A Generative Model for Disentangling Galaxy Photometric Parameters
- URL: http://arxiv.org/abs/2507.15898v1
- Date: Mon, 21 Jul 2025 03:09:37 GMT
- Title: A Generative Model for Disentangling Galaxy Photometric Parameters
- Authors: Keen Leung, Colen Yan, Jun Yin,
- Abstract summary: We propose a Conditional AutoEncoder (CAE) framework to simultaneously model and characterize galaxy morphology.<n>Our CAE is trained on a suite of realistic mock galaxy images generated via GalSim, encompassing a broad range of galaxy types, photometric parameters, and observational conditions.<n>By encoding each galaxy image into a low-dimensional latent representation conditioned on key parameters, our model effectively recovers these morphological features in a disentangled manner, while also reconstructing the original image.
- Score: 1.8227840589648028
- License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
- Abstract: Ongoing and future photometric surveys will produce unprecedented volumes of galaxy images, necessitating robust, efficient methods for deriving galaxy morphological parameters at scale. Traditional approaches, such as parametric light-profile fitting, offer valuable insights but become computationally prohibitive when applied to billions of sources. In this work, we propose a Conditional AutoEncoder (CAE) framework to simultaneously model and characterize galaxy morphology. Our CAE is trained on a suite of realistic mock galaxy images generated via GalSim, encompassing a broad range of galaxy types, photometric parameters (e.g., flux, half-light radius, Sersic index, ellipticity), and observational conditions. By encoding each galaxy image into a low-dimensional latent representation conditioned on key parameters, our model effectively recovers these morphological features in a disentangled manner, while also reconstructing the original image. The results demonstrate that the CAE approach can accurately and efficiently infer complex structural properties, offering a powerful alternative to existing methods.
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