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Observational astronomy relies on visual feature identification to detect critical astrophysical phenomena. While machine learning (ML) increasingly automates this process, models often struggle with generalization in large-scale surveys…

Astrophysics of Galaxies · Physics 2026-01-15 Chenrui Ma , Zechang Sun , Tao Jing , Zheng Cai , Yuan-Sen Ting , Song Huang , Mingyu Li

Galaxy morphology is a fundamental quantity, that is essential not only for the full spectrum of galaxy-evolution studies, but also for a plethora of science in observational cosmology. While a rich literature exists on…

Astrophysics of Galaxies · Physics 2020-01-08 Garreth Martin , Sugata Kaviraj , Alex Hocking , Shaun C. Read , James E. Geach

We present a machine learning framework to simulate realistic galaxies for the Euclid Survey. The proposed method combines a control on galaxy shape parameters offered by analytic models with realistic surface brightness distributions…

Astrophysics of Galaxies · Physics 2022-01-26 Euclid Collaboration , H. Bretonnière , M. Huertas-Company , A. Boucaud , F. Lanusse , E. Jullo , E. Merlin , D. Tuccillo , M. Castellano , J. Brinchmann , C. J. Conselice , H. Dole , R. Cabanac , H. M. Courtois , F. J. Castander , P. A. Duc , P. Fosalba , D. Guinet , S. Kruk , U. Kuchner , S. Serrano , E. Soubrie , A. Tramacere , L. Wang , A. Amara , N. Auricchio , R. Bender , C. Bodendorf , D. Bonino , E. Branchini , V. Capobianco , C. Carbone , J. Carretero , S. Cavuoti , A. Cimatti , R. Cledassou , L. Corcione , A. Costille , H. Degaudenzi , M. Douspis , F. Dubath , S. Dusini , S. Ferriol , M. Frailis , E. Franceschi , M. Fumana , B. Garilli , C. Giocoli , A. Grazian , F. Grupp , S. V. H. Haugan , W. Holmes , F. Hormuth , P. Hudelot , K. Jahnke , A. Kiessling , M. Kilbinger , T. Kitching , M. Kümmel , M. Kunz , H. Kurki-Suonio , S. Ligori , P. B. Lilje , I. Lloro , E. Maiorano , O. Mansutti , O. Marggraf , K. Markovic , R. Massey , M. Melchior , M. Meneghetti , G. Meylan , L. Moscardini , S. M. Niemi , C. Padilla , S. Paltani , F. Pasian , K. Pedersen , V. Pettorino , S. Pires , M. Poncet , L. Popa , L. Pozzetti , F. Raison , R. Rebolo , J. Rhodes , M. Roncarelli , E. Rossetti , R. Saglia , P. Schneider , A. Secroun , G. Seidel , C. Sirignano , G. Sirri , J. -L. Starck , A. N. Taylor , I. Tereno , R. Toledo-Moreo , E. A. Valentijn , L. Valenziano , Y. Wang , J. Weller , G. Zamorani , J. Zoubian , M. Baldi , S. Bardelli , S. Brau-Nogue , M. Brescia , S. Camera , G. Congedo , L. Conversi , Y. Copin , C . A. J. Duncan , X. Dupac , R. Farinelli , B. Gillis , S. Kermiche , R. Kohley , F. Marulli , E. Medinaceli , S. Mei , M. Moresco , B. Morin , E. Munari , G. Polenta , E. Romelli , P. Tallada-Crespí , M. Tenti , F. Torradeflot , T. Vassallo , N. Welikala , A. Zacchei , E. Zucca , C. Baccigalupi , A. Balaguera-Antolínez , A. Biviano , S. Borgani , E. Bozzo , C. Burigana , A. Cappi , C. S. Carvalho , S. Casas , G. Castignani , C. Colodro-Conde , J. Coupon , A. Da Silva , S. de la Torre , M. Fabricius , M. Farina , S. Farrens , P. G. Ferreira , P. Flose-Reimberg , S. Fotopoulou , S. Galeotta , K. Ganga , J. Garcia-Bellido , E. Gaztanaga , W. Gillard , G. Gozaliasl , I. M. Hook , B. Joachimi , V. Kansal , A. Kashlinsky , E. Keihanen , C. C. Kirkpatrick , V. Lindholm , G. Mainetti , D. Maino , R. Maoli , M. Martinelli , N. Martinet , S. Maurogordato , H. J. McCracken , R. B. Metcalf , G. Morgante , N. Morisset , R. Nakajima , J. Nightingale , A. Nucita , L. Patrizii , D. Potter , A. Renzi , G. Riccio , A. G. Sánchez , D. Sapone , M. Schirmer , M. Schultheis , V. Scottez , E. Sefusatti , L. Stanco , R. Teyssier , I. Tutusaus , J. Valiviita , M. Viel , L. Whittaker , J. H Knapen

Large-scale structure surveys measure the shapes and positions of millions of galaxies in order to constrain the cosmological model with high precision. The resulting large data volume poses a challenge for the analysis of the data, from…

Cosmology and Nongalactic Astrophysics · Physics 2025-10-28 Silvan Fischbacher , Beatrice Moser , Tomasz Kacprzak , Joerg Herbel , Luca Tortorelli , Uwe Schmitt , Alexandre Refregier , Adam Amara

