Source code for gammapy.modeling.models.spatial

# Licensed under a 3-clause BSD style license - see LICENSE.rst
"""Spatial models."""
import logging
import os
import numpy as np
import scipy.integrate
import scipy.special
import astropy.units as u
from astropy.coordinates import Angle, SkyCoord
from astropy.coordinates.angle_utilities import angular_separation, position_angle
from astropy.utils import lazyproperty
from regions import (
    CircleAnnulusSkyRegion,
    CircleSkyRegion,
    EllipseSkyRegion,
    PointSkyRegion,
    RectangleSkyRegion,
)
import matplotlib.pyplot as plt
from gammapy.maps import Map, WcsGeom
from gammapy.modeling import Parameter
from gammapy.modeling.covariance import copy_covariance
from gammapy.utils.gauss import Gauss2DPDF
from gammapy.utils.scripts import make_path
from .core import ModelBase

__all__ = [
    "ConstantFluxSpatialModel",
    "ConstantSpatialModel",
    "DiskSpatialModel",
    "GaussianSpatialModel",
    "GeneralizedGaussianSpatialModel",
    "PointSpatialModel",
    "Shell2SpatialModel",
    "ShellSpatialModel",
    "SpatialModel",
    "TemplateSpatialModel",
]


log = logging.getLogger(__name__)

MAX_OVERSAMPLING = 200


def compute_sigma_eff(lon_0, lat_0, lon, lat, phi, major_axis, e):
    """Effective radius, used for the evaluation of elongated models"""
    phi_0 = position_angle(lon_0, lat_0, lon, lat)
    d_phi = phi - phi_0
    minor_axis = Angle(major_axis * np.sqrt(1 - e**2))

    a2 = (major_axis * np.sin(d_phi)) ** 2
    b2 = (minor_axis * np.cos(d_phi)) ** 2
    denominator = np.sqrt(a2 + b2)
    sigma_eff = major_axis * minor_axis / denominator
    return minor_axis, sigma_eff


[docs]class SpatialModel(ModelBase): """Spatial model base class.""" _type = "spatial" def __init__(self, **kwargs): frame = kwargs.pop("frame", "icrs") super().__init__(**kwargs) if not hasattr(self, "frame"): self.frame = frame
[docs] def __call__(self, lon, lat, energy=None): """Call evaluate method""" kwargs = {par.name: par.quantity for par in self.parameters} if energy is None and self.is_energy_dependent: raise ValueError("Missing energy value for evaluation") if energy is not None: kwargs["energy"] = energy return self.evaluate(lon, lat, **kwargs)
@property def evaluation_bin_size_min(self): return None # TODO: make this a hard-coded class attribute? @lazyproperty def is_energy_dependent(self): varnames = self.evaluate.__code__.co_varnames return "energy" in varnames @property def position(self): """Spatial model center position (`~astropy.coordinates.SkyCoord`)""" lon = self.lon_0.quantity lat = self.lat_0.quantity return SkyCoord(lon, lat, frame=self.frame) @position.setter def position(self, skycoord): """Spatial model center position""" coord = skycoord.transform_to(self.frame) self.lon_0.quantity = coord.data.lon self.lat_0.quantity = coord.data.lat @property def position_lonlat(self): """Spatial model center position `(lon, lat)` in rad and frame of the model""" lon = self.lon_0.quantity.to_value(u.rad) lat = self.lat_0.quantity.to_value(u.rad) return lon, lat # TODO: get rid of this! _phi_0 = 0.0 @property def phi_0(self): return self._phi_0 @phi_0.setter def phi_0(self, phi_0=0.0): self._phi_0 = phi_0 @property def position_error(self): """Get 95% containment position error as (`~regions.EllipseSkyRegion`)""" if self.covariance is None: raise ValueError("No position error information available.") pars = self.parameters sub_covar = self.covariance.get_subcovariance(["lon_0", "lat_0"]).data.copy() cos_lat = np.cos(self.lat_0.quantity.to_value("rad")) sub_covar[0, 0] *= cos_lat**2.0 sub_covar[0, 1] *= cos_lat sub_covar[1, 0] *= cos_lat eig_vals, eig_vecs = np.linalg.eig(sub_covar) lon_err, lat_err = np.sqrt(eig_vals) y_vec = eig_vecs[:, 0] phi = (np.arctan2(y_vec[1], y_vec[0]) * u.rad).to("deg") + self.phi_0 err = np.sort([lon_err, lat_err]) scale_r95 = Gauss2DPDF(sigma=1).containment_radius(0.95) err *= scale_r95 if err[1] == lon_err * scale_r95: phi += 90 * u.deg height = 2 * err[1] * pars["lon_0"].unit width = 2 * err[0] * pars["lat_0"].unit else: height = 2 * err[1] * pars["lat_0"].unit width = 2 * err[0] * pars["lon_0"].unit return EllipseSkyRegion( center=self.position, height=height, width=width, angle=phi )
