From f62c9581ab78472dc4c559eef3637d57219a9c63 Mon Sep 17 00:00:00 2001
From: James Nightingale <james.w.nightingale@durham.ac.uk>
Date: Tue, 30 Jan 2024 17:33:25 +0000
Subject: [PATCH 1/2] rename subtracted_signal_to_noise_map_of_galaxies

---
 autolens/imaging/fit_imaging.py | 19 +++++++++++++++++++
 1 file changed, 19 insertions(+)

diff --git a/autolens/imaging/fit_imaging.py b/autolens/imaging/fit_imaging.py
index 7aacf2aaf..b7f601fda 100644
--- a/autolens/imaging/fit_imaging.py
+++ b/autolens/imaging/fit_imaging.py
@@ -205,6 +205,25 @@ def subtracted_images_of_galaxies_dict(self) -> Dict[ag.Galaxy, np.ndarray]:
 
         return subtracted_images_of_galaxies_dict
 
+    @property
+    def subtracted_signal_to_noise_maps_of_galaxies_dict(self) -> Dict[ag.Galaxy, np.ndarray]:
+        """
+        A dictionary which associates every galaxy in the tracer with its `subtracted image`.
+
+        A subtracted image of a galaxy is the data where all other galaxy images are subtracted from it, therefore
+        showing how a galaxy appears in the data in the absence of all other galaxies.
+
+        This is used to visualize the contribution of each galaxy in the data.
+        """
+
+        subtracted_signal_to_noise_maps_of_galaxies_dict = {}
+
+        for (galaxy, subtracted_image) in self.subtracted_images_of_galaxies_dict.items():
+
+            subtracted_signal_to_noise_maps_of_galaxies_dict[galaxy] = subtracted_image / self.noise_map
+
+        return subtracted_signal_to_noise_maps_of_galaxies_dict
+
     @property
     def model_images_of_planes_list(self) -> List[aa.Array2D]:
         """

From e8ce0b48d6658ab28d9dd80f429b726d88caf22a Mon Sep 17 00:00:00 2001
From: James Nightingale <james.w.nightingale@durham.ac.uk>
Date: Thu, 1 Feb 2024 18:32:41 +0000
Subject: [PATCH 2/2] fix interferometer adapt_images

---
 autolens/interferometer/model/result.py | 27 +++++++++++++++++++++++++
 1 file changed, 27 insertions(+)

diff --git a/autolens/interferometer/model/result.py b/autolens/interferometer/model/result.py
index 3edb5dd3a..a4a893671 100644
--- a/autolens/interferometer/model/result.py
+++ b/autolens/interferometer/model/result.py
@@ -3,6 +3,7 @@
 import autoarray as aa
 import autogalaxy as ag
 
+from autogalaxy.analysis.adapt_images import AdaptImages
 from autolens.lens.ray_tracing import Tracer
 from autolens.interferometer.fit_interferometer import FitInterferometer
 from autolens.analysis.result import ResultDataset
@@ -67,3 +68,29 @@ def real_space_mask(self) -> aa.Mask2D:
         The real space mask used by this model-fit.
         """
         return self.max_log_likelihood_fit.dataset.real_space_mask
+
+    def adapt_images_from(self, use_model_images : bool = False) -> AdaptImages:
+        """
+        Returns the adapt-images which are used to make a pixelization's mesh and regularization adapt to the
+        reconstructed galaxy's morphology.
+
+        This can use either:
+
+        - The model image of each galaxy in the best-fit model.
+        - The subtracted image of each galaxy in the best-fit model, where the subtracted image is the dataset
+          minus the model images of all other galaxies.
+
+        In **PyAutoLens** these adapt images have had lensing calculations performed on them and therefore for source
+        galaxies are their lensed model images in the image-plane.
+
+        Parameters
+        ----------
+        use_model_images
+            If True, the model images of the galaxies are used to create the adapt images. If False, the subtracted
+            images of the galaxies are used.
+        """
+
+        return AdaptImages.from_result(
+            result=self,
+            use_model_images=True
+        )
\ No newline at end of file