We show that a Denoising Diffusion Probabalistic Model (DDPM), a class of score-based generative model, can be used to produce realistic mock images that mimic observations of galaxies. Our method is tested with Dark Energy Spectroscopic…

Instrumentation and Methods for Astrophysics · Physics 2022-02-01 Michael J. Smith , James E. Geach , Ryan A. Jackson , Nikhil Arora , Connor Stone , Stéphane Courteau

With the advent of future big-data surveys, automated tools for unsupervised discovery are becoming ever more necessary. In this work, we explore the ability of deep generative networks for detecting outliers in astronomical imaging…

Generative models have recently revolutionized image generation tasks across diverse domains, including galaxy image synthesis. This study investigates the statistical learning and consistency of three generative models: light-weight-gan (a…

Instrumentation and Methods for Astrophysics · Physics 2025-05-13 Jean-Eric Campagne

During the last decade, there has been an explosive growth in survey data and deep learning techniques, both of which have enabled great advances for astronomy. The amount of data from various surveys from multiple epochs with a wide range…

Instrumentation and Methods for Astrophysics · Physics 2021-02-08 Brandon Buncher , Awshesh Nath Sharma , Matias Carrasco Kind

Context. Generative models open up the possibility to interrogate scientific data in a more data-driven way. Aims: We propose a method that uses generative models to explore hypotheses in astrophysics and other areas. We use a neural…

Astrophysics of Galaxies · Physics 2018-12-06 Kevin Schawinski , M. Dennis Turp , Ce Zhang

Cosmological galaxy formation simulations are powerful tools to understand the complex processes that govern the formation and evolution of galaxies. However, evaluating the realism of these simulations remains a challenge. The two common…

Upcoming cosmological weak lensing surveys are expected to constrain cosmological parameters with unprecedented precision. In preparation for these surveys, large simulations with realistic galaxy populations are required to test and…

Astrophysics of Galaxies · Physics 2022-12-13 Yesukhei Jagvaral , Rachel Mandelbaum , Francois Lanusse

Generative models producing images have enormous potential to advance discoveries across scientific fields and require metrics capable of quantifying the high dimensional output. We propose that astrophysics data, such as galaxy images, can…

Instrumentation and Methods for Astrophysics · Physics 2024-07-11 Yun Qi Li , Tuan Do , Evan Jones , Bernie Boscoe , Kevin Alfaro , Zooey Nguyen

In recent years, deep learning models have been successfully employed for augmenting low-resolution cosmological simulations with small-scale information, a task known as "super-resolution". So far, these cosmological super-resolution…

Cosmology and Nongalactic Astrophysics · Physics 2024-11-14 Andreas Schanz , Florian List , Oliver Hahn

Cosmologists at the Institute of Computational Cosmology, Durham University, have developed a state of the art model of galaxy formation known as Galform, intended to contribute to our understanding of the formation, growth and subsequent…

Methodology · Statistics 2014-05-21 Ian Vernon , Michael Goldstein , Richard Bower

We present GLASS, the Generator for Large Scale Structure, a new code for the simulation of galaxy surveys for cosmology, which iteratively builds a light cone with matter, galaxies, and weak gravitational lensing signals as a sequence of…

Cosmology and Nongalactic Astrophysics · Physics 2023-03-28 Nicolas Tessore , Arthur Loureiro , Benjamin Joachimi , Maximilian von Wietersheim-Kramsta , Niall Jeffrey

We present the 'simage' software suite for the simulation of artificial extragalactic images, based empirically around real observations of the Hubble Ultra Deep Field (UDF). The simulations reproduce galaxies with realistic and complex…

Instrumentation and Methods for Astrophysics · Physics 2015-05-19 Benjamin M. Dobke , David E. Johnston , Richard Massey , F. William High , Matthew Ferry , Jason Rhodes , R. Ali Vanderveld

Morphological classification is a key piece of information to define samples of galaxies aiming to study the large-scale structure of the universe. In essence, the challenge is to build up a robust methodology to perform a reliable…

Instrumentation and Methods for Astrophysics · Physics 2019-11-05 P. H. Barchi , R. R. de Carvalho , R. R. Rosa , R. Sautter , M. Soares-Santos , B. A. D. Marques , E. Clua , T. S. Gonçalves , C. de Sá-Freitas , T. C. Moura

Deep generative modeling has emerged as a powerful tool for synthesizing realistic medical images, driving advances in medical image analysis, disease diagnosis, and treatment planning. This chapter explores various deep generative models…

Image and Video Processing · Electrical Eng. & Systems 2024-10-24 Paul Friedrich , Yannik Frisch , Philippe C. Cattin

Maps of cosmic structure produced by galaxy surveys are one of the key tools for answering fundamental questions about the Universe. Accurate theoretical predictions for these quantities are needed to maximize the scientific return of these…

Cosmology and Nongalactic Astrophysics · Physics 2020-12-02 Noah Kasmanoff , Francisco Villaescusa-Navarro , Jeremy Tinker , Shirley Ho

Modern spectroscopic surveys can only target a small fraction of the vast amount of photometrically cataloged sources in wide-field surveys. Here, we report the development of a generative AI method capable of predicting optical galaxy…