def test_energy_dispersion():
'''Test our energy dispersion is readable by gammapy'''
pytest.importorskip('gammapy')
from pyirf.io import create_energy_dispersion_hdu
from gammapy.irf import EnergyDispersion2D
e_bins = np.geomspace(0.1, 100, 31) * u.TeV
migra_bins = np.linspace(0.2, 5, 101)
fov_bins = [0, 1, 2, 3] * u.deg
edisp = np.zeros((30, 100, 3))
edisp[:, 50, :] = 1.0
for point_like in [True, False]:
with tempfile.NamedTemporaryFile(suffix='.fits') as f:
hdu = create_energy_dispersion_hdu(edisp,
e_bins,
migra_bins,
fov_bins,
point_like=point_like)
fits.HDUList([fits.PrimaryHDU(), hdu]).writeto(f.name)
# test reading with gammapy works
edisp2d = EnergyDispersion2D.read(f.name, 'EDISP')
assert u.allclose(edisp, edisp2d.data.data, atol=1e-16)
def edisp_hdus():
from pyirf.io import create_energy_dispersion_hdu
edisp = np.zeros((len(e_bins) - 1, len(migra_bins) - 1, len(fov_bins) - 1))
edisp[:, 50, :] = 1.0
hdus = [
create_energy_dispersion_hdu(edisp,
e_bins,
migra_bins,
fov_bins,
point_like=point_like)
for point_like in [True, False]
]
return edisp, hdus
def main():
# Read arguments
parser = argparse.ArgumentParser(description='Make performance files')
parser.add_argument('--config_file', type=str, required=True, help='')
mode_group = parser.add_mutually_exclusive_group()
mode_group.add_argument('--wave',
dest="mode",
action='store_const',
const="wave",
default="tail",
help="if set, use wavelet cleaning")
mode_group.add_argument('--tail',
dest="mode",
action='store_const',
const="tail",
help="if set, use tail cleaning (default)")
args = parser.parse_args()
# Read configuration file
cfg = load_config(args.config_file)
# Create output directory if necessary
outdir = os.path.join(
cfg['general']['outdir'],
'performance_protopipe_{}_CTA{}_{}_Zd{}_{}_Time{:.2f}{}'.format(
cfg['general']['prod'], cfg['general']['site'],
cfg['general']['array'], cfg['general']['zenith'],
cfg['general']['azimuth'], cfg['analysis']['obs_time']['value'],
cfg['analysis']['obs_time']['unit']),
)
indir = cfg['general']['indir']
template_input_file = cfg['general']['template_input_file']
T_OBS = cfg['analysis']['obs_time']['value'] * u.Unit(
cfg['analysis']['obs_time']['unit'])
# scaling between on and off region.
# Make off region 5 times larger than on region for better
# background statistics
ALPHA = cfg['analysis']['alpha']
# Radius to use for calculating bg rate
MAX_BG_RADIUS = cfg['analysis']['max_bg_radius'] * u.deg
particles = {
"gamma": {
"file":
os.path.join(indir, template_input_file.format(args.mode,
"gamma")),
"target_spectrum":
CRAB_HEGRA,
"run_header":
cfg['particle_information']['gamma']
},
"proton": {
"file":
os.path.join(indir,
template_input_file.format(args.mode, "proton")),
"target_spectrum":
IRFDOC_PROTON_SPECTRUM,
"run_header":
cfg['particle_information']['proton']
},
"electron": {
"file":
os.path.join(indir,
template_input_file.format(args.mode, "electron")),
"target_spectrum":
IRFDOC_ELECTRON_SPECTRUM,
"run_header":
cfg['particle_information']['electron']
},
}
logging.basicConfig(level=logging.INFO)
logging.getLogger("pyirf").setLevel(logging.DEBUG)
for particle_type, p in particles.items():
log.info(f"Simulated {particle_type.title()} Events:")
p["events"], p["simulation_info"] = read_DL2_pyirf(
p["file"], p["run_header"])
# Multiplicity cut
p["events"] = p["events"][
p["events"]["multiplicity"] >= cfg['analysis']
['cut_on_multiplicity']].copy()
p["simulated_spectrum"] = PowerLaw.from_simulation(
p["simulation_info"], T_OBS)
# Weight events
p["events"]["weight"] = calculate_event_weights(
p["events"]["true_energy"], p["target_spectrum"],
p["simulated_spectrum"])
for prefix in ('true', 'reco'):
k = f"{prefix}_source_fov_offset"
p["events"][k] = calculate_source_fov_offset(p["events"],
prefix=prefix)
# calculate theta / distance between reco and assuemd source positoin
# we handle only ON observations here, so the assumed source pos
# is the pointing position
p["events"]["theta"] = calculate_theta(
p["events"],
assumed_source_az=p["events"]["pointing_az"],
assumed_source_alt=p["events"]["pointing_alt"],
)
log.info(p["simulation_info"])
log.info("")
gammas = particles["gamma"]["events"]
# background table composed of both electrons and protons
background = table.vstack(
[particles["proton"]["events"], particles["electron"]["events"]])
MAX_GH_CUT_EFFICIENCY = 0.8
GH_CUT_EFFICIENCY_STEP = 0.01
# gh cut used for first calculation of the binned theta cuts
INITIAL_GH_CUT_EFFICENCY = 0.4
INITIAL_GH_CUT = np.quantile(gammas['gh_score'],
(1 - INITIAL_GH_CUT_EFFICENCY))
log.info(
f"Using fixed G/H cut of {INITIAL_GH_CUT} to calculate theta cuts")
# event display uses much finer bins for the theta cut than
# for the sensitivity
theta_bins = add_overflow_bins(
create_bins_per_decade(
10**(-1.9) * u.TeV,
10**2.3005 * u.TeV,
50,
))
# theta cut is 68 percent containmente of the gammas
# for now with a fixed global, unoptimized score cut
mask_theta_cuts = gammas["gh_score"] >= INITIAL_GH_CUT
theta_cuts = calculate_percentile_cut(
gammas["theta"][mask_theta_cuts],
gammas["reco_energy"][mask_theta_cuts],
bins=theta_bins,
min_value=0.05 * u.deg,
fill_value=0.32 * u.deg,
max_value=0.32 * u.deg,
percentile=68,
)
# same bins as event display uses
sensitivity_bins = add_overflow_bins(
create_bins_per_decade(10**-1.9 * u.TeV,
10**2.31 * u.TeV,
bins_per_decade=5))
log.info("Optimizing G/H separation cut for best sensitivity")
gh_cut_efficiencies = np.arange(
GH_CUT_EFFICIENCY_STEP,
MAX_GH_CUT_EFFICIENCY + GH_CUT_EFFICIENCY_STEP / 2,
GH_CUT_EFFICIENCY_STEP)
sensitivity_step_2, gh_cuts = optimize_gh_cut(
gammas,
background,
reco_energy_bins=sensitivity_bins,
gh_cut_efficiencies=gh_cut_efficiencies,
op=operator.ge,
theta_cuts=theta_cuts,
alpha=ALPHA,
background_radius=MAX_BG_RADIUS,
)