[docs] def evaluate_geom(self, geom): """Evaluate model on `~gammapy.maps.Geom` Parameters ---------- geom : `~gammapy.maps.WcsGeom` Returns ------- `~gammapy.maps.Map` """ coords = geom.get_coord(frame=self.frame, sparse=True) if self.is_energy_dependent: return self(coords.lon, coords.lat, energy=coords["energy_true"]) else: return self(coords.lon, coords.lat)
[docs] def integrate_geom(self, geom, oversampling_factor=None): """Integrate model on `~gammapy.maps.Geom` or `~gammapy.maps.RegionGeom`. Integration is performed by simple rectangle approximation, the pixel center model value is multiplied by the pixel solid angle. An oversampling factor can be used for precision. By default, this parameter is set to None and an oversampling factor is automatically estimated based on the model estimation maximal bin width. For a RegionGeom, the model is integrated on a tangent WCS projection in the region. Parameters ---------- geom : `~gammapy.maps.WcsGeom` or `~gammapy.maps.RegionGeom` The geom on which the integration is performed oversampling_factor : int or None The oversampling factor to use for integration. Default is None: the factor is estimated from the model minimimal bin size Returns ------- `~gammapy.maps.Map` or `gammapy.maps.RegionNDMap`, containing the integral value in each spatial bin. """ wcs_geom = geom mask = None if geom.is_region: wcs_geom = geom.to_wcs_geom().to_image() result = Map.from_geom(geom=wcs_geom) pix_scale = np.max(wcs_geom.pixel_scales.to_value("deg")) if oversampling_factor is None: if self.evaluation_bin_size_min is not None: res_scale = self.evaluation_bin_size_min.to_value("deg") if res_scale > 0: oversampling_factor = np.minimum( int(np.ceil(pix_scale / res_scale)), MAX_OVERSAMPLING ) else: oversampling_factor = MAX_OVERSAMPLING else: oversampling_factor = 1 if oversampling_factor > 1: if self.evaluation_radius is not None: # Is it still needed? width = 2 * np.maximum( self.evaluation_radius.to_value("deg"), pix_scale ) wcs_geom = wcs_geom.cutout(self.position, width) upsampled_geom = wcs_geom.upsample(oversampling_factor, axis_name=None) # assume the upsampled solid angles are approximately factor**2 smaller values = self.evaluate_geom(upsampled_geom) / oversampling_factor**2 upsampled = Map.from_geom(upsampled_geom, unit=values.unit) upsampled += values if geom.is_region: mask = geom.contains(upsampled_geom.get_coord()).astype("int") integrated = upsampled.downsample( oversampling_factor, preserve_counts=True, weights=mask ) # Finally stack result result._unit = integrated.unit result.stack(integrated) else: values = self.evaluate_geom(wcs_geom) result._unit = values.unit result += values result *= result.geom.solid_angle() if geom.is_region: mask = result.geom.region_mask([geom.region]) result = Map.from_geom( geom, data=np.sum(result.data[mask]), unit=result.unit ) return result
[docs] def to_dict(self, full_output=False): """Create dict for YAML serilisation""" data = super().to_dict(full_output) data["spatial"]["frame"] = self.frame data["spatial"]["parameters"] = data["spatial"].pop("parameters") return data
def _get_plot_map(self, geom): if self.evaluation_radius is None and geom is None: raise ValueError( f"{self.__class__.__name__} requires geom to be defined for plotting." ) if geom is None: width = 2 * max(self.evaluation_radius, 0.1 * u.deg) geom = WcsGeom.create( skydir=self.position, frame=self.frame, width=width, binsz=0.02 ) data = self.evaluate_geom(geom) return Map.from_geom(geom, data=data.value, unit=data.unit)
