EventList¶

class gammapy.data.EventList(table)[source]¶

Bases: gammapy.data.EventListBase

Event list for IACT dataset.

Data format specification: EVENTS

For further information, see the base class: EventListBase.

Parameters

tableTable: Event list table

Examples

To load an example H.E.S.S. event list:

>>> from gammapy.data import EventList
>>> filename = '$GAMMAPY_DATA/hess-dl3-dr1/data/hess_dl3_dr1_obs_id_023523.fits.gz'
>>> events = EventList.read(filename)

Attributes Summary

`altaz`	ALT / AZ position computed from RA / DEC (`SkyCoord`).
`altaz_frame`	ALT / AZ frame (`AltAz`).
`altaz_from_table`	ALT / AZ position from table (`SkyCoord`).
`energy`	Event energies (`Quantity`).
`galactic`	Event Galactic sky coordinates (`SkyCoord`).
`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`).
`observation_time_end`	Observation stop time (`Time`).
`observation_time_start`	Observation start time (`Time`).
`observatory_earth_location`	Observatory location (`EarthLocation`).
`offset`	Event offset from the array pointing position (`Angle`).
`pointing_radec`	Pointing RA / DEC sky coordinates (`SkyCoord`).
`radec`	Event RA / DEC sky coordinates (`SkyCoord`).
`time`	Event times (`Time`).
`time_ref`	Time reference (`Time`).

Methods Summary

`check`(self[, checks])	Run checks.
`map_coord`(self, geom)	Event map coordinates for a given geometry.
`peek`(self)	Quick look plots.
`plot_energy`(self[, ax, ebounds])	Plot counts as a function of energy.
`plot_energy_offset`(self[, ax])	Plot counts histogram with energy and offset axes.
`plot_image`(self)	Quick look counts map sky plot.
`plot_offset2_distribution`(self[, ax, center])	Plot offset^2 distribution of the events.
`plot_time`(self[, ax])	Plots an event rate time curve.
`read`(filename, \\kwargs)	Read from FITS file.
`select_energy`(self, energy_band)	Select events in energy band.
`select_map_mask`(self, mask)	Select events inside a mask (`EventList`).
`select_offset`(self, offset_band)	Select events in offset band.
`select_parameter`(self, parameter, band)	Select events with respect to a specified parameter.
`select_region`(self, region[, wcs])	Select events in given region.
`select_row_subset`(self, row_specifier)	Select table row subset.
`select_time`(self, time_interval)	Select events in time interval.
`stack`(event_lists, \\kwargs)	Stack (concatenate) list of event lists.

Attributes Documentation

altaz¶: ALT / AZ position computed from RA / DEC (SkyCoord).

altaz_frame¶: ALT / AZ frame (AltAz).

altaz_from_table¶: ALT / AZ position from table (SkyCoord).

energy¶: Event energies (Quantity).

galactic¶

Event Galactic sky coordinates (SkyCoord).

Always computed from RA / DEC using Astropy.

observation_dead_time_fraction¶

Dead-time fraction (float).

This is a keyword related to IACTs Defined as dead-time over observation time.

Dead-time is defined as the time during the observation where the detector didn’t record events: http://en.wikipedia.org/wiki/Dead_time https://ui.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.

observation_live_time_duration¶

Live-time duration in seconds (Quantity).

The dead-time-corrected observation time.

In Fermi-LAT it is automatically provided in the header of the event list.
In IACTs is computed as t_live = t_observation * (1 - f_dead)

where f_dead is the dead-time fraction.

observation_time_duration¶

Observation time duration in seconds (Quantity).

This is a keyword related to IACTs The wall time, including dead-time.

observation_time_end¶: Observation stop time (Time).

observation_time_start¶: Observation start time (Time).

observatory_earth_location¶: Observatory location (EarthLocation).

offset¶: Event offset from the array pointing position (Angle).

pointing_radec¶: Pointing RA / DEC sky coordinates (SkyCoord).

radec¶: Event RA / DEC sky coordinates (SkyCoord).

time¶

Event times (Time).

Notes

Times are automatically converted to 64-bit floats. With 32-bit floats times will be incorrect by a few seconds when e.g. adding them to the reference time.

time_ref¶: Time reference (Time).

Methods Documentation

check(self, checks='all')¶

Run checks.

This is a generator that yields a list of dicts.

map_coord(self, geom)¶

Event map coordinates for a given geometry.

Parameters

geomGeom: Geometry

Returns

coordMapCoord: Coordinates

peek(self)[source]¶: Quick look plots.

plot_energy(self, ax=None, ebounds=None, **kwargs)¶: Plot counts as a function of energy.

plot_energy_offset(self, ax=None)¶: Plot counts histogram with energy and offset axes.

plot_image(self)[source]¶: Quick look counts map sky plot.

plot_offset2_distribution(self, ax=None, center=None, **kwargs)¶

Plot offset^2 distribution of the events.

