DataStoreObservation¶
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class
gammapy.data.
DataStoreObservation
(obs_id, data_store)[source]¶ Bases:
object
IACT data store observation.
See Data Store
Parameters: obs_id : int
Observation ID
data_store :
DataStore
Data store
Attributes Summary
aeff
Load effective area object (lazy property). bkg
Load background object (lazy property). edisp
Load energy dispersion object (lazy property). events
Load gammapy.data.EventList
object (lazy property).gti
Load gammapy.data.GTI
object (lazy property).muoneff
Observation muon efficiency. obs_info
Observation information ( OrderedDict
).observation_dead_time_fraction
Dead-time fraction (float). observation_live_time_duration
Live-time duration in seconds ( Quantity
).observation_time_duration
Observation time duration in seconds ( Quantity
).observatory_earth_location
Observatory location ( EarthLocation
).pointing_altaz
Pointing ALT / AZ sky coordinates ( SkyCoord
).pointing_radec
Pointing RA / DEC sky coordinates ( SkyCoord
).pointing_zen
Pointing zenith angle sky ( Quantity
).psf
Load point spread function object (lazy property). target_radec
Target RA / DEC sky coordinates ( SkyCoord
).tstart
Observation start time ( Time
).tstop
Observation stop time ( Time
).Methods Summary
check_observation
()Perform some basic sanity checks on this observation. load
([hdu_type, hdu_class])Load data file as appropriate object. location
([hdu_type, hdu_class])HDU location object. make_psf
(position[, energy, rad])Make energy-dependent PSF for a given source position. peek
()Quick-look plots in a few panels. Attributes Documentation
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aeff
¶ Load effective area object (lazy property).
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bkg
¶ Load background object (lazy property).
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edisp
¶ Load energy dispersion object (lazy property).
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events
¶ Load
gammapy.data.EventList
object (lazy property).
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gti
¶ Load
gammapy.data.GTI
object (lazy property).
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muoneff
¶ Observation muon efficiency.
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obs_info
¶ Observation information (
OrderedDict
).
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observation_dead_time_fraction
¶ Dead-time fraction (float).
Defined as dead-time over observation time.
Dead-time is defined as the time during the observation where the detector didn’t record events: https://en.wikipedia.org/wiki/Dead_time https://adsabs.harvard.edu/abs/2004APh….22..285F
The dead-time fraction is used in the live-time computation, which in turn is used in the exposure and flux computation.
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observation_live_time_duration
¶ Live-time duration in seconds (
Quantity
).The dead-time-corrected observation time.
Computed as
t_live = t_observation * (1 - f_dead)
wheref_dead
is the dead-time fraction.
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observation_time_duration
¶ Observation time duration in seconds (
Quantity
).The wall time, including dead-time.
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observatory_earth_location
¶ Observatory location (
EarthLocation
).
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psf
¶ Load point spread function object (lazy property).
Methods Documentation
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check_observation
()[source]¶ Perform some basic sanity checks on this observation.
Returns: results : list
List with failure messages for the checks that failed
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load
(hdu_type=None, hdu_class=None)[source]¶ Load data file as appropriate object.
Parameters: hdu_type : str
HDU type (see
VALID_HDU_TYPE
)hdu_class : str
HDU class (see
VALID_HDU_CLASS
)Returns: object : object
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location
(hdu_type=None, hdu_class=None)[source]¶ HDU location object.
Parameters: hdu_type : str
HDU type (see
VALID_HDU_TYPE
)hdu_class : str
HDU class (see
VALID_HDU_CLASS
)Returns: location :
HDULocation
HDU location
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make_psf
(position, energy=None, rad=None)[source]¶ Make energy-dependent PSF for a given source position.
Parameters: position :
SkyCoord
Position at which to compute the PSF
energy :
Quantity
1-dim energy array for the output PSF. If none is given, the energy array of the PSF from the observation is used.
rad :
Angle
1-dim offset wrt source position array for the output PSF. If none is given, the offset array of the PSF from the observation is used.
Returns: psf :
EnergyDependentTablePSF
Energy dependent psf table
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