[docs] def plot(self, ax=None, geom=None, **kwargs): """Plot spatial model. Parameters ---------- ax : `~matplotlib.axes.Axes`, optional Axis geom : `~gammapy.maps.WcsGeom`, optional Geom to use for plotting. **kwargs : dict Keyword arguments passed to `~gammapy.maps.WcsMap.plot()` Returns ------- ax : `~matplotlib.axes.Axes`, optional Axis """ m = self._get_plot_map(geom) if not m.geom.is_flat: raise TypeError( "Use .plot_interactive() or .plot_grid() for Map dimension > 2" ) return m.plot(ax=ax, **kwargs)
[docs] def plot_interative(self, ax=None, geom=None, **kwargs): """Plot spatial model. Parameters ---------- ax : `~matplotlib.axes.Axes`, optional Axis geom : `~gammapy.maps.WcsGeom`, optional Geom to use for plotting. **kwargs : dict Keyword arguments passed to `~gammapy.maps.WcsMap.plot()` Returns ------- ax : `~matplotlib.axes.Axes`, optional Axis """ m = self._get_plot_map(geom) if m.geom.is_image: raise TypeError("Use .plot() for 2D Maps") m.plot_interactive(ax=ax, **kwargs)
[docs] def plot_error(self, ax=None, **kwargs): """Plot position error Parameters ---------- ax : `~matplotlib.axes.Axes`, optional Axis **kwargs : dict Keyword arguments passed to `~gammapy.maps.WcsMap.plot()` Returns ------- ax : `~matplotlib.axes.Axes`, optional Axis """ # plot center position lon, lat = self.lon_0.value, self.lat_0.value ax = plt.gca() if ax is None else ax kwargs.setdefault("marker", "x") kwargs.setdefault("color", "red") kwargs.setdefault("label", "position") ax.scatter(lon, lat, transform=ax.get_transform(self.frame), **kwargs) # plot position error if not np.all(self.covariance.data == 0): region = self.position_error.to_pixel(ax.wcs) artist = region.as_artist(facecolor="none", edgecolor=kwargs["color"]) ax.add_artist(artist) return ax
[docs] def plot_grid(self, geom=None, **kwargs): """Plot spatial model energy slices in a grid. Parameters ---------- geom : `~gammapy.maps.WcsGeom`, optional Geom to use for plotting. **kwargs : dict Keyword arguments passed to `~gammapy.maps.WcsMap.plot()` Returns ------- ax : `~matplotlib.axes.Axes`, optional Axis """ if (geom is None) or geom.is_image: raise TypeError("Use .plot() for 2D Maps") m = self._get_plot_map(geom) m.plot_grid(**kwargs)
[docs] @classmethod def from_position(cls, position, **kwargs): """Define the position of the model using a sky coord Parameters ---------- position : `~astropy.coordinates.SkyCoord` Position Returns ------- model : `SpatialModel` Spatial model """ lon_0, lat_0 = position.data.lon, position.data.lat return cls(lon_0=lon_0, lat_0=lat_0, frame=position.frame, **kwargs)
@property def evaluation_radius(self): """Evaluation radius""" return None @property def evaluation_region(self): """Evaluation region""" if hasattr(self, "to_region"): return self.to_region() elif self.evaluation_radius is not None: return CircleSkyRegion( center=self.position, radius=self.evaluation_radius, ) else: return None
[docs]class PointSpatialModel(SpatialModel): r"""Point Source. For more information see :ref:`point-spatial-model`. Parameters ---------- lon_0, lat_0 : `~astropy.coordinates.Angle` Center position frame : {"icrs", "galactic"} Center position coordinate frame """ tag = ["PointSpatialModel", "point"] lon_0 = Parameter("lon_0", "0 deg") lat_0 = Parameter("lat_0", "0 deg", min=-90, max=90) is_energy_dependent = False @property def evaluation_bin_size_min(self): """Minimal evaluation bin size (`~astropy.coordinates.Angle`).""" return 0 * u.deg @property def evaluation_radius(self): """Evaluation radius (`~astropy.coordinates.Angle`). Set as zero degrees. """ return 0 * u.deg @staticmethod def _grid_weights(x, y, x0, y0): """Compute 4-pixel weights such that centroid is preserved.""" dx = np.abs(x - x0) dx = np.where(dx < 1, 1 - dx, 0) dy = np.abs(y - y0) dy = np.where(dy < 1, 1 - dy, 0) return dx * dy
[docs] def is_energy_dependent(self): return False
[docs] def evaluate_geom(self, geom): """Evaluate model on `~gammapy.maps.Geom`.""" values = self.integrate_geom(geom).data return values / geom.solid_angle()
