TY - JOUR
T1 - DELIGHT
T2 - Deep Learning Identification of Galaxy Hosts of Transients using Multiresolution Images
AU - Förster, Francisco
AU - Muñoz Arancibia, Alejandra M.
AU - Reyes-Jainaga, Ignacio
AU - Gagliano, Alexander
AU - Britt, Dylan
AU - Cuellar-Carrillo, Sara
AU - Figueroa-Tapia, Felipe
AU - Polzin, Ava
AU - Yousef, Yara
AU - Arredondo, Javier
AU - Rodríguez-Mancini, Diego
AU - Correa-Orellana, Javier
AU - Bayo, Amelia
AU - Bauer, Franz E.
AU - Catelan, Márcio
AU - Cabrera-Vives, Guillermo
AU - Dastidar, Raya
AU - Estévez, Pablo A.
AU - Pignata, Giuliano
AU - Hernández-García, Lorena
AU - Huijse, Pablo
AU - Reyes, Esteban
AU - Sánchez-Sáez, Paula
AU - Ramírez, Mauricio
AU - Grandón, Daniela
AU - Pineda-García, Jonathan
AU - Chabour-Barra, Francisca
AU - Silva-Farfán, Javier
N1 - Publisher Copyright:
© 2022. The Author(s). Published by the American Astronomical Society.
PY - 2022/11/1
Y1 - 2022/11/1
N2 - We present DELIGHT, or Deep Learning Identification of Galaxy Hosts of Transients, a new algorithm designed to automatically and in real time identify the host galaxies of extragalactic transients. The proposed algorithm receives as input compact, multiresolution images centered at the position of a transient candidate and outputs two-dimensional offset vectors that connect the transient with the center of its predicted host. The multiresolution input consists of a set of images with the same number of pixels, but with progressively larger pixel sizes and fields of view. A sample of 16,791 galaxies visually identified by the Automatic Learning for the Rapid Classification of Events broker team was used to train a convolutional neural network regression model. We show that this method is able to correctly identify both relatively large (10″ < r < 60″) and small (r ≤ 10″) apparent size host galaxies using much less information (32 kB) than with a large, single-resolution image (920 kB). The proposed method has fewer catastrophic errors in recovering the position and is more complete and has less contamination (<0.86%) recovering the crossmatched redshift than other state-of-the-art methods. The more efficient representation provided by multiresolution input images could allow for the identification of transient host galaxies in real time, if adopted in alert streams from new generation of large -etendue telescopes such as the Vera C. Rubin Observatory.
AB - We present DELIGHT, or Deep Learning Identification of Galaxy Hosts of Transients, a new algorithm designed to automatically and in real time identify the host galaxies of extragalactic transients. The proposed algorithm receives as input compact, multiresolution images centered at the position of a transient candidate and outputs two-dimensional offset vectors that connect the transient with the center of its predicted host. The multiresolution input consists of a set of images with the same number of pixels, but with progressively larger pixel sizes and fields of view. A sample of 16,791 galaxies visually identified by the Automatic Learning for the Rapid Classification of Events broker team was used to train a convolutional neural network regression model. We show that this method is able to correctly identify both relatively large (10″ < r < 60″) and small (r ≤ 10″) apparent size host galaxies using much less information (32 kB) than with a large, single-resolution image (920 kB). The proposed method has fewer catastrophic errors in recovering the position and is more complete and has less contamination (<0.86%) recovering the crossmatched redshift than other state-of-the-art methods. The more efficient representation provided by multiresolution input images could allow for the identification of transient host galaxies in real time, if adopted in alert streams from new generation of large -etendue telescopes such as the Vera C. Rubin Observatory.
UR - http://www.scopus.com/inward/record.url?scp=85141324091&partnerID=8YFLogxK
U2 - 10.3847/1538-3881/ac912a
DO - 10.3847/1538-3881/ac912a
M3 - Article
AN - SCOPUS:85141324091
SN - 0004-6256
VL - 164
JO - Astronomical Journal
JF - Astronomical Journal
IS - 5
M1 - 195
ER -