2022AJ....164..195F


Query : 2022AJ....164..195F

2022AJ....164..195F - Astron. J., 164, 195 (2022/November-0)

DELIGHT: Deep Learning Identification of Galaxy Hosts of Transients using Multiresolution Images.

FORSTER F., MUNOZ ARANCIBIA A.M., REYES-JAINAGA I., GAGLIANO A., BRITT D., CUELLAR-CARRILLO S., FIGUEROA-TAPIA F., POLZIN A., YOUSEF Y., ARREDONDO J., RODRIGUEZ-MANCINI D., CORREA-ORELLANA J., BAYO A., BAUER F.E., CATELAN M., CABRERA-VIVES G., DASTIDAR R., ESTEVEZ P.A., PIGNATA G., HERNANDEZ-GARCIA L., HUIJSE P., REYES E., SANCHEZ-SAEZ P., RAMIREZ M., GRANDON D., PINEDA-GARCIA J., CHABOUR-BARRA F. and SILVA-FARFAN J.

Abstract (from CDS):

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.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Supernovae - Galaxies - Astroinformatics - Astronomical object identification - Classification

Simbad objects: 14

goto Full paper

goto View the references in ADS

Number of rows : 14
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SN 2004eh SN* 02 26 11.82 +27 36 24.1     17.1     SNIb 8 1
2 SN 2012fk SN* 02 30 52.04 +22 28 45.9           SNIa 10 1
3 SN 2009bw SN* 03 56 06.92 +72 55 40.9           SNII 70 1
4 AT 2020wub ev 07 02 46.07179714286 +07 30 00.7335514286           ~ 1 0
5 AT 2021fm ev 07 33 31.5091 +33 45 06.066           ~ 1 0
6 AT 2019tdt ev 08 21 00.50494800000 +05 45 03.2489100000           ~ 1 0
7 SN 2009jy SN* 