[docs] def integrate_geom(self, geom, oversampling_factor=None): """Integrate model on `~gammapy.maps.Geom` Parameters ---------- geom : `Geom` Map geometry Returns ------- flux : `Map` Predicted flux map """ geom_image = geom.to_image() if geom.is_hpx: idx, weights = geom_image.interp_weights({"skycoord": self.position}) data = np.zeros(geom_image.data_shape) data[tuple(idx)] = weights else: x, y = geom_image.get_pix() x0, y0 = self.position.to_pixel(geom.wcs) data = self._grid_weights(x, y, x0, y0) return Map.from_geom(geom=geom_image, data=data, unit="")
[docs] def to_region(self, **kwargs): """Model outline (`~regions.PointSkyRegion`).""" return PointSkyRegion(center=self.position, **kwargs)
[docs]class GaussianSpatialModel(SpatialModel): r"""Two-dimensional Gaussian model. For more information see :ref:`gaussian-spatial-model`. Parameters ---------- lon_0, lat_0 : `~astropy.coordinates.Angle` Center position sigma : `~astropy.coordinates.Angle` Length of the major semiaxis of the Gaussian, in angular units. e : `float` Eccentricity of the Gaussian (:math:`0< e< 1`). phi : `~astropy.coordinates.Angle` Rotation angle :math:`\phi`: of the major semiaxis. Increases counter-clockwise from the North direction. frame : {"icrs", "galactic"} Center position coordinate frame """ tag = ["GaussianSpatialModel", "gauss"] lon_0 = Parameter("lon_0", "0 deg") lat_0 = Parameter("lat_0", "0 deg", min=-90, max=90) sigma = Parameter("sigma", "1 deg", min=0) e = Parameter("e", 0, min=0, max=1, frozen=True) phi = Parameter("phi", "0 deg", frozen=True) @property def evaluation_bin_size_min(self): """Minimal evaluation bin size (`~astropy.coordinates.Angle`) chosen as sigma/3.""" return self.parameters["sigma"].quantity / 3.0 @property def evaluation_radius(self): r"""Evaluation radius (`~astropy.coordinates.Angle`). Set as :math:`5\sigma`. """ return 5 * self.parameters["sigma"].quantity
[docs] @staticmethod def evaluate(lon, lat, lon_0, lat_0, sigma, e, phi): """Evaluate model.""" sep = angular_separation(lon, lat, lon_0, lat_0) if e == 0: a = 1.0 - np.cos(sigma) norm = (1 / (4 * np.pi * a * (1.0 - np.exp(-1.0 / a)))).value else: minor_axis, sigma_eff = compute_sigma_eff( lon_0, lat_0, lon, lat, phi, sigma, e ) a = 1.0 - np.cos(sigma_eff) norm = (1 / (2 * np.pi * sigma * minor_axis)).to_value("sr-1") exponent = -0.5 * ((1 - np.cos(sep)) / a) return u.Quantity(norm * np.exp(exponent).value, "sr-1", copy=False)
[docs] def to_region(self, x_sigma=1.5, **kwargs): r"""Model outline at a given number of :math:`\sigma`. Parameters ---------- x_sigma : float Number of :math:`\sigma Default is :math:`1.5\sigma` which corresponds to about 68% containment for a 2D symmetric Gaussian. Returns ------- region : `~regions.EllipseSkyRegion` Model outline. """ minor_axis = Angle(self.sigma.quantity * np.sqrt(1 - self.e.quantity**2)) return EllipseSkyRegion( center=self.position, height=2 * x_sigma * self.sigma.quantity, width=2 * x_sigma * minor_axis, angle=self.phi.quantity, **kwargs, )
@property def evaluation_region(self): """Evaluation region consistent with evaluation radius""" return self.to_region(x_sigma=5)
[docs]class GeneralizedGaussianSpatialModel(SpatialModel): r"""Two-dimensional Generealized Gaussian model. For more information see :ref:`generalized-gaussian-spatial-model`. Parameters ---------- lon_0, lat_0 : `~astropy.coordinates.Angle` Center position r_0 : `~astropy.coordinates.Angle` Length of the major semiaxis, in angular units. eta : `float` Shape parameter whitin (0, 1]. Special cases for disk: ->0, Gaussian: 0.5, Laplace:1 e : `float` Eccentricity (:math:`0< e< 1`). phi : `~astropy.coordinates.Angle` Rotation angle :math:`\phi`: of the major semiaxis. Increases counter-clockwise from the North direction. frame : {"icrs", "galactic"} Center position coordinate frame """ tag = ["GeneralizedGaussianSpatialModel", "gauss-general"] lon_0 = Parameter("lon_0", "0 deg") lat_0 = Parameter("lat_0", "0 deg", min=-90, max=90) r_0 = Parameter("r_0", "1 deg") eta = Parameter("eta", 0.5, min=0.01, max=1.0) e = Parameter("e", 0.0, min=0.0, max=1.0, frozen=True) phi = Parameter("phi", "0 deg", frozen=True)
