SourceCatalogObject3FGL#

class gammapy.catalog.SourceCatalogObject3FGL(data, data_extended=None)[source]#

Bases: gammapy.catalog.fermi.SourceCatalogObjectFermiBase

One source from the Fermi-LAT 3FGL catalog.

Catalog is represented by SourceCatalog3FGL.

Attributes Summary

asso

energy_range

Energy range used for the catalog.

flux_points

Flux points (FluxPoints).

flux_points_meta

flux_points_table

Flux points (Table).

is_pointlike

name

Source name (str)

position

Source position (SkyCoord).

row_index

Row index of source in catalog (int)

Methods Summary

info([info])

Summary info string.

lightcurve()

Lightcurve (FluxPoints).

sky_model([name])

Sky model (SkyModel).

spatial_model()

Spatial model (SpatialModel).

spectral_model()

Best fit spectral model (SpectralModel).

Attributes Documentation

asso = ['ASSOC1', 'ASSOC2', 'ASSOC_TEV', 'ASSOC_GAM1', 'ASSOC_GAM2', 'ASSOC_GAM3']#
energy_range = <Quantity [   100., 100000.] MeV>#

Energy range used for the catalog.

Paper says that analysis uses data up to 300 GeV, but results are all quoted up to 100 GeV only to be consistent with previous catalogs.

flux_points#

Flux points (FluxPoints).

flux_points_meta = {'n_sigma': 1, 'n_sigma_ul': 2, 'sed_type_init': 'flux', 'sqrt_ts_threshold_ul': 1}#
flux_points_table#

Flux points (Table).

is_pointlike#
name#

Source name (str)

position#

Source position (SkyCoord).

row_index#

Row index of source in catalog (int)

Methods Documentation

info(info='all')#

Summary info string.

Parameters
info{‘all’, ‘basic’, ‘more’, ‘position’, ‘spectral’,’lightcurve’}

Comma separated list of options

lightcurve()[source]#

Lightcurve (FluxPoints).

sky_model(name=None)#

Sky model (SkyModel).

spatial_model()[source]#

Spatial model (SpatialModel).

spectral_model()[source]#

Best fit spectral model (SpectralModel).