18-19 April 2024
Institut de Ciencies de L'Espai (ICE)
Europe/Madrid timezone
Spring 2024

Identifying stellar disk truncations in Euclid galaxy images using Segment Anything Model

19 Apr 2024, 11:50
10m
Alberto Lobo (Institut de Ciencies de L'Espai (ICE))

Alberto Lobo

Institut de Ciencies de L'Espai (ICE)

Campus UAB, Carrer de Can Magrans s/n Cerdanyola (Barcelona)
Talk Galaxy

Speaker

Jesús Vega Ferrero (Centro de Estudios de Física del Cosmos de Aragón (CEFCA))

Description

Stellar disk truncations are a long-sought galactic size indicator based on the radial location of the gas density threshold for star formation, i.e., the edge/limit of the luminous matter in a galaxy. The study of galaxy sizes is crucial for understanding the physical processes that shape galaxy evolution across cosmic time. Current and future ultradeep and large-area imaging surveys, such as the ESA's Euclid mission, will allow us to explore the growth of galaxies and trace the limits of star formation in their outskirts.

The task of identifying the disk truncations in galaxy images is equivalent to what is called (informed) image segmentation in computer vision. Recently, the Meat AI research team published the Segment Anything Model (SAM, Kirillov et al. 2023). SAM is a foundational deep learning model that is capable of segmenting any type of data (including text, images, and audio) into smaller components or segments. The model is designed to be highly adaptable and versatile making it suitable for a wide range of applications.

In preparation for automatically identifying disk truncations in the galaxy images that will be soon released by Euclid, we run SAM over a dataset of more than 1000 disc galaxies within the HST CANDELS fields presented in Buitrago & Trujillo 2024. We 'euclidize' the HST galaxy images by making composite RGB images using the H, J and I+V HST filters, respectively. Using these images as input for the SAM, we retrieve various truncation masks for each galaxy image given different configurations of the input dataset (i.e. varying the stretch and normalization of the input images). Finally, we present a comparison of the truncations obtained with the SAM on the whole 'euclidized' dataset with the results presented in Buitrago & Trujillo 2024, in which truncations are evaluated using the radial positions of the edge in the light profiles of galaxies. Our findings indicate the exceptional capability of SAM to identify truncations in large samples of galaxies in a fully automated manner, eliminating the need for extensive data preprocessing or a labeled dataset.

Primary authors

Jesús Vega Ferrero (Centro de Estudios de Física del Cosmos de Aragón (CEFCA)) Fernando Buitrago (Universidad de Valladolid (UVa)) Jesús Fernández (Universidad de Valladolid (UVa)) Benjamín Sahelices (Universidad de Valladolid (UVa))

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