[docs] @staticmethod def evaluate(lon, lat, lon_0, lat_0, r_0, eta, e, phi): sep = angular_separation(lon, lat, lon_0, lat_0) if isinstance(eta, u.Quantity): eta = eta.value # gamma function does not allow quantities minor_axis, r_eff = compute_sigma_eff(lon_0, lat_0, lon, lat, phi, r_0, e) z = sep / r_eff norm = 1 / (2 * np.pi * minor_axis * r_0 * eta * scipy.special.gamma(2 * eta)) return (norm * np.exp(-(z ** (1 / eta)))).to("sr-1")
@property def evaluation_bin_size_min(self): """Minimal evaluation bin size (`~astropy.coordinates.Angle`). The bin min size is defined as r_0/(3+8*eta)/(e+1). """ return self.r_0.quantity / (3 + 8 * self.eta.value) / (self.e.value + 1) @property def evaluation_radius(self): r"""Evaluation radius (`~astropy.coordinates.Angle`). The evaluation radius is defined as r_eval = r_0*(1+8*eta) so it verifies: r_eval -> r_0 if eta -> 0 r_eval = 5*r_0 > 5*sigma_gauss = 5*r_0/sqrt(2) ~ 3.5*r_0 if eta=0.5 r_eval = 9*r_0 > 5*sigma_laplace = 5*sqrt(2)*r_0 ~ 7*r_0 if eta = 1 r_eval -> inf if eta -> inf """ return self.r_0.quantity * (1 + 8 * self.eta.value)
[docs] def to_region(self, x_r_0=1, **kwargs): """Model outline at a given number of r_0. Parameters ---------- x_r_0 : float Number of r_0 (Default is 1). Returns ------- region : `~regions.EllipseSkyRegion` Model outline. """ minor_axis = Angle(self.r_0.quantity * np.sqrt(1 - self.e.quantity**2)) return EllipseSkyRegion( center=self.position, height=2 * x_r_0 * self.r_0.quantity, width=2 * x_r_0 * minor_axis, angle=self.phi.quantity, **kwargs, )
@property def evaluation_region(self): """Evaluation region consistent with evaluation radius""" scale = self.evaluation_radius / self.r_0.quantity return self.to_region(x_r_0=scale)
[docs]class DiskSpatialModel(SpatialModel): r"""Constant disk model. For more information see :ref:`disk-spatial-model`. Parameters ---------- lon_0, lat_0 : `~astropy.coordinates.Angle` Center position r_0 : `~astropy.coordinates.Angle` :math:`a`: length of the major semiaxis, in angular units. e : `float` Eccentricity of the ellipse (:math:`0< e< 1`). phi : `~astropy.coordinates.Angle` Rotation angle :math:`\phi`: of the major semiaxis. Increases counter-clockwise from the North direction. edge_width : float Width of the edge. The width is defined as the range within which the smooth edge of the model drops from 95% to 5% of its amplitude. It is given as fraction of r_0. frame : {"icrs", "galactic"} Center position coordinate frame """ tag = ["DiskSpatialModel", "disk"] lon_0 = Parameter("lon_0", "0 deg") lat_0 = Parameter("lat_0", "0 deg", min=-90, max=90) r_0 = Parameter("r_0", "1 deg", min=0) e = Parameter("e", 0, min=0, max=1, frozen=True) phi = Parameter("phi", "0 deg", frozen=True) edge_width = Parameter("edge_width", value=0.01, min=0, max=1, frozen=True) @property def evaluation_bin_size_min(self): """Minimal evaluation bin size (`~astropy.coordinates.Angle`). The bin min size is defined as r_0*(1-edge_width)/10. """ return self.r_0.quantity * (1 - self.edge_width.quantity) / 10.0 @property def evaluation_radius(self): """Evaluation radius (`~astropy.coordinates.Angle`). Set to the length of the semi-major axis plus the edge width. """ return 1.1 * self.r_0.quantity * (1 + self.edge_width.quantity) @staticmethod def _evaluate_norm_factor(r_0, e): """Compute the normalization factor.""" semi_minor = r_0 * np.sqrt(1 - e**2) def integral_fcn(x, a, b): A = 1 / np.sin(a) ** 2 B = 1 / np.sin(b) ** 2 C = A - B cs2 = np.cos(x) ** 2 return 1 - np.sqrt(1 - 1 / (B + C * cs2)) return ( 2 * scipy.integrate.quad( lambda x: integral_fcn(x, r_0, semi_minor), 0, np.pi )[0] ) ** -1 @staticmethod def _evaluate_smooth_edge(x, width): value = (x / width).to_value("") edge_width_95 = 2.326174307353347 return 0.5 * (1 - scipy.special.erf(value * edge_width_95))
