HillasReconstructor#
- class ctapipe.reco.hillas_reconstructor.HillasReconstructor(**kwargs: Any)[source]#
Bases:
HillasGeometryReconstructor
class that reconstructs the direction of an atmospheric shower using a simple hillas parametrisation of the camera images it provides a direction estimate in two steps and an estimate for the shower’s impact position on the ground.
so far, it does neither provide an energy estimator nor an uncertainty on the reconstructed parameters
Methods Summary
__call__
(event)Perform the full shower geometry reconstruction.
estimate_core_position
(array_pointing, psi, ...)Estimate the core position by intersection the major ellipse lines of each telescope.
estimate_direction
(norm, weight)calculates the origin of the gamma as the weighted average direction of the intersections of all hillas planes
estimate_relative_h_max
(cog_vectors, positions)Estimate the relative (to the observatory) vertical height of shower-max by intersecting the lines of the cog directions of each telescope.
initialize_arrays
(event, hillas_dict)Creates flat arrays of needed quantities from the event structure.
Methods Documentation
- __call__(event)[source]#
Perform the full shower geometry reconstruction.
- Parameters:
- event
ArrayEventContainer
The event, needs to have dl1 parameters. Will be filled with the corresponding dl2 containers, reconstructed stereo geometry and telescope-wise impact position.
- event
- static estimate_core_position(array_pointing, psi, positions)[source]#
Estimate the core position by intersection the major ellipse lines of each telescope.
- Parameters:
- hillas_dict: dict[HillasContainer]
dictionary of hillas moments
- array_pointing: SkyCoord[HorizonFrame]
Pointing direction of the array
- Returns:
- core_x: u.Quantity
estimated x position of impact
- core_y: u.Quantity
estimated y position of impact
Notes
The part of the algorithm taking into account divergent pointing mode and the usage of a corrected psi angle is explained in [Gas20] section 7.1.4.
- static estimate_direction(norm, weight)[source]#
calculates the origin of the gamma as the weighted average direction of the intersections of all hillas planes
- Returns:
- gammashape (3) numpy array
direction of origin of the reconstructed shower as a 3D vector
- crossingsshape (n,3) list
an error estimate
- static estimate_relative_h_max(cog_vectors, positions)[source]#
Estimate the relative (to the observatory) vertical height of shower-max by intersecting the lines of the cog directions of each telescope.
- Returns:
- astropy.unit.Quantity:
the estimated height above observatory level (not sea level) of the shower-max point
- initialize_arrays(event, hillas_dict)[source]#
Creates flat arrays of needed quantities from the event structure.
- Parameters:
- hillas_dictdictionary
dictionary of hillas moments
- subarrayctapipe.instrument.SubarrayDescription
subarray information
- telescopes_pointings: dictionary
dictionary of pointing direction per each telescope
- array_pointing: SkyCoord[AltAz]
pointing direction of the array
Notes
The part of the algorithm taking into account divergent pointing mode and the correction to the psi angle is explained in [Gas20], section 7.1.4.