Source code for photutils.profiles.core

# Licensed under a 3-clause BSD style license - see LICENSE.rst
"""
Base class for profiles.
"""

import abc
import warnings
from functools import cached_property

import astropy.units as u
import numpy as np
from astropy.utils.exceptions import AstropyUserWarning

from photutils.aperture.core import _update_method_subpixels_docstring
from photutils.aperture.photometry import AperturePhotometry
from photutils.utils._deprecation import deprecated_positional_kwargs
from photutils.utils._quantity_helpers import process_quantities
from photutils.utils._stats import nanmax, nansum

__all__ = ['ProfileBase']


[docs] @_update_method_subpixels_docstring class ProfileBase(metaclass=abc.ABCMeta): # numpydoc ignore: PR01,PR02,PR04,PR07 """ Abstract base class for profile classes. Parameters ---------- data : 2D `~numpy.ndarray` The 2D data array. The data should be background-subtracted. xycen : tuple of 2 floats The ``(x, y)`` pixel coordinate of the source center. radii : 1D float `~numpy.ndarray` An array of radii defining the profile apertures. ``radii`` must be strictly increasing with a minimum value greater than or equal to zero, and contain at least 2 values. The radial spacing does not need to be constant. See the subclass documentation for details on how ``radii`` is interpreted. error : 2D `~numpy.ndarray`, optional The 1-sigma errors of the input ``data``. ``error`` is assumed to include all sources of error, including the Poisson error of the sources (see `~photutils.utils.calc_total_error`). ``error`` must have the same shape as the input ``data``. mask : 2D bool `~numpy.ndarray`, optional A boolean mask with the same shape as ``data`` where a `True` value indicates the corresponding element of ``data`` is masked. Masked data are excluded from all calculations. <method_subpixels_descriptions> """ # Define axis labels used by `~photutils.profiles.ProfileBase.plot`. # Subclasses may override these. _xlabel = 'Radius (pixels)' _ylabel = 'Profile' # The user-facing name of the ``radii`` parameter, used in # validation error messages. Subclasses that rename the parameter # (e.g., ``half_sizes``) may override this. _radii_name = 'radii' def __init__(self, data, xycen, radii, *, error=None, mask=None, method='exact', subpixels=5): (data, error), unit = process_quantities((data, error), ('data', 'error')) if error is not None and error.shape != data.shape: msg = 'error must have the same shape as data' raise ValueError(msg) self.data = data self.unit = unit self.xycen = xycen self.radii = self._validate_radii(radii) self.error = error self.mask = self._compute_mask(data, error, mask) self.method = method self.subpixels = subpixels # The total normalization applied to the profile. This is the # only mutable state of the class. All normalization-dependent # attributes (e.g., ``profile``) are derived from immutable # cached values divided by this value, and `normalize` and # `unnormalize` update it with a single atomic attribute # store, making the class safe for concurrent reads during # normalization changes. self.normalization_value = 1.0 def _validate_radii(self, radii): """ Validate and return the radii array. """ name = self._radii_name if isinstance(radii, u.Quantity): msg = (f'{name} must be a plain array of pixel values, ' 'not a Quantity') raise TypeError(msg) radii = np.array(radii) if radii.ndim != 1 or radii.size < 2: msg = f'{name} must be a 1D array and have at least two values' raise ValueError(msg) if radii.min() < 0: msg = f'minimum {name} must be >= 0' raise ValueError(msg) if not np.all(radii[1:] > radii[:-1]): msg = f'{name} must be strictly increasing' raise ValueError(msg) return radii def _compute_mask(self, data, error, mask): """ Compute the mask array, automatically masking non-finite data or error values. """ badmask = ~np.isfinite(data) if error is not None: badmask |= ~np.isfinite(error) if mask is not None: if mask.shape != data.shape: msg = 'mask must have the same shape as data' raise ValueError(msg) # Keep only non-finite values not already masked by the user badmask &= ~mask combined_mask = mask | badmask # all masked pixels else: combined_mask = badmask if np.any(badmask): msg = ('Input