[docs] @staticmethod def evaluate(lon, lat, lon_0, lat_0, r_0, e, phi, edge_width): """Evaluate model.""" sep = angular_separation(lon, lat, lon_0, lat_0) if e == 0: sigma_eff = r_0 else: sigma_eff = compute_sigma_eff(lon_0, lat_0, lon, lat, phi, r_0, e)[1] norm = DiskSpatialModel._evaluate_norm_factor(r_0, e) in_ellipse = DiskSpatialModel._evaluate_smooth_edge( sep - sigma_eff, sigma_eff * edge_width ) return u.Quantity(norm * in_ellipse, "sr-1", copy=False)
[docs] def to_region(self, **kwargs): """Model outline (`~regions.EllipseSkyRegion`).""" minor_axis = Angle(self.r_0.quantity * np.sqrt(1 - self.e.quantity**2)) return EllipseSkyRegion( center=self.position, height=2 * self.r_0.quantity, width=2 * minor_axis, angle=self.phi.quantity, **kwargs, )
[docs]class ShellSpatialModel(SpatialModel): r"""Shell model. For more information see :ref:`shell-spatial-model`. Parameters ---------- lon_0, lat_0 : `~astropy.coordinates.Angle` Center position radius : `~astropy.coordinates.Angle` Inner radius, :math:`r_{in}` width : `~astropy.coordinates.Angle` Shell width frame : {"icrs", "galactic"} Center position coordinate frame See Also -------- Shell2SpatialModel """ tag = ["ShellSpatialModel", "shell"] lon_0 = Parameter("lon_0", "0 deg") lat_0 = Parameter("lat_0", "0 deg", min=-90, max=90) radius = Parameter("radius", "1 deg") width = Parameter("width", "0.2 deg") @property def evaluation_bin_size_min(self): """Minimal evaluation bin size (`~astropy.coordinates.Angle`). The bin min size is defined as the shell width. """ return self.width.quantity @property def evaluation_radius(self): r"""Evaluation radius (`~astropy.coordinates.Angle`). Set to :math:`r_\text{out}`. """ return self.radius.quantity + self.width.quantity
[docs] @staticmethod def evaluate(lon, lat, lon_0, lat_0, radius, width): """Evaluate model.""" sep = angular_separation(lon, lat, lon_0, lat_0) radius_out = radius + width norm = 3 / (2 * np.pi * (radius_out**3 - radius**3)) with np.errstate(invalid="ignore"): # np.where and np.select do not work with quantities, so we use the # workaround with indexing value = np.sqrt(radius_out**2 - sep**2) mask = sep < radius value[mask] = (value - np.sqrt(radius**2 - sep**2))[mask] value[sep > radius_out] = 0 return norm * value
[docs] def to_region(self, **kwargs): """Model outline (`~regions.CircleAnnulusSkyRegion`).""" return CircleAnnulusSkyRegion( center=self.position, inner_radius=self.radius.quantity, outer_radius=self.radius.quantity + self.width.quantity, **kwargs, )
[docs]class Shell2SpatialModel(SpatialModel): r"""Shell model with outer radius and relative width parametrization For more information see :ref:`shell2-spatial-model`. Parameters ---------- lon_0, lat_0 : `~astropy.coordinates.Angle` Center position r_0 : `~astropy.coordinates.Angle` Outer radius, :math:`r_{out}` eta : float Shell width relative to outer radius, r_0, should be within (0,1] frame : {"icrs", "galactic"} Center position coordinate frame See Also -------- ShellSpatialModel """ tag = ["Shell2SpatialModel", "shell2"] lon_0 = Parameter("lon_0", "0 deg") lat_0 = Parameter("lat_0", "0 deg", min=-90, max=90) r_0 = Parameter("r_0", "1 deg") eta = Parameter("eta", 0.2, min=0.02, max=1) @property def evaluation_bin_size_min(self): """Minimal evaluation bin size (`~astropy.coordinates.Angle`). The bin min size is defined as r_0*eta. """ return self.eta.value * self.r_0.quantity @property def evaluation_radius(self): r"""Evaluation radius (`~astropy.coordinates.Angle`). Set to :math:`r_\text{out}`. """ return self.r_0.quantity @property def r_in(self): return (1 - self.eta.quantity) * self.r_0.quantity
