コード例 #1
0
def run_benchmark():
    # Set up data store and select N_OBS times the observation OBS_ID
    data_store = DataStore.from_dir('$GAMMAPY_EXTRA/test_datasets/cta_1dc/')
    obs_ids = OBS_ID * np.ones(N_OBS)
    obs_list = data_store.obs_list(obs_id=obs_ids)

    target_position = SkyCoord(0, 0, unit='deg', frame='galactic')
    on_radius = 0.2 * u.deg
    on_region = CircleSkyRegion(center=target_position, radius=on_radius)

    bkg_estimator = RingBackgroundEstimator(
        r_in=0.5 * u.deg,
        width=0.2 * u.deg,
    )

    # Define reference image centered on the target
    xref = target_position.galactic.l.value
    yref = target_position.galactic.b.value

    ref_image = SkyImage.empty(
        nxpix=800,
        nypix=600,
        binsz=0.02,
        xref=xref,
        yref=yref,
        proj='TAN',
        coordsys='GAL',
    )

    exclusion_mask = ref_image.region_mask(on_region)
    exclusion_mask.data = 1 - exclusion_mask.data

    image_estimator = IACTBasicImageEstimator(
        reference=ref_image,
        emin=100 * u.GeV,
        emax=100 * u.TeV,
        offset_max=3 * u.deg,
        background_estimator=bkg_estimator,
        exclusion_mask=exclusion_mask,
    )
    result = image_estimator.run(obs_list)
コード例 #2
0
def run_benchmark():
    # Set up data store and select N_OBS times the observation OBS_ID
    data_store = DataStore.from_dir('$GAMMAPY_EXTRA/test_datasets/cta_1dc/')
    obs_ids = OBS_ID * np.ones(N_OBS)
    obs_list = data_store.obs_list(obs_id=obs_ids)

    target_position = SkyCoord(0, 0, unit='deg', frame='galactic')
    on_radius = 0.2 * u.deg
    on_region = CircleSkyRegion(center=target_position, radius=on_radius)

    bkg_estimator = RingBackgroundEstimator(
        r_in=0.5 * u.deg,
        width=0.2 * u.deg,
    )

    # Define reference image centered on the target
    xref = target_position.galactic.l.value
    yref = target_position.galactic.b.value

    ref_image = SkyImage.empty(
        nxpix=800, nypix=600, binsz=0.02,
        xref=xref, yref=yref,
        proj='TAN', coordsys='GAL',
    )

    exclusion_mask = ref_image.region_mask(on_region)
    exclusion_mask.data = 1 - exclusion_mask.data

    image_estimator = IACTBasicImageEstimator(
        reference=ref_image,
        emin=100 * u.GeV,
        emax=100 * u.TeV,
        offset_max=3 * u.deg,
        background_estimator=bkg_estimator,
        exclusion_mask=exclusion_mask,
    )
    result = image_estimator.run(obs_list)
コード例 #3
0
ファイル: geminga.py プロジェクト: ltostirepository/prova
exclusion_mask = ref_image.region_mask(on_region)
exclusion_mask.data = 1 - exclusion_mask.data
bkg_estimator = RingBackgroundEstimator(
    r_in=0.5 * u.deg,
    width=0.2 * u.deg,
)
image_estimator = IACTBasicImageEstimator(
    reference=ref_image,
    emin=100 * u.GeV,
    emax=100 * u.TeV,
    #offset_max=3 * u.deg,
    background_estimator=bkg_estimator,
    exclusion_mask=exclusion_mask,
)
images_new = image_estimator.run(obs_list)
print("\n\n\n")
print(images_new.names)
print(result2.names)
print("\n\n\n")
# Let's have a look at the background image and the exclusion mask

# This doesn't work yet ... need to do SkyImage.plot fixes:
# fig, axes = plt.subplots(nrows=1, ncols=3, figsize=(10, 3))
# background_image.plot(ax=axes[0])
# exclusion_image.plot(ax=axes[1])
# significance_image.plot(ax=axes[2])
print("bkg metodo 1")
background_image = result2['background']
background_image2 = images_new['background']
norm = simple_norm(background_image.data, stretch='sqrt', min_cut=0, max_cut=0.5)
コード例 #4
0
# In[12]:

bkg_estimator = RingBackgroundEstimator(
    r_in=0.5 * u.deg,
    width=0.2 * u.deg,
)
image_estimator = IACTBasicImageEstimator(
    reference=ref_image,
    emin=100 * u.GeV,
    emax=100 * u.TeV,
    offset_max=3 * u.deg,
    background_estimator=bkg_estimator,
    exclusion_mask=exclusion_mask,
)
images = image_estimator.run(obs_list)
images.names

# ### Show images
#
# Let's define a little helper function and then show all the resulting images that were computed.

# In[13]:


def show_image(image, radius=3, vmin=0, vmax=3):
    """Little helper function to show the images for this application here."""
    image.smooth(radius=radius).show(vmin=vmin, vmax=vmax, add_cbar=True)
    image.cutout(
        position=SkyCoord(0.5, 0, unit='deg', frame='galactic'),
        size=(2 * u.deg, 3 * u.deg),
コード例 #5
0
ファイル: LMC_image_all.py プロジェクト: AtreyeeS/LMC
exclusion_mask.plot(add_cbar=True)

bkg_estimator = FoVBackgroundEstimator()

emin = 0.5 * u.TeV
emax = 20 * u.TeV
offset_max = 2.3 * u.deg

image_estimator = IACTBasicImageEstimator(reference=ref_image,
                                          emin=emin,
                                          emax=emax,
                                          offset_max=offset_max,
                                          background_estimator=bkg_estimator,
                                          exclusion_mask=exclusion_mask)

comp_image = image_estimator.run(mylist)
comp_image.names

images = comp_image

print("Total number of counts", images[0].data.sum())
print("Total number of excess events", images[3].data.sum())

fermi = SkyImage.read("FDA16.fits")
fermi_rep = fermi.reproject(ref_image)

#Make sure that the exclusion mask properly excludes all sources

masked_excess = SkyImage.empty_like(images['excess'])
masked_excess.data = comp_image['excess'].data * exclusion_mask.data
masked_excess_cutout = masked_excess.cutout(position=SkyCoord(