data contains non-finite values (e.g., NaN ' 'or inf) that were automatically masked.') warnings.warn(msg, AstropyUserWarning) return combined_mask @property @abc.abstractmethod def radius(self): """ The profile radius in pixels as a 1D `~numpy.ndarray`. """ @property @abc.abstractmethod def _raw_profile(self): """ The raw (unnormalized) profile as a 1D `~numpy.ndarray`. """ @property @abc.abstractmethod def _raw_profile_error(self): """ The raw (unnormalized) profile errors as a 1D `~numpy.ndarray`. If no ``error`` array was provided, an empty array with shape ``(0,)`` is returned. """ @property def profile(self): """ The profile as a 1D `~numpy.ndarray`. The returned values reflect the current profile normalization (see `normalize`). """ return self._raw_profile / self.normalization_value @property def profile_error(self): """ The profile errors as a 1D `~numpy.ndarray`. The returned values reflect the current profile normalization (see `normalize`). If no ``error`` array was provided, an empty array with shape ``(0,)`` is returned. """ return self._raw_profile_error / self.normalization_value @cached_property def _circular_apertures(self): """ A list of `~photutils.aperture.CircularAperture` objects. The first element may be `None`. """ from photutils.aperture import CircularAperture apertures = [] for radius in self.radii: if radius <= 0.0: apertures.append(None) else: apertures.append(CircularAperture(self.xycen, radius)) return apertures def _compute_photometry(self, apertures): """ Compute aperture fluxes, flux errors, and areas for the given apertures using a single batched photometry call. Parameters ---------- apertures : list A list of aperture objects sharing the same position. Leading elements may be `None` (e.g., for a zero radius), in which case the corresponding flux, error, and area are set to zero. Returns ------- flux : `~numpy.ndarray` The aperture fluxes. flux_err : `~numpy.ndarray` The aperture flux errors. areas : `~numpy.ndarray` The aperture areas. """ n_none = sum(aperture is None for aperture in apertures) result = AperturePhotometry( self.data, apertures[n_none:], error=self.error, mask=self.mask, method=self.method, subpixels=self.subpixels) fluxes = result.flux areas = result.area.to_value(u.pix ** 2) flux_errs = (result.flux_err if self.error is not None else np.array([])) if n_none > 0: zeros = np.zeros(n_none) fluxes = np.concatenate((zeros, fluxes)) areas = np.concatenate((zeros, areas)) if self.error is not None: flux_errs = np.concatenate((zeros, flux_errs)) if self.unit is not None: fluxes = fluxes << self.unit flux_errs = flux_errs << self.unit return fluxes, flux_errs, areas @cached_property def _photometry(self): """ The aperture fluxes, flux errors, and areas as a function of radius. """ return self._compute_photometry(self._circular_apertures)
[docs] @deprecated_positional_kwargs(since='3.0', until='4.0') def normalize(self, method='max'): """ Normalize the profile. The normalization is computed from the raw (unnormalized) profile values, so repeated calls do not accumulate. The most recent call determines the normalization. Because both normalization methods scale linearly with the profile values, this is equivalent to normalizing an already-normalized profile. Parameters ---------- method : {'max', 'sum'}, optional The method used to normalize the profile: * ``'max'`` (default): The profile is normalized such that its maximum value is 1. * ``'sum'``: The profile is normalized such that the sum of its values is 1. """ if method == 'max': func = nanmax elif method == 'sum': func = nansum else: msg = "invalid method, must be 'max' or 'sum'" raise ValueError(msg) with warnings.catch_warnings(): warnings.simplefilter('ignore', RuntimeWarning) normalization = func(self._raw_profile) if normalization == 0 or not np.isfinite(normalization): msg = ('The profile cannot be normalized because the max or ' 'sum is zero or non-finite.') warnings.warn(msg, AstropyUserWarning) else: # A single atomic attribute store. Concurrent readers see # either the old or the new normalization, never a mixed # state. self.normalization_value = normalization
[docs] def unnormalize(self): """ Unnormalize the profile back to the original state before any calls to `normalize`. """ self.normalization_value = 1.0