[docs] @staticmethod def evaluate(lon, lat, lon_0, lat_0, r_0, eta): """Evaluate model.""" sep = angular_separation(lon, lat, lon_0, lat_0) r_in = (1 - eta) * r_0 norm = 3 / (2 * np.pi * (r_0**3 - r_in**3)) with np.errstate(invalid="ignore"): # np.where and np.select do not work with quantities, so we use the # workaround with indexing value = np.sqrt(r_0**2 - sep**2) mask = sep < r_in value[mask] = (value - np.sqrt(r_in**2 - sep**2))[mask] value[sep > r_0] = 0 return norm * value
[docs] def to_region(self, **kwargs): """Model outline (`~regions.CircleAnnulusSkyRegion`).""" return CircleAnnulusSkyRegion( center=self.position, inner_radius=self.r_in, outer_radius=self.r_0.quantity, **kwargs, )
[docs]class ConstantSpatialModel(SpatialModel): """Spatially constant (isotropic) spatial model. For more information see :ref:`constant-spatial-model`. Parameters ---------- value : `~astropy.units.Quantity` Value """ tag = ["ConstantSpatialModel", "const"] value = Parameter("value", "1 sr-1", frozen=True) frame = "icrs" evaluation_radius = None position = None
[docs] def to_dict(self, full_output=False): """Create dict for YAML serilisation""" # redefined to ignore frame attribute from parent class data = super().to_dict(full_output) data["spatial"].pop("frame") data["spatial"]["parameters"] = [] return data
[docs] @staticmethod def evaluate(lon, lat, value): """Evaluate model.""" return value
[docs] def to_region(self, **kwargs): """Model outline (`~regions.RectangleSkyRegion`).""" return RectangleSkyRegion( center=SkyCoord(0 * u.deg, 0 * u.deg, frame=self.frame), height=180 * u.deg, width=360 * u.deg, **kwargs, )
[docs]class ConstantFluxSpatialModel(SpatialModel): """Spatially constant flux spatial model. For more information see :ref:`constant-spatial-model`. """ tag = ["ConstantFluxSpatialModel", "const-flux"] frame = "icrs" evaluation_radius = None position = None
[docs] def to_dict(self, full_output=False): """Create dict for YAML serilisation""" # redefined to ignore frame attribute from parent class data = super().to_dict(full_output) data["spatial"].pop("frame") return data
[docs] @staticmethod def evaluate(lon, lat): """Evaluate model.""" return 1 / u.sr
[docs] @staticmethod def evaluate_geom(geom): """Evaluate model.""" return 1 / geom.solid_angle()
[docs] @staticmethod def integrate_geom(geom, oversampling_factor=None): """Evaluate model.""" return Map.from_geom(geom=geom, data=1)
[docs] def to_region(self, **kwargs): """Model outline (`~regions.RectangleSkyRegion`).""" return RectangleSkyRegion( center=SkyCoord(0 * u.deg, 0 * u.deg, frame=self.frame), height=180 * u.deg, width=360 * u.deg, **kwargs, )
[docs]class TemplateSpatialModel(SpatialModel): """Spatial sky map template model. For more information see :ref:`template-spatial-model`. Parameters ---------- map : `~gammapy.maps.Map` Map template. meta : dict, optional Meta information, meta['filename'] will be used for serialization normalize : bool Normalize the input map so that it integrates to unity. interp_kwargs : dict Interpolation keyword arguments passed to `gammapy.maps.Map.interp_by_coord`. Default arguments are {'method': 'linear', 'fill_value': 0, "values_scale": "log"}. Filename : str Name of the map file copy_data : bool Create a deepcopy of the map data or directly use the original. True by default, can be turned to False to save memory in case of large maps. """ tag = ["TemplateSpatialModel", "template"] def __init__( self, map, meta=None, normalize=True, interp_kwargs=None, filename=None, copy_data=True, ): if (map.data < 0).any(): log.warning("Map has negative values. Check and fix this!") if filename is not None: filename = str(make_path(filename)) self.normalize = normalize if normalize: # Normalize the diffuse map model so that it integrates to unity if map.geom.is_image: data_sum = map.data.sum() else: # Normalize in each energy bin data_sum = map.data.sum(axis=(1, 2)).reshape((-1, 1, 1)) data = map.data / data_sum data /= map.geom.solid_angle().to_value("sr") map = map.copy(data=data, unit="sr-1") if map.unit.is_equivalent(""): map = map.copy(data=map.data, unit="sr-1") log.warning("Missing spatial template unit, assuming sr^-1") if copy_data: self._map = map.copy() else: self._map = map.copy(data=map.data) self.meta = {} if meta is None else meta interp_kwargs = {} if interp_kwargs is None else interp_kwargs interp_kwargs.setdefault("method", "linear") interp_kwargs.setdefault("fill_value", 0) interp_kwargs.setdefault("values_scale", "log") self._interp_kwargs = interp_kwargs self.filename = filename super().