RadMax2D#

class gammapy.irf.RadMax2D(axes, data=0, unit='', is_pointlike=False, fov_alignment=FoVAlignment.RADEC, meta=None, interp_kwargs=None)[source]#

Bases: gammapy.irf.core.IRF

2D Rad Max table.

This is not directly a IRF component but is needed as additional information for point-like IRF components when an energy or field of view dependent directional cut has been applied.

Data format specification: RAD_MAX_2D

Parameters
energy_axisMapAxis

Reconstructed energy axis

offset_axisMapAxis

Field of view offset axis.

dataQuantity

Applied directional cut

metadict

Meta data

Attributes Summary

axes

MapAxes

data

default_interp_kwargs

default_unit

fov_alignment

Alignment of the field of view coordinate axes, see FoVAlignment

has_offset_axis

Whether the IRF explicitly depends on offset

is_fixed_rad_max

Returns True if rad_max axes are flat.

is_pointlike

Whether the IRF is pointlike of full containment.

quantity

Quantity

required_axes

tag

unit

Map unit (Unit)

Methods Summary

cumsum(axis_name)

Compute cumsum along a given axis

evaluate([method])

Evaluate IRF

from_hdulist(hdulist[, hdu, format])

Create from HDUList.

from_irf(irf)

Create a RadMax2D instance from another IRF component.

from_table(table[, format])

Read from Table.

integral(axis_name, **kwargs)

Compute integral along a given axis

integrate_log_log(axis_name, **kwargs)

Integrate along a given axis.

interp_missing_data(axis_name)

Interpolate missing data along a given axis

is_allclose(other[, rtol_axes, atol_axes])

Compare two data IRFs for equivalency

normalize(axis_name)

Normalise data in place along a given axis.

pad(pad_width, axis_name, **kwargs)

Pad irf along a given axis.

plot_rad_max_vs_energy([ax])

Plot rad max value against energy.

read(filename[, hdu, format])

Read from file.

to_hdulist([format])

to_table([format])

Convert to table

to_table_hdu([format])

Convert to BinTableHDU.

to_unit(unit)

Convert irf to different unit

write(filename, *args, **kwargs)

Write IRF to fits.

Attributes Documentation

axes#

MapAxes

data#
default_interp_kwargs = {'bounds_error': False, 'fill_value': 0.0}#
default_unit = Unit("deg")#
fov_alignment#

Alignment of the field of view coordinate axes, see FoVAlignment

has_offset_axis#

Whether the IRF explicitly depends on offset

is_fixed_rad_max#

Returns True if rad_max axes are flat.

is_pointlike#

Whether the IRF is pointlike of full containment.

quantity#

Quantity

required_axes = ['energy', 'offset']#
tag = 'rad_max_2d'#
unit#

Map unit (Unit)

Methods Documentation

cumsum(axis_name)#

Compute cumsum along a given axis

Parameters
axis_namestr

Along which axis to integrate.

Returns
irfIRF

Cumsum IRF

evaluate(method=None, **kwargs)#

Evaluate IRF

Parameters
**kwargsdict

Coordinates at which to evaluate the IRF

methodstr {‘linear’, ‘nearest’}, optional

Interpolation method

Returns
arrayQuantity

Interpolated values

classmethod from_hdulist(hdulist, hdu=None, format='gadf-dl3')#

Create from HDUList.

Parameters
hdulistHDUList

HDU list

hdustr

HDU name

format{“gadf-dl3”}

Format specification

Returns
irfIRF

IRF class

classmethod from_irf(irf)[source]#

Create a RadMax2D instance from another IRF component.

This reads the RAD_MAX metadata keyword from the irf and creates a RadMax2D with a single bin in energy and offset using the ranges from the input irf.

Parameters
irf: `~gammapy.irf.EffectiveAreaTable2D` or `~gammapy.irf.EnergyDispersion2D`

IRF instance from which to read the RAD_MAX and limit information

Returns
rad_max: RadMax2D

RadMax2D object with a single bin corresponding to the fixed RAD_MAX cut.

Notes

This assumes the true energy axis limits are also valid for the reco energy limits.

classmethod from_table(table, format='gadf-dl3')#

Read from Table.

Parameters
tableTable

Table with irf data

format{“gadf-dl3”}

Format specification

Returns
irfIRF

IRF class.

integral(axis_name, **kwargs)#

Compute integral along a given axis

This method uses interpolation of the cumulative sum.

Parameters
axis_namestr

Along which axis to integrate.

**kwargsdict

Coordinates at which to evaluate the IRF

Returns
arrayQuantity

Returns 2D array with axes offset

integrate_log_log(axis_name, **kwargs)#

Integrate along a given axis.

This method uses log-log trapezoidal integration.

Parameters
axis_namestr

Along which axis to integrate.

**kwargsdict

Coordinates at which to evaluate the IRF

Returns
arrayQuantity

Returns 2D array with axes offset

interp_missing_data(axis_name)#

Interpolate missing data along a given axis

is_allclose(other, rtol_axes=0.001, atol_axes=1e-06, **kwargs)#

Compare two data IRFs for equivalency

Parameters
othergammapy.irfs.IRF

The irf to compare against

rtol_axesfloat

Relative tolerance for the axes comparison.

atol_axesfloat

Relative tolerance for the axes comparison.

**kwargsdict

keywords passed to numpy.allclose

Returns
is_allclosebool

Whether the IRF is all close.

normalize(axis_name)#

Normalise data in place along a given axis.

Parameters
axis_namestr

Along which axis to normalize.

pad(pad_width, axis_name, **kwargs)#

Pad irf along a given axis.

Parameters
pad_width{sequence, array_like, int}

Number of pixels padded to the edges of each axis.

axis_namestr

Which axis to downsample. By default spatial axes are padded.

**kwargsdict

Keyword argument forwarded to pad

Returns
irfIRF

Padded irf

plot_rad_max_vs_energy(ax=None, **kwargs)[source]#

Plot rad max value against energy.

Parameters
axAxes

Axes to plot on.

**kwargsdict

Keyword arguments passed to pcolormesh

Returns
axAxes

Axes to plot on.

classmethod read(filename, hdu=None, format='gadf-dl3')#

Read from file.

Parameters
filenamestr or Path

Filename

hdustr

HDU name

format{“gadf-dl3”}

Format specification

Returns
irfIRF

IRF class

to_hdulist(format='gadf-dl3')#
to_table(format='gadf-dl3')#

Convert to table

Parameters
format{“gadf-dl3”}

Format specification

Returns
tableTable

IRF data table

to_table_hdu(format='gadf-dl3')#

Convert to BinTableHDU.

Parameters
format{“gadf-dl3”}

Format specification

Returns
hduBinTableHDU

IRF data table hdu

to_unit(unit)#

Convert irf to different unit

Parameters
unitUnit or str

New unit

Returns
irfIRF

IRF with new unit and converted data

write(filename, *args, **kwargs)#

Write IRF to fits.

Calls writeto, forwarding all arguments.