# now that we have the optimized gh cuts, we recalculate the theta
# cut as 68 percent containment on the events surviving these cuts.
log.info('Recalculating theta cut for optimized GH Cuts')
for tab in (gammas, background):
tab["selected_gh"] = evaluate_binned_cut(tab["gh_score"],
tab["reco_energy"], gh_cuts,
operator.ge)
theta_cuts_opt = calculate_percentile_cut(
gammas[gammas['selected_gh']]["theta"],
gammas[gammas['selected_gh']]["reco_energy"],
theta_bins,
percentile=68,
fill_value=0.32 * u.deg,
max_value=0.32 * u.deg,
min_value=0.05 * u.deg,
)
gammas["selected_theta"] = evaluate_binned_cut(gammas["theta"],
gammas["reco_energy"],
theta_cuts_opt, operator.le)
gammas["selected"] = gammas["selected_theta"] & gammas["selected_gh"]
# calculate sensitivity
signal_hist = create_histogram_table(gammas[gammas["selected"]],
bins=sensitivity_bins)
background_hist = estimate_background(
background[background["selected_gh"]],
reco_energy_bins=sensitivity_bins,
theta_cuts=theta_cuts_opt,
alpha=ALPHA,
background_radius=MAX_BG_RADIUS,
)
sensitivity = calculate_sensitivity(signal_hist,
background_hist,
alpha=ALPHA)
# scale relative sensitivity by Crab flux to get the flux sensitivity
spectrum = particles['gamma']['target_spectrum']
for s in (sensitivity_step_2, sensitivity):
s["flux_sensitivity"] = (s["relative_sensitivity"] *
spectrum(s['reco_energy_center']))
log.info('Calculating IRFs')
hdus = [
fits.PrimaryHDU(),
fits.BinTableHDU(sensitivity, name="SENSITIVITY"),
fits.BinTableHDU(sensitivity_step_2, name="SENSITIVITY_STEP_2"),
fits.BinTableHDU(theta_cuts, name="THETA_CUTS"),
fits.BinTableHDU(theta_cuts_opt, name="THETA_CUTS_OPT"),
fits.BinTableHDU(gh_cuts, name="GH_CUTS"),
]
masks = {
"": gammas["selected"],
"_NO_CUTS": slice(None),
"_ONLY_GH": gammas["selected_gh"],
"_ONLY_THETA": gammas["selected_theta"],
}
# binnings for the irfs
true_energy_bins = add_overflow_bins(
create_bins_per_decade(10**-1.9 * u.TeV, 10**2.31 * u.TeV, 10))
reco_energy_bins = add_overflow_bins(
create_bins_per_decade(10**-1.9 * u.TeV, 10**2.31 * u.TeV, 5))
fov_offset_bins = [0, 0.5] * u.deg
source_offset_bins = np.arange(0, 1 + 1e-4, 1e-3) * u.deg
energy_migration_bins = np.geomspace(0.2, 5, 200)
for label, mask in masks.items():
effective_area = effective_area_per_energy(
gammas[mask],
particles["gamma"]["simulation_info"],
true_energy_bins=true_energy_bins,
)
hdus.append(
create_aeff2d_hdu(
effective_area[..., np.newaxis], # +1 dimension for FOV offset
true_energy_bins,
fov_offset_bins,
extname="EFFECTIVE_AREA" + label,
))
edisp = energy_dispersion(
gammas[mask],
true_energy_bins=true_energy_bins,
fov_offset_bins=fov_offset_bins,
migration_bins=energy_migration_bins,
)
hdus.append(
create_energy_dispersion_hdu(
edisp,
true_energy_bins=true_energy_bins,
migration_bins=energy_migration_bins,
fov_offset_bins=fov_offset_bins,
extname="ENERGY_DISPERSION" + label,
))
# Here we use reconstructed energy instead of true energy for the sake of
# current pipelines comparisons
bias_resolution = energy_bias_resolution(gammas[gammas["selected"]],
reco_energy_bins,
energy_type="reco")
# Here we use reconstructed energy instead of true energy for the sake of
# current pipelines comparisons
ang_res = angular_resolution(gammas[gammas["selected_gh"]],
reco_energy_bins,
energy_type="reco")
psf = psf_table(
gammas[gammas["selected_gh"]],
true_energy_bins,
fov_offset_bins=fov_offset_bins,
source_offset_bins=source_offset_bins,
)
background_rate = background_2d(
background[background['selected_gh']],
reco_energy_bins,
fov_offset_bins=np.arange(0, 11) * u.deg,
t_obs=T_OBS,
)
hdus.append(
create_background_2d_hdu(
background_rate,
reco_energy_bins,
fov_offset_bins=np.arange(0, 11) * u.deg,
))
hdus.append(
create_psf_table_hdu(
psf,
true_energy_bins,
source_offset_bins,
fov_offset_bins,
))
hdus.append(
create_rad_max_hdu(theta_cuts_opt["cut"][:, np.newaxis], theta_bins,
fov_offset_bins))
hdus.append(fits.BinTableHDU(ang_res, name="ANGULAR_RESOLUTION"))
hdus.append(
fits.BinTableHDU(bias_resolution, name="ENERGY_BIAS_RESOLUTION"))
log.info('Writing outputfile')
fits.HDUList(hdus).writeto(outdir + '.fits.gz', overwrite=True)
def main():
log = logging.getLogger("lstchain MC DL2 to IRF - sensitivity curves")