The distribution shown in this plot is for this quantity:

offset = center.separation(events.radec).deg
offset2 = offset ** 2

Note that this method is just for a quicklook plot.

If you want to do computations with the offset or offset^2 values, you can use the line above. As an example, here’s how to compute the 68% event containment radius using numpy.percentile:

import numpy as np
r68 = np.percentile(offset, q=68)

Parameters

axAxes (optional): Axes
centerastropy.coordinates.SkyCoord: Center position for the offset^2 distribution. Default is the observation pointing position.
**kwargs :: Extra keyword arguments are passed to matplotlib.pyplot.hist.

Returns

axAxes: Axes

Examples

Load an example event list:

>>> from gammapy.data import EventList
>>> events = EventList.read('$GAMMAPY_DATA/hess-dl3-dr1/data/hess_dl3_dr1_obs_id_023523.fits.gz')

Plot the offset^2 distribution wrt. the observation pointing position (this is a commonly used plot to check the background spatial distribution):

>>> events.plot_offset2_distribution()

Plot the offset^2 distribution wrt. the Crab pulsar position (this is commonly used to check both the gamma-ray signal and the background spatial distribution):

>>> import numpy as np
>>> from astropy.coordinates import SkyCoord
>>> center = SkyCoord(83.63307, 22.01449, unit='deg')
>>> bins = np.linspace(start=0, stop=0.3 ** 2, num=30)
>>> events.plot_offset2_distribution(center=center, bins=bins)

Note how we passed the bins option of matplotlib.pyplot.hist to control the histogram binning, in this case 30 bins ranging from 0 to (0.3 deg)^2.

plot_time(self, ax=None)¶

Plots an event rate time curve.

Parameters

axAxes or None: Axes

Returns

axAxes: Axes

classmethod read(filename, **kwargs)¶

Read from FITS file.

Format specification: EVENTS

Parameters

filenamepathlib.Path, str: Filename

select_energy(self, energy_band)¶

Select events in energy band.

Parameters

energy_bandQuantity: Energy band [energy_min, energy_max)

Returns

event_listEventList: Copy of event list with selection applied.

Examples

>>> from astropy.units import Quantity
>>> from gammapy.data import EventList
>>> event_list = EventList.read('events.fits')
>>> energy_band = Quantity([1, 20], 'TeV')
>>> event_list = event_list.select_energy()

select_map_mask(self, mask)¶

Select events inside a mask (EventList).

Parameters

maskMap: Mask

select_offset(self, offset_band)[source]¶

Select events in offset band.

Parameters

offset_bandAngle: offset band [offset_min, offset_max)

Returns

event_listEventList: Copy of event list with selection applied.

select_parameter(self, parameter, band)¶

Select events with respect to a specified parameter.

Parameters

parameterstr: Parameter used for the selection. Must be present in self.table.
bandtuple or astropy.units.Quantity: Min and max value for the parameter to be selected (min <= parameter < max). If parameter is not dimensionless you have to provide a Quantity.

Returns

event_listEventList: Copy of event list with selection applied.

Examples

>>> from gammapy.data import EventList
>>> event_list = EventList.read('events.fits')
>>> phase_region = (0.3, 0.5)
>>> event_list = event_list.select_parameter(parameter='PHASE', band=phase_region)

select_region(self, region, wcs=None)¶

Select events in given region.

Parameters

regionSkyRegion or str: Sky region or string defining a sky region
wcsWCS: World coordinate system transformation

Returns

event_listEventList: Copy of event list with selection applied.

select_row_subset(self, row_specifier)¶

Select table row subset.

Parameters

row_specifierslice, int, or array of ints: Specification for rows to select, passed on to self.table[row_specifier].

Returns

event_listEventList: New event list with table row subset selected

Examples

Use a boolean mask as row_specifier:

mask = events.table[‘FOO’] > 42 events2 = events.select_row_subset(mask)

Use row index array as row_specifier:

idx = np.where(events.table[‘FOO’] > 42)[0] events2 = events.select_row_subset(idx)

select_time(self, time_interval)¶

Select events in time interval.

Parameters

time_intervalastropy.time.Time: Start time (inclusive) and stop time (exclusive) for the selection.

Returns

eventsEventList: Copy of event list with selection applied.

classmethod stack(event_lists, **kwargs)¶

Stack (concatenate) list of event lists.

Calls vstack.

Parameters

event_listslist: list of EventList to stack