Source code for astrophot.models.point_source

from typing import Optional

import torch
import numpy as np

from .base import Model
from .model_object import ComponentModel
from ..image import ModelImage
from ..utils.decorators import ignore_numpy_warnings, combine_docstrings
from ..utils.interpolate import interp2d
from ..image import Window, PSFImage
from ..errors import SpecificationConflict
from ..param import forward
from ..backend_obj import backend, ArrayLike
from .. import config
from . import func

__all__ = ("PointSource",)


[docs] @combine_docstrings class PointSource(ComponentModel): """Describes a point source in the image, this is a delta function at some position in the sky. This is typically used to describe stars, supernovae, very small galaxies, quasars, asteroids or any other object which can essentially be entirely described by a position and total flux (no structure). **Parameters:** - `flux`: The total flux of the point source """ _model_type = "point" _parameter_specs = { "flux": {"units": "flux", "valid": (0, None), "shape": (), "dynamic": True}, } internal_psf = True usable = True def __init__(self, *args, integrate_mode="none", **kwargs): super().__init__(*args, integrate_mode=integrate_mode, **kwargs)
[docs] @torch.no_grad() @ignore_numpy_warnings def initialize(self): super().initialize() if self.psf is None: raise SpecificationConflict("PointSource needs a psf!") if self.flux.initialized: return target_area = self.target[self.window] dat = backend.to_numpy(target_area._data).copy() mask = backend.to_numpy(target_area._mask) dat[mask] = np.median(dat[~mask]) edge = np.concatenate((dat[:, 0], dat[:, -1], dat[0, :], dat[-1, :])) edge_average = np.median(edge) self.flux.value = np.abs(np.sum(dat - edge_average))
@property def integrate_mode(self): return "none" @integrate_mode.setter def integrate_mode(self, value): if value != "none": config.logger.warning( "PointSource models are restricted to integrate mode of 'none', ignoring integrate_mode setting." ) # Psf convolution should be on by default since this is a delta function @property def psf_convolve(self): return True @psf_convolve.setter def psf_convolve(self, value): pass def _prep_psf(self): psf = self.psf if isinstance(psf, PSFImage): return psf._data, psf.upsample, 0 if isinstance(psf, Model): return psf, psf.upsample, 0 return None, 1, 0
[docs] @forward def sample( self, I_: ArrayLike, J_: ArrayLike, psf: ArrayLike = None, crop: int = 0, downsample: int = 1, center=None, flux=None, _CD=None, _crtan=None, _crpix=None, ): if isinstance(psf, Model): psf = psf()._data if _CD is None: i0, j0 = self.target.plane_to_pixel(*center) else: i0, j0 = self.target.plane_to_pixel(*center, CD=_CD, crtan=_crtan, _crpix=_crpix) Z = interp2d( psf, (I_ - i0) * downsample + (psf.shape[0] // 2), (J_ - j0) * downsample + (psf.shape[1] // 2), ) Z = self._pixel_integrator(Z) Z = Z * flux Z = func.downsample(Z, downsample) return Z