@staticmethod def _trim_to_monotonic(xarr, profile, name): """ Trim arrays to the first monotonically increasing region. This is used by interpolation methods that require a monotonically increasing profile. Parameters ---------- xarr : 1D `~numpy.ndarray` The x-axis values (e.g., radius or half-size). profile : 1D `~numpy.ndarray` The profile values. name : str A descriptive name for the profile used in the error message. Returns ------- xarr, profile : tuple of `~numpy.ndarray` The trimmed arrays. """ finite_mask = np.isfinite(profile) if not np.all(finite_mask): # Keep only the leading finite segment first_nonfinite = np.argmin(finite_mask) xarr = xarr[:first_nonfinite] profile = profile[:first_nonfinite] # np.diff produces an array of length n-1: diff[i] represents # the step from profile[i] to profile[i+1]. A value <= 0 means # the profile stopped increasing at that step. diff = np.diff(profile) <= 0 if np.any(diff): # idx is an index into the *diff* array, not the profile # array. diff[idx] <= 0 means the drop occurs between # profile[idx] and profile[idx+1], so profile[idx] is # the last good value. We therefore need profile[:idx+1] # (inclusive) to retain it. idx = np.argmax(diff) # first non-monotonic step in diff-space xarr = xarr[:idx + 1] profile = profile[:idx + 1] if len(xarr) < 2: msg = (f'The {name} profile is not monotonically ' 'increasing even at the smallest values -- cannot ' 'interpolate. Try using different input values ' '(especially the starting values) and/or using the ' '"exact" aperture overlap method.') raise ValueError(msg) return xarr, profile def __repr__(self): cls_name = self.__class__.__name__ n_radii = len(self.radii) normalized = self.normalization_value != 1.0 return (f'{cls_name}(xycen={self.xycen}, n_radii={n_radii}, ' f'normalized={normalized})')
[docs] @deprecated_positional_kwargs(since='3.0', until='4.0') def plot(self, ax=None, **kwargs): """ Plot the profile. Parameters ---------- ax : `matplotlib.axes.Axes` or `None`, optional The matplotlib axes on which to plot. If `None`, then the current `~matplotlib.axes.Axes` instance is used. **kwargs : dict, optional Any keyword arguments accepted by `matplotlib.pyplot.plot`. Returns ------- lines : list of `~matplotlib.lines.Line2D` A list of lines representing the plotted data. """ import matplotlib.pyplot as plt if ax is None: ax = plt.gca() profile = self.profile unit = None if isinstance(profile, u.Quantity): unit = profile.unit profile = profile.value lines = ax.plot(self.radius, profile, **kwargs) ax.set_xlabel(self._xlabel) ylabel = self._ylabel # A normalized profile is dimensionless, so the unit is # included only when the profile has a physical unit if unit is not None and unit != u.dimensionless_unscaled: ylabel = f'{ylabel} ({unit})' ax.set_ylabel(ylabel) return lines
[docs] @deprecated_positional_kwargs(since='3.0', until='4.0') def plot_error(self, ax=None, **kwargs): """ Plot the profile errors. Parameters ---------- ax : `matplotlib.axes.Axes` or `None`, optional The matplotlib axes on which to plot. If `None`, then the current `~matplotlib.axes.Axes` instance is used. **kwargs : dict, optional Any keyword arguments accepted by `matplotlib.pyplot.fill_between`. Returns ------- poly : `matplotlib.collections.PolyCollection` or `None` A `~matplotlib.collections.PolyCollection` containing the plotted polygons, or `None` if no errors were input. """ if len(self.profile_error) == 0: msg = 'Errors were not input' warnings.warn(msg, AstropyUserWarning) return None import matplotlib.pyplot as plt if ax is None: ax = plt.gca() # Set default fill_between facecolor. # facecolor must be first key, otherwise it will override color # kwarg (i.e., cannot use setdefault here) if 'facecolor' not in kwargs: kws = {'facecolor': (0.5, 0.5, 0.5, 0.3)} kws.update(kwargs) else: kws = kwargs profile = self.profile profile_error = self.profile_error if isinstance(profile, u.Quantity): profile = profile.value if isinstance(profile_error, u.Quantity): profile_error = profile_error.value ymin = profile - profile_error ymax = profile + profile_error return ax.fill_between(self.radius, ymin, ymax, **kws)