parser = argparse.ArgumentParser(description="MC DL2 to IRF")
# Required arguments
parser.add_argument(
"--gamma-dl2", "-g", type=str, dest="gamma_file", help="Path to the dl2 gamma file"
)
parser.add_argument(
"--proton-dl2",
"-p",
type=str,
dest="proton_file",
help="Path to the dl2 proton file",
)
parser.add_argument(
"--electron-dl2",
"-e",
type=str,
dest="electron_file",
help="Path to the dl2 electron file",
)
parser.add_argument(
"--outfile",
"-o",
action="store",
type=str,
dest="outfile",
help="Path where to save IRF FITS file",
default="sensitivity.fits.gz",
)
parser.add_argument(
"--source_alt",
action="store",
type=float,
dest="source_alt",
help="Source altitude (optional). If not provided, it will be guessed from the gammas true altitude",
default=None
)
parser.add_argument(
"--source_az",
action="store",
type=float,
dest="source_az",
help="Source azimuth (optional). If not provided, it will be guessed from the gammas true altitude",
default=None
)
# Optional arguments
# parser.add_argument('--config', '-c', action='store', type=Path,
# dest='config_file',
# help='Path to a configuration file. If none is given, a standard configuration is applied',
# default=None
# )
args = parser.parse_args()
logging.basicConfig(level=logging.INFO)
logging.getLogger("pyirf").setLevel(logging.DEBUG)
particles = {
"gamma": {"file": args.gamma_file, "target_spectrum": CRAB_HEGRA},
"proton": {"file": args.proton_file, "target_spectrum": IRFDOC_PROTON_SPECTRUM},
"electron": {
"file": args.electron_file,
"target_spectrum": IRFDOC_ELECTRON_SPECTRUM,
},
}
for particle_type, p in particles.items():
log.info("Simulated Events: {}".format(particle_type.title()))
p["events"], p["simulation_info"] = read_mc_dl2_to_QTable(p["file"])
# p['events'] = filter_events(p['events'], filters)
print("=====", particle_type, "=====")
# p["events"]["particle_type"] = particle_type
p["simulated_spectrum"] = PowerLaw.from_simulation(p["simulation_info"], T_OBS)
p["events"]["weight"] = calculate_event_weights(
p["events"]["true_energy"], p["target_spectrum"], p["simulated_spectrum"]
)
for prefix in ("true", "reco"):
k = f"{prefix}_source_fov_offset"
p["events"][k] = calculate_source_fov_offset(p["events"], prefix=prefix)
gammas = particles["gamma"]["events"]
# background table composed of both electrons and protons
background = table.vstack(
[particles["proton"]["events"], particles["electron"]["events"]]
)
if args.source_alt is None or args.source_az is None:
source_alt, source_az = determine_source_position(gammas)
else:
source_alt, source_az = args.source_alt, args.source_az
for particle_type, p in particles.items():
# calculate theta / distance between reco and assumed source position
# we handle only ON observations here, so the assumed source pos is the pointing position
p["events"]["theta"] = calculate_theta(p["events"], assumed_source_az=source_az, assumed_source_alt=source_alt)
log.info(p["simulation_info"])
log.info("")
INITIAL_GH_CUT = np.quantile(gammas["gh_score"], (1 - INITIAL_GH_CUT_EFFICENCY))
log.info("Using fixed G/H cut of {} to calculate theta cuts".format(INITIAL_GH_CUT))
# event display uses much finer bins for the theta cut than
# for the sensitivity
theta_bins = add_overflow_bins(
create_bins_per_decade(MIN_ENERGY, MAX_ENERGY, N_BIN_PER_DECADE)
)
# theta cut is 68 percent containment of the gammas
# for now with a fixed global, unoptimized score cut
mask_theta_cuts = gammas["gh_score"] >= INITIAL_GH_CUT
theta_cuts = calculate_percentile_cut(
gammas["theta"][mask_theta_cuts],
gammas["reco_energy"][mask_theta_cuts],
bins=theta_bins,
min_value=MIN_THETA_CUT,
fill_value=MAX_THETA_CUT,
max_value=MAX_THETA_CUT,
percentile=68,
)
# same number of bins per decade than official CTA IRFs
sensitivity_bins = add_overflow_bins(
create_bins_per_decade(MIN_ENERGY, MAX_ENERGY, bins_per_decade=N_BIN_PER_DECADE)
)
log.info("Optimizing G/H separation cut for best sensitivity")
gh_cut_efficiencies = np.arange(
GH_CUT_EFFICIENCY_STEP,
MAX_GH_CUT_EFFICIENCY + GH_CUT_EFFICIENCY_STEP / 2,
GH_CUT_EFFICIENCY_STEP,
)
sensitivity_step_2, gh_cuts = optimize_gh_cut(
gammas,
background,
reco_energy_bins=sensitivity_bins,
gh_cut_efficiencies=gh_cut_efficiencies,
op=operator.ge,
theta_cuts=theta_cuts,
alpha=ALPHA,
background_radius=MAX_BG_RADIUS,
)
