Source code for astrophot.models.pixelated_psf_model

import torch

from .psf_model_object import PSF_Model
from ..image import PSF_Image
from ..utils.decorators import ignore_numpy_warnings, default_internal
from ..utils.interpolate import interp2d
from ._shared_methods import select_target
from ..param import Param_Unlock, Param_SoftLimits
from .. import AP_config

__all__ = ["Pixelated_PSF"]


[docs] class Pixelated_PSF(PSF_Model): """point source model which uses an image of the PSF as its representation for point sources. Using bilinear interpolation it will shift the PSF within a pixel to accurately represent the center location of a point source. There is no funcitonal form for this object type as any image can be supplied. The image pixels will be optimized as individual parameters. This can very quickly result in a large number of parameters and a near impossible fitting task, ideally this should be restricted to a very small area likely at the center of the PSF. To initialize the PSF image will by default be set to the target PSF_Image values, thus one can use an empirical PSF as a starting point. Since only bilinear interpolation is performed, it is recommended to provide the PSF at a higher resolution than the image if it is near the nyquist sampling limit. Bilinear interpolation is very fast and accurate for smooth models, so this way it is possible to do the expensive interpolation before optimization and save time. Note that if you do this you must provide the PSF as a PSF_Image object with the correct pixelscale (essentially just divide the pixelscale by the upsampling factor you used). Parameters: pixels: the total flux within each pixel, represented as the log of the flux. """ model_type = f"pixelated {PSF_Model.model_type}" parameter_specs = { "pixels": {"units": "log10(flux/arcsec^2)"}, } _parameter_order = PSF_Model._parameter_order + ("pixels",) useable = True model_integrated = True
[docs] @torch.no_grad() @ignore_numpy_warnings @select_target @default_internal def initialize(self, target=None, parameters=None, **kwargs): super().initialize(target=target, parameters=parameters) target_area = target[self.window] with Param_Unlock(parameters["pixels"]), Param_SoftLimits(parameters["pixels"]): if parameters["pixels"].value is None: dat = torch.abs(target_area.data) dat[dat == 0] = torch.median(dat) * 1e-7 parameters["pixels"].value = torch.log10(dat / target.pixel_area) if parameters["pixels"].uncertainty is None: parameters["pixels"].uncertainty = torch.abs(parameters["pixels"].value) * self.default_uncertainty
[docs] @default_internal def evaluate_model(self, X=None, Y=None, image=None, parameters=None, **kwargs): if X is None: Coords = image.get_coordinate_meshgrid() X, Y = Coords - parameters["center"].value[..., None, None] # Convert coordinates into pixel locations in the psf image pX, pY = self.target.plane_to_pixel(X, Y) # Select only the pixels where the PSF image is defined select = torch.logical_and( torch.logical_and(pX > -0.5, pX < parameters["pixels"].shape[1] - 0.5), torch.logical_and(pY > -0.5, pY < parameters["pixels"].shape[0] - 0.5), ) # Zero everywhere outside the psf result = torch.zeros_like(X) # Use bilinear interpolation of the PSF at the requested coordinates result[select] = interp2d(parameters["pixels"].value, pX[select], pY[select]) return image.pixel_area * 10 ** result