel[k]
            o[k+'_fixed'] = fixed_srcmodel[k]

    gta.logger.info('Finished time range %i %i' % (time[0], time[1]))
    return o