__init__() @copy_covariance def copy(self, copy_data=False, **kwargs): """Copy model Parameters ---------- copy_data : bool Whether to copy the data. **kwargs : dict Keyword arguments forwarded to `TemplateSpatialModel` Returns ------- model : `TemplateSpatialModel` Copied template spatial model. """ kwargs.setdefault("map", self.map) kwargs.setdefault("meta", self.meta.copy()) kwargs.setdefault("normalize", self.normalize) kwargs.setdefault("interp_kwargs", self._interp_kwargs) kwargs.setdefault("filename", self.filename) return self.__class__(copy_data=copy_data, **kwargs) @property def map(self): """Template map (`~gammapy.maps.Map`)""" return self._map @property def is_energy_dependent(self): return "energy_true" in self.map.geom.axes.names @property def evaluation_radius(self): """Evaluation radius (`~astropy.coordinates.Angle`). Set to half of the maximal dimension of the map. """ return np.max(self.map.geom.width) / 2.0
[docs] @classmethod def read(cls, filename, normalize=True, **kwargs): """Read spatial template model from FITS image. If unit is not given in the FITS header the default is ``sr-1``. Parameters ---------- filename : str FITS image filename. normalize : bool Normalize the input map so that it integrates to unity. kwargs : dict Keyword arguments passed to `Map.read()`. """ m = Map.read(filename, **kwargs) return cls(m, normalize=normalize, filename=filename)
[docs] def evaluate(self, lon, lat, energy=None): """Evaluate the model at given coordinates. Note that, if the map data assume negative values, these are clipped to zero. """ coord = { "lon": lon.to_value("deg"), "lat": lat.to_value("deg"), } if energy is not None: coord["energy_true"] = energy val = self.map.interp_by_coord(coord, **self._interp_kwargs) val = np.clip(val, 0, a_max=None) return u.Quantity(val, self.map.unit, copy=False)
@property def position(self): """`~astropy.coordinates.SkyCoord`""" return self.map.geom.center_skydir @property def position_lonlat(self): """Spatial model center position `(lon, lat)` in rad and frame of the model""" lon = self.position.data.lon.rad lat = self.position.data.lat.rad return lon, lat @property def frame(self): return self.position.frame.name
[docs] @classmethod def from_dict(cls, data): data = data["spatial"] filename = data["filename"] normalize = data.get("normalize", True) m = Map.read(filename) return cls(m, normalize=normalize, filename=filename)
[docs] def to_dict(self, full_output=False): """Create dict for YAML serilisation""" data = super().to_dict(full_output) data["spatial"]["filename"] = self.filename data["spatial"]["normalize"] = self.normalize data["spatial"]["unit"] = str(self.map.unit) return data
[docs] def write(self, overwrite=False): if self.filename is None: raise IOError("Missing filename") elif os.path.isfile(self.filename) and not overwrite: log.warning("Template file already exits, and overwrite is False") else: self.map.write(self.filename, overwrite=overwrite)
[docs] def to_region(self, **kwargs): """Model outline from template map boundary (`~regions.RectangleSkyRegion`).""" return RectangleSkyRegion( center=self.map.geom.center_skydir, width=self.map.geom.width[0][0], height=self.map.geom.width[1][0], **kwargs, )
[docs] def plot(self, ax=None, geom=None, **kwargs): if geom is None: geom = self.map.geom super().plot(ax=ax, geom=geom, **kwargs)
[docs] def plot_interative(self, ax=None, geom=None, **kwargs): if geom is None: geom = self.map.geom super().plot_interative(ax=ax, geom=geom, **kwargs)