# now that we have the optimized gh cuts, we recalculate the theta
# cut as 68 percent containment on the events surviving these cuts.
log.info("Recalculating theta cut for optimized GH Cuts")
for tab in (gammas, background):
tab["selected_gh"] = evaluate_binned_cut(
tab["gh_score"], tab["reco_energy"], gh_cuts, operator.ge
)
theta_cuts_opt = calculate_percentile_cut(
gammas[gammas["selected_gh"]]["theta"],
gammas[gammas["selected_gh"]]["reco_energy"],
theta_bins,
percentile=68,
fill_value=MAX_THETA_CUT,
max_value=MAX_THETA_CUT,
min_value=MIN_THETA_CUT,
)
gammas["selected_theta"] = evaluate_binned_cut(
gammas["theta"], gammas["reco_energy"], theta_cuts_opt, operator.le
)
gammas["selected"] = gammas["selected_theta"] & gammas["selected_gh"]
# calculate sensitivity
signal_hist = create_histogram_table(
gammas[gammas["selected"]], bins=sensitivity_bins
)
background_hist = estimate_background(
background[background["selected_gh"]],
reco_energy_bins=sensitivity_bins,
theta_cuts=theta_cuts_opt,
alpha=ALPHA,
background_radius=MAX_BG_RADIUS,
)
sensitivity = calculate_sensitivity(signal_hist, background_hist, alpha=ALPHA)
# scale relative sensitivity by Crab flux to get the flux sensitivity
spectrum = particles["gamma"]["target_spectrum"]
for s in (sensitivity_step_2, sensitivity):
s["flux_sensitivity"] = s["relative_sensitivity"] * spectrum(
s["reco_energy_center"]
)
log.info("Calculating IRFs")
hdus = [
fits.PrimaryHDU(),
fits.BinTableHDU(sensitivity, name="SENSITIVITY"),
fits.BinTableHDU(sensitivity_step_2, name="SENSITIVITY_STEP_2"),
fits.BinTableHDU(theta_cuts, name="THETA_CUTS"),
fits.BinTableHDU(theta_cuts_opt, name="THETA_CUTS_OPT"),
fits.BinTableHDU(gh_cuts, name="GH_CUTS"),
]
masks = {
"": gammas["selected"],
"_NO_CUTS": slice(None),
"_ONLY_GH": gammas["selected_gh"],
"_ONLY_THETA": gammas["selected_theta"],
}
# binnings for the irfs
true_energy_bins = add_overflow_bins(
create_bins_per_decade(MIN_ENERGY, MAX_ENERGY, N_BIN_PER_DECADE)
)
reco_energy_bins = add_overflow_bins(
create_bins_per_decade(MIN_ENERGY, MAX_ENERGY, N_BIN_PER_DECADE)
)
fov_offset_bins = [0, 0.6] * u.deg
source_offset_bins = np.arange(0, 1 + 1e-4, 1e-3) * u.deg
energy_migration_bins = np.geomspace(0.2, 5, 200)
for label, mask in masks.items():
effective_area = effective_area_per_energy(
gammas[mask],
particles["gamma"]["simulation_info"],
true_energy_bins=true_energy_bins,
)
hdus.append(
create_aeff2d_hdu(
effective_area[..., np.newaxis], # add one dimension for FOV offset
true_energy_bins,
fov_offset_bins,
extname="EFFECTIVE_AREA" + label,
)
)
edisp = energy_dispersion(
gammas[mask],
true_energy_bins=true_energy_bins,
fov_offset_bins=fov_offset_bins,
migration_bins=energy_migration_bins,
)
hdus.append(
create_energy_dispersion_hdu(
edisp,
true_energy_bins=true_energy_bins,
migration_bins=energy_migration_bins,
fov_offset_bins=fov_offset_bins,
extname="ENERGY_DISPERSION" + label,
)
)
bias_resolution = energy_bias_resolution(
gammas[gammas["selected"]],
true_energy_bins,
resolution_function=energy_resolution_absolute_68,
)
ang_res = angular_resolution(gammas[gammas["selected_gh"]], true_energy_bins)
psf = psf_table(
gammas[gammas["selected_gh"]],
true_energy_bins,
fov_offset_bins=fov_offset_bins,
source_offset_bins=source_offset_bins,
)
background_rate = background_2d(
background[background["selected_gh"]],
reco_energy_bins,
fov_offset_bins=np.arange(0, 11) * u.deg,
t_obs=T_OBS,
)
hdus.append(
create_background_2d_hdu(
background_rate, reco_energy_bins, fov_offset_bins=np.arange(0, 11) * u.deg
)
)
hdus.append(
create_psf_table_hdu(psf, true_energy_bins, source_offset_bins, fov_offset_bins)
)
hdus.append(
create_rad_max_hdu(
theta_cuts_opt["cut"][:, np.newaxis], theta_bins, fov_offset_bins
)
)
hdus.append(fits.BinTableHDU(ang_res, name="ANGULAR_RESOLUTION"))
hdus.append(fits.BinTableHDU(bias_resolution, name="ENERGY_BIAS_RESOLUTION"))
log.info("Writing output file")
Path(args.outfile).parent.mkdir(exist_ok=True)
fits.HDUList(hdus).writeto(args.outfile, overwrite=True)
def main():
logging.basicConfig(level=logging.INFO)
logging.getLogger("pyirf").setLevel(logging.DEBUG)
for k, p in particles.items():
log.info(f"Simulated {k.title()} Events:")
p["events"], p["simulation_info"] = read_eventdisplay_fits(p["file"])
p["simulated_spectrum"] = PowerLaw.from_simulation(
p["simulation_info"], T_OBS)
p["events"]["weight"] = calculate_event_weights(
p["events"]["true_energy"], p["target_spectrum"],
p["simulated_spectrum"])
p["events"]["source_fov_offset"] = calculate_source_fov_offset(
p["events"])
# calculate theta / distance between reco and assuemd source positoin
# we handle only ON observations here, so the assumed source pos
# is the pointing position
p["events"]["theta"] = calculate_theta(
p["events"],
assumed_source_az=p["events"]["pointing_az"],
assumed_source_alt=p["events"]["pointing_alt"],
)
log.info(p["simulation_info"])
log.info("")
gammas = particles["gamma"]["events"]
# background table composed of both electrons and protons
background = table.vstack(
[particles["proton"]["events"], particles["electron"]["events"]])
log.info(
f"Using fixed G/H cut of {INITIAL_GH_CUT} to calculate theta cuts")
# event display uses much finer bins for the theta cut than
# for the sensitivity
theta_bins = add_overflow_bins(
create_bins_per_decade(
10**(-1.9) * u.TeV,
10**2.3005 * u.TeV,
50,
))
# theta cut is 68 percent containmente of the gammas
# for now with a fixed global, unoptimized score cut
mask_theta_cuts = gammas["gh_score"] >= INITIAL_GH_CUT
theta_cuts = calculate_percentile_cut(
gammas["theta"][mask_theta_cuts],
gammas["reco_energy"][mask_theta_cuts],
bins=theta_bins,
min_value=0.05 * u.deg,
fill_value=np.nan * u.deg,
percentile=68,
)
# evaluate the theta cut
gammas["selected_theta"] = evaluate_binned_cut(gammas["theta"],
gammas["reco_energy"],
theta_cuts, operator.le)
# we make the background region larger by a factor of ALPHA,
# so the radius by sqrt(ALPHA) to get better statistics for the background
theta_cuts_bg = get_bg_cuts(theta_cuts, ALPHA)
background["selected_theta"] = evaluate_binned_cut(
background["theta"], background["reco_energy"], theta_cuts_bg,
operator.le)
# same bins as event display uses
sensitivity_bins = add_overflow_bins(
create_bins_per_decade(10**-1.9 * u.TeV,
10**2.31 * u.TeV,
bins_per_decade=5))
log.info("Optimizing G/H separation cut for best sensitivity")
sensitivity_step_2, gh_cuts = optimize_gh_cut(
gammas[gammas["selected_theta"]],
background[background["selected_theta"]],
bins=sensitivity_bins,
cut_values=np.arange(-1.0, 1.005, 0.05),
op=operator.ge,
alpha=ALPHA,
)
# now that we have the optimized gh cuts, we recalculate the theta
# cut as 68 percent containment on the events surviving these cuts.
for tab in (gammas, background):
tab["selected_gh"] = evaluate_binned_cut(tab["gh_score"],
tab["reco_energy"], gh_cuts,
operator.ge)
theta_cuts_opt = calculate_percentile_cut(
gammas["theta"],
gammas["reco_energy"],
theta_bins,
fill_value=np.nan * u.deg,
percentile=68,
min_value=0.05 * u.deg,
)
theta_cuts_opt_bg = get_bg_cuts(theta_cuts_opt, ALPHA)
for tab, cuts in zip([gammas, background],
[theta_cuts_opt, theta_cuts_opt_bg]):
tab["selected_theta"] = evaluate_binned_cut(tab["theta"],
tab["reco_energy"], cuts,
operator.le)
tab["selected"] = tab["selected_theta"] & tab["selected_gh"]
signal_hist = create_histogram_table(gammas[gammas["selected"]],
bins=sensitivity_bins)
background_hist = create_histogram_table(
background[background["selected"]], bins=sensitivity_bins)
sensitivity = calculate_sensitivity(signal_hist,
background_hist,
alpha=ALPHA)
# scale relative sensitivity by Crab flux to get the flux sensitivity
for s in (sensitivity_step_2, sensitivity):
s["flux_sensitivity"] = s["relative_sensitivity"] * CRAB_HEGRA(
s["reco_energy_center"])
# write OGADF output file
hdus = [
fits.PrimaryHDU(),
fits.BinTableHDU(sensitivity, name="SENSITIVITY"),
fits.BinTableHDU(sensitivity_step_2, name="SENSITIVITY_STEP_2"),
fits.BinTableHDU(theta_cuts, name="THETA_CUTS"),
fits.BinTableHDU(theta_cuts_opt, name="THETA_CUTS_OPT"),
fits.BinTableHDU(gh_cuts, name="GH_CUTS"),
]
masks = {
"": gammas["selected"],
"_NO_CUTS": slice(None),
"_ONLY_GH": gammas["selected_gh"],
"_ONLY_THETA": gammas["selected_theta"],
}
# binnings for the irfs
true_energy_bins = add_overflow_bins(
create_bins_per_decade(
10**-1.9 * u.TeV,
10**2.31 * u.TeV,
10,
))
reco_energy_bins = add_overflow_bins(
create_bins_per_decade(
10**-1.9 * u.TeV,
10**2.31 * u.TeV,
10,
))
fov_offset_bins = [0, 0.5] * u.deg
source_offset_bins = np.arange(0, 1 + 1e-4, 1e-3) * u.deg
energy_migration_bins = np.geomspace(0.2, 5, 200)
for label, mask in masks.items():
effective_area = point_like_effective_area(
gammas[mask],
particles["gamma"]["simulation_info"],
true_energy_bins=true_energy_bins,
)
hdus.append(
create_aeff2d_hdu(
effective_area[...,
np.newaxis], # add one dimension for FOV offset
true_energy_bins,
fov_offset_bins,
extname="EFFECTIVE_AREA" + label,
))
edisp = energy_dispersion(
gammas[mask],
true_energy_bins=true_energy_bins,
fov_offset_bins=fov_offset_bins,
migration_bins=energy_migration_bins,
)
hdus.append(
create_energy_dispersion_hdu(
edisp,
true_energy_bins=true_energy_bins,
migration_bins=energy_migration_bins,
fov_offset_bins=fov_offset_bins,
extname="ENERGY_DISPERSION" + label,
))
bias_resolution = energy_bias_resolution(
gammas[gammas["selected"]],
true_energy_bins,
)
ang_res = angular_resolution(
gammas[gammas["selected_gh"]],
true_energy_bins,
)
psf = psf_table(
gammas[gammas["selected_gh"]],
true_energy_bins,
fov_offset_bins=fov_offset_bins,
source_offset_bins=source_offset_bins,
)
background_rate = background_2d(
background[background['selected_gh']],
reco_energy_bins,
fov_offset_bins=np.arange(0, 11) * u.deg,
t_obs=T_OBS,
)
hdus.append(
create_background_2d_hdu(
background_rate,
reco_energy_bins,
fov_offset_bins=np.arange(0, 11) * u.deg,
))
hdus.append(
create_psf_table_hdu(
psf,
true_energy_bins,
source_offset_bins,
fov_offset_bins,
))
hdus.append(
create_rad_max_hdu(theta_bins,
fov_offset_bins,
rad_max=theta_cuts_opt["cut"][:, np.newaxis]))
hdus.append(fits.BinTableHDU(ang_res, name="ANGULAR_RESOLUTION"))
hdus.append(
fits.BinTableHDU(bias_resolution, name="ENERGY_BIAS_RESOLUTION"))
fits.HDUList(hdus).writeto("pyirf_eventdisplay.fits.gz", overwrite=True)
def main():
logging.basicConfig(level=logging.INFO)
logging.getLogger("pyirf").setLevel(logging.DEBUG)
for particle_type, p in particles.items():
log.info(f"Simulated {particle_type.title()} Events:")
p["events"], p["simulation_info"] = read_eventdisplay_fits(p["file"])
p["events"]["particle_type"] = particle_type
p["simulated_spectrum"] = PowerLaw.from_simulation(
p["simulation_info"], T_OBS)
p["events"]["weight"] = calculate_event_weights(
p["events"]["true_energy"], p["target_spectrum"],
p["simulated_spectrum"])
for prefix in ('true', 'reco'):
k = f"{prefix}_source_fov_offset"
p["events"][k] = calculate_source_fov_offset(p["events"],
prefix=prefix)
# calculate theta / distance between reco and assuemd source positoin
# we handle only ON observations here, so the assumed source pos
# is the pointing position
p["events"]["theta"] = calculate_theta(
p["events"],
assumed_source_az=p["events"]["pointing_az"],
assumed_source_alt=p["events"]["pointing_alt"],
)
log.info(p["simulation_info"])
log.info("")
gammas = particles["gamma"]["events"]
# background table composed of both electrons and protons
background = table.vstack(
[particles["proton"]["events"], particles["electron"]["events"]])
INITIAL_GH_CUT = np.quantile(gammas['gh_score'],
(1 - INITIAL_GH_CUT_EFFICENCY))
log.info(
f"Using fixed G/H cut of {INITIAL_GH_CUT} to calculate theta cuts")
# event display uses much finer bins for the theta cut than
# for the sensitivity
theta_bins = add_overflow_bins(
create_bins_per_decade(10**(-1.9) * u.TeV, 10**2.3005 * u.TeV, 50))
# same bins as event display uses
sensitivity_bins = add_overflow_bins(
create_bins_per_decade(10**-1.9 * u.TeV,
10**2.31 * u.TeV,
bins_per_decade=5))
# theta cut is 68 percent containmente of the gammas
# for now with a fixed global, unoptimized score cut
# the cut is calculated in the same bins as the sensitivity,
# but then interpolated to 10x the resolution.
mask_theta_cuts = gammas["gh_score"] >= INITIAL_GH_CUT
theta_cuts_coarse = calculate_percentile_cut(
gammas["theta"][mask_theta_cuts],
gammas["reco_energy"][mask_theta_cuts],
bins=sensitivity_bins,
min_value=0.05 * u.deg,
fill_value=0.32 * u.deg,
max_value=0.32 * u.deg,
percentile=68,
)
# interpolate to 50 bins per decade
theta_center = bin_center(theta_bins)
inter_center = bin_center(sensitivity_bins)
theta_cuts = table.QTable({
"low":
theta_bins[:-1],
"high":
theta_bins[1:],
"center":
theta_center,
"cut":
np.interp(np.log10(theta_center / u.TeV),
np.log10(inter_center / u.TeV), theta_cuts_coarse['cut']),
})
log.info("Optimizing G/H separation cut for best sensitivity")
gh_cut_efficiencies = np.arange(
GH_CUT_EFFICIENCY_STEP,
MAX_GH_CUT_EFFICIENCY + GH_CUT_EFFICIENCY_STEP / 2,
GH_CUT_EFFICIENCY_STEP)
sensitivity, gh_cuts = optimize_gh_cut(
gammas,
background,
reco_energy_bins=sensitivity_bins,
gh_cut_efficiencies=gh_cut_efficiencies,
op=operator.ge,
theta_cuts=theta_cuts,
alpha=ALPHA,
background_radius=MAX_BG_RADIUS,
)
# now that we have the optimized gh cuts, we recalculate the theta
# cut as 68 percent containment on the events surviving these cuts.
log.info('Recalculating theta cut for optimized GH Cuts')
for tab in (gammas, background):
tab["selected_gh"] = evaluate_binned_cut(tab["gh_score"],
tab["reco_energy"], gh_cuts,
operator.ge)
gammas["selected_theta"] = evaluate_binned_cut(gammas["theta"],
gammas["reco_energy"],
theta_cuts, operator.le)
gammas["selected"] = gammas["selected_theta"] & gammas["selected_gh"]
# scale relative sensitivity by Crab flux to get the flux sensitivity
spectrum = particles['gamma']['target_spectrum']
sensitivity["flux_sensitivity"] = (
sensitivity["relative_sensitivity"] *
spectrum(sensitivity['reco_energy_center']))
log.info('Calculating IRFs')
hdus = [
fits.PrimaryHDU(),
fits.BinTableHDU(sensitivity, name="SENSITIVITY"),
fits.BinTableHDU(theta_cuts, name="THETA_CUTS"),
fits.BinTableHDU(gh_cuts, name="GH_CUTS"),
]
masks = {
"": gammas["selected"],
"_NO_CUTS": slice(None),
"_ONLY_GH": gammas["selected_gh"],
"_ONLY_THETA": gammas["selected_theta"],
}
# binnings for the irfs
true_energy_bins = add_overflow_bins(
create_bins_per_decade(10**-1.9 * u.TeV, 10**2.31 * u.TeV, 10))
reco_energy_bins = add_overflow_bins(
create_bins_per_decade(10**-1.9 * u.TeV, 10**2.31 * u.TeV, 5))
fov_offset_bins = [0, 0.5] * u.deg
source_offset_bins = np.arange(0, 1 + 1e-4, 1e-3) * u.deg
energy_migration_bins = np.geomspace(0.2, 5, 200)
for label, mask in masks.items():
effective_area = effective_area_per_energy(
gammas[mask],
particles["gamma"]["simulation_info"],
true_energy_bins=true_energy_bins,
)
hdus.append(
create_aeff2d_hdu(
effective_area[...,
np.newaxis], # add one dimension for FOV offset
true_energy_bins,
fov_offset_bins,
extname="EFFECTIVE_AREA" + label,
))
edisp = energy_dispersion(
gammas[mask],
true_energy_bins=true_energy_bins,
fov_offset_bins=fov_offset_bins,
migration_bins=energy_migration_bins,
)
hdus.append(
create_energy_dispersion_hdu(
edisp,
true_energy_bins=true_energy_bins,
migration_bins=energy_migration_bins,
fov_offset_bins=fov_offset_bins,
extname="ENERGY_DISPERSION" + label,
))
bias_resolution = energy_bias_resolution(gammas[gammas["selected"]],
reco_energy_bins,
energy_type="reco")
ang_res = angular_resolution(gammas[gammas["selected_gh"]],
reco_energy_bins,
energy_type="reco")
psf = psf_table(
gammas[gammas["selected_gh"]],
true_energy_bins,
fov_offset_bins=fov_offset_bins,
source_offset_bins=source_offset_bins,
)
background_rate = background_2d(
background[background['selected_gh']],
reco_energy_bins,
fov_offset_bins=np.arange(0, 11) * u.deg,
t_obs=T_OBS,
)
hdus.append(
create_background_2d_hdu(
background_rate,
reco_energy_bins,
fov_offset_bins=np.arange(0, 11) * u.deg,
))
hdus.append(
create_psf_table_hdu(
psf,
true_energy_bins,
source_offset_bins,
fov_offset_bins,
))
hdus.append(
create_rad_max_hdu(theta_cuts["cut"][:, np.newaxis], theta_bins,
fov_offset_bins))
hdus.append(fits.BinTableHDU(ang_res, name="ANGULAR_RESOLUTION"))
hdus.append(
fits.BinTableHDU(bias_resolution, name="ENERGY_BIAS_RESOLUTION"))
log.info('Writing outputfile')
fits.HDUList(hdus).writeto("pyirf_eventdisplay.fits.gz", overwrite=True)
def main(gammafile, protonfile, electronfile, outputfile):
logging.basicConfig(level=logging.INFO)
logging.getLogger("pyirf").setLevel(logging.DEBUG)
particles = {
"gamma": {
"file": gammafile,
"target_spectrum": CRAB_HEGRA,
},
"proton": {
"file": protonfile,
"target_spectrum": IRFDOC_PROTON_SPECTRUM,
},
"electron": {
"file": electronfile,
"target_spectrum": IRFDOC_ELECTRON_SPECTRUM,
},
}
for particle_type, p in particles.items():
log.info(f"Simulated {particle_type.title()} Events:")
p["events"], p["simulation_info"] = read_file(p["file"])
p["events"]["particle_type"] = particle_type
p["simulated_spectrum"] = PowerLaw.from_simulation(
p["simulation_info"], T_OBS)
p["events"]["weight"] = calculate_event_weights(
p["events"]["true_energy"], p["target_spectrum"],
p["simulated_spectrum"])
for prefix in ('true', 'reco'):
k = f"{prefix}_source_fov_offset"
p["events"][k] = calculate_source_fov_offset(p["events"],
prefix=prefix)
log.info(p["simulation_info"])
log.info("")
gammas = particles["gamma"]["events"]
background = table.vstack(
[particles["proton"]["events"], particles["electron"]["events"]])
# calculate theta / distance between reco and assuemd source position
gammas["theta"] = calculate_theta(
gammas,
assumed_source_az=gammas["true_az"],
assumed_source_alt=gammas["true_alt"],
)
INITIAL_GH_CUT = np.quantile(gammas['gh_score'],
(1 - INITIAL_GH_CUT_EFFICENCY))
log.info(
f"Using fixed G/H cut of {INITIAL_GH_CUT} to calculate theta cuts")
theta_bins = add_overflow_bins(
create_bins_per_decade(10**-1.8 * u.TeV,
10**2.41 * u.TeV,
bins_per_decade=25))
sensitivity_bins = add_overflow_bins(
create_bins_per_decade(10**-1.8 * u.TeV,
10**2.41 * u.TeV,
bins_per_decade=5))
# theta cut is 68 percent containmente of the gammas
# for now with a fixed global, unoptimized score cut
mask_theta_cuts = gammas["gh_score"] >= INITIAL_GH_CUT
theta_cuts = calculate_percentile_cut(
gammas["theta"][mask_theta_cuts],
gammas["reco_energy"][mask_theta_cuts],
bins=theta_bins,
min_value=0.05 * u.deg,
fill_value=0.32 * u.deg,
max_value=0.32 * u.deg,
percentile=68,
)
log.info("Optimizing G/H separation cut for best sensitivity")
gh_cut_efficiencies = np.arange(
GH_CUT_EFFICIENCY_STEP,
MAX_GH_CUT_EFFICIENCY + GH_CUT_EFFICIENCY_STEP / 2,
GH_CUT_EFFICIENCY_STEP)
sensitivity_step_2, gh_cuts = optimize_gh_cut(
gammas,
background,
reco_energy_bins=sensitivity_bins,
gh_cut_efficiencies=gh_cut_efficiencies,
op=operator.ge,
theta_cuts=theta_cuts,
alpha=ALPHA,
background_radius=MAX_BG_RADIUS,
)
# now that we have the optimized gh cuts, we recalculate the theta
# cut as 68 percent containment on the events surviving these cuts.
log.info('Recalculating theta cut for optimized GH Cuts')
for tab in (gammas, background):
tab["selected_gh"] = evaluate_binned_cut(tab["gh_score"],
tab["reco_energy"], gh_cuts,
operator.ge)
theta_cuts_opt = calculate_percentile_cut(
gammas[gammas['selected_gh']]["theta"],
gammas[gammas['selected_gh']]["reco_energy"],
theta_bins,
percentile=68,
fill_value=0.32 * u.deg,
max_value=0.32 * u.deg,
min_value=0.05 * u.deg,
)
gammas["selected_theta"] = evaluate_binned_cut(gammas["theta"],
gammas["reco_energy"],
theta_cuts_opt, operator.le)
gammas["selected"] = gammas["selected_theta"] & gammas["selected_gh"]
# calculate sensitivity
signal_hist = create_histogram_table(gammas[gammas["selected"]],
bins=sensitivity_bins)
background_hist = estimate_background(
background[background["selected_gh"]],
reco_energy_bins=sensitivity_bins,
theta_cuts=theta_cuts_opt,
alpha=ALPHA,
background_radius=MAX_BG_RADIUS,
)
sensitivity = calculate_sensitivity(signal_hist,
background_hist,
alpha=ALPHA)
# scale relative sensitivity by Crab flux to get the flux sensitivity
spectrum = particles['gamma']['target_spectrum']
for s in (sensitivity_step_2, sensitivity):
s["flux_sensitivity"] = (s["relative_sensitivity"] *
spectrum(s['reco_energy_center']))
hdus = [
fits.PrimaryHDU(),
fits.BinTableHDU(sensitivity, name="SENSITIVITY"),
fits.BinTableHDU(sensitivity_step_2, name="SENSITIVITY_STEP_2"),
fits.BinTableHDU(theta_cuts, name="THETA_CUTS"),
fits.BinTableHDU(theta_cuts_opt, name="THETA_CUTS_OPT"),
fits.BinTableHDU(gh_cuts, name="GH_CUTS"),
]
# calculate sensitivity using unoptimised cuts
gammas["theta_unop"] = gammas["theta"].to_value(u.deg) <= np.sqrt(0.03)
gammas["gh_unop"] = gammas["gh_score"] > 0.85
theta_cut_unop = table.QTable()
theta_cut_unop['low'] = theta_cuts_opt['low']
theta_cut_unop['high'] = theta_cuts_opt['high']
theta_cut_unop['center'] = theta_cuts_opt['center']
theta_cut_unop['cut'] = np.sqrt(0.03) * u.deg
signal_hist_unop = create_histogram_table(gammas[gammas["theta_unop"]
& gammas["gh_unop"]],
bins=sensitivity_bins)
background_hist_unop = estimate_background(
background[background["gh_score"] > 0.85],
reco_energy_bins=sensitivity_bins,
theta_cuts=theta_cut_unop,
alpha=ALPHA,
background_radius=MAX_BG_RADIUS,
)
sensitivity_unop = calculate_sensitivity(signal_hist_unop,
background_hist_unop,
alpha=ALPHA)
sensitivity_unop["flux_sensitivity"] = (
sensitivity_unop["relative_sensitivity"] *
spectrum(sensitivity_unop['reco_energy_center']))
hdus.append(fits.BinTableHDU(sensitivity_unop, name="SENSITIVITY_UNOP"))
log.info('Calculating IRFs')
masks = {
"": gammas["selected"],
"_NO_CUTS": slice(None),
"_ONLY_GH": gammas["selected_gh"],
"_ONLY_THETA": gammas["selected_theta"],
}
# binnings for the irfs
true_energy_bins = add_overflow_bins(
create_bins_per_decade(10**-1.8 * u.TeV,
10**2.41 * u.TeV,
bins_per_decade=10))
reco_energy_bins = add_overflow_bins(
create_bins_per_decade(10**-1.8 * u.TeV,
10**2.41 * u.TeV,
bins_per_decade=5))
fov_offset_bins = [0, 0.5] * u.deg
source_offset_bins = np.arange(0, 1 + 1e-4, 1e-3) * u.deg
energy_migration_bins = np.geomspace(0.2, 5, 200)
for label, mask in masks.items():
effective_area = effective_area_per_energy(
gammas[mask],
particles["gamma"]["simulation_info"],
true_energy_bins=true_energy_bins,
)
hdus.append(
create_aeff2d_hdu(
effective_area[...,
np.newaxis], # add one dimension for FOV offset
true_energy_bins,
fov_offset_bins,
extname="EFFECTIVE_AREA" + label,
))
edisp = energy_dispersion(
gammas[mask],
true_energy_bins=true_energy_bins,
fov_offset_bins=fov_offset_bins,
migration_bins=energy_migration_bins,
)
hdus.append(
create_energy_dispersion_hdu(
edisp,
true_energy_bins=true_energy_bins,
migration_bins=energy_migration_bins,
fov_offset_bins=fov_offset_bins,
extname="ENERGY_DISPERSION" + label,
))
bias_resolution = energy_bias_resolution(
gammas[gammas["selected"]],
true_energy_bins,
)
ang_res = angular_resolution(
gammas[gammas["selected_gh"]],
true_energy_bins,
)
psf = psf_table(
gammas[gammas["selected_gh"]],
true_energy_bins,
fov_offset_bins=fov_offset_bins,
source_offset_bins=source_offset_bins,
)
background_rate = background_2d(
background[background['selected_gh']],
reco_energy_bins,
fov_offset_bins=np.arange(0, 11) * u.deg,
t_obs=T_OBS,
)
hdus.append(
create_background_2d_hdu(
background_rate,
reco_energy_bins,
fov_offset_bins=np.arange(0, 11) * u.deg,
))
hdus.append(
create_psf_table_hdu(
psf,
true_energy_bins,
source_offset_bins,
fov_offset_bins,
))
hdus.append(
create_rad_max_hdu(theta_cuts_opt["cut"][:, np.newaxis], theta_bins,
fov_offset_bins))
hdus.append(fits.BinTableHDU(ang_res, name="ANGULAR_RESOLUTION"))
hdus.append(
fits.BinTableHDU(bias_resolution, name="ENERGY_BIAS_RESOLUTION"))
log.info('Writing outputfile')
fits.HDUList(hdus).writeto(outputfile, overwrite=True)
