DataStoreObservation¶
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class
gammapy.data.DataStoreObservation(obs_id, data_store)[source]¶ Bases:
objectIACT data store observation.
See Data Store
Parameters: obs_id : int
Observation ID
data_store :
DataStoreData store
Attributes Summary
aeffLoad effective area object (lazy property). bkgLoad background object (lazy property). edispLoad energy dispersion object (lazy property). eventsLoad gammapy.data.EventListobject (lazy property).gtiLoad gammapy.data.GTIobject (lazy property).muoneffObservation muon efficiency. obs_infoObservation information ( OrderedDict).observation_dead_time_fractionDead-time fraction (float). observation_live_time_durationLive-time duration in seconds ( Quantity).observation_time_durationObservation time duration in seconds ( Quantity).observatory_earth_locationObservatory location ( EarthLocation).pointing_altazPointing ALT / AZ sky coordinates ( SkyCoord).pointing_radecPointing RA / DEC sky coordinates ( SkyCoord).pointing_zenPointing zenith angle sky ( Quantity).psfLoad point spread function object (lazy property). target_radecTarget RA / DEC sky coordinates ( SkyCoord).tstartObservation start time ( Time).tstopObservation 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.EventListobject (lazy property).
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gti¶ Load
gammapy.data.GTIobject (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_deadis 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 :
HDULocationHDU location
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make_psf(position, energy=None, rad=None)[source]¶ Make energy-dependent PSF for a given source position.
Parameters: position :
SkyCoordPosition at which to compute the PSF
energy :
Quantity1-dim energy array for the output PSF. If none is given, the energy array of the PSF from the observation is used.
rad :
Angle1-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 :
EnergyDependentTablePSFEnergy dependent psf table
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