LightCurveEstimator¶
-
class
gammapy.time.
LightCurveEstimator
(spec_extract)[source]¶ Bases:
object
Light curve estimator.
For a usage example see light_curve.html.
Parameters: - spec_extract :
SpectrumExtraction
Contains statistics, IRF and event lists
Methods Summary
compute_flux_point
(time_interval, …[, …])Compute one flux point for one time interval. light_curve
(time_intervals, spectral_model, …)Compute light curve. make_time_intervals_fixes
(time_step, …)Create time intervals of fixed size. make_time_intervals_min_significance
(…[, …])Create time intervals such that each bin of a light curve reach a given significance Methods Documentation
-
compute_flux_point
(time_interval, spectral_model, energy_range, ul_significance=3)[source]¶ Compute one flux point for one time interval.
Parameters: - time_interval :
Time
Time interval (2-element array, or a tuple of Time objects)
- spectral_model :
SpectralModel
Spectral model
- energy_range :
Quantity
True energy range to evaluate integrated flux (true energy)
- ul_significance : float
Upper limit confidence level significance
Returns: - useinterval : bool
Is True if the time_interval produce a valid flux point
- measurements : dict
Dictionary with flux point measurement in the time interval
- time_interval :
-
light_curve
(time_intervals, spectral_model, energy_range, ul_significance=3)[source]¶ Compute light curve.
Implementation follows what is done in: http://adsabs.harvard.edu/abs/2010A%26A…520A..83H.
To be discussed: assumption that threshold energy in the same in reco and true energy.
Parameters: - time_intervals : list of
Time
List of time intervals
- spectral_model :
SpectralModel
Spectral model
- energy_range :
Quantity
True energy range to evaluate integrated flux (true energy)
- ul_significance : float
Upper limit confidence level significance
Returns: - lc :
LightCurve
Light curve
- time_intervals : list of
-
static
make_time_intervals_fixes
(time_step, spectrum_extraction)[source]¶ Create time intervals of fixed size.
Parameters: - time_step : float
Size of the light curve bins in seconds
- spectrum_extraction :
SpectrumExtraction
Contains statistics, IRF and event lists
Returns: - table :
Table
Table of time intervals
Examples
To extract intervals for light curve:
intervals = list(zip(table['t_start'], table['t_stop']))
-
make_time_intervals_min_significance
(significance, significance_method, energy_range, spectrum_extraction, separators=None)[source]¶ Create time intervals such that each bin of a light curve reach a given significance
The function work event by event to create an interval containing enough statistic and then starting a new one
Parameters: - significance : float
Target significance for each light curve point
- significance_method : {‘lima’, ‘simple’}
Significance method (see
significance_on_off
)- energy_range :
Quantity
True energy range to evaluate integrated flux (true energy)
- spectrum_extraction :
SpectrumExtraction
Contains statistics, IRF and event lists
- separators : list of
Time
Contains a list of time to stop the current point creation (not saved) and start a new one Mostly useful between observations separated by a large time gap
Returns: - table :
Table
Table of time intervals and information about their content : on/off events, alpha, significance
Examples
- extract intervals for light curve :
- intervals = list(zip(table[‘t_start’], table[‘t_stop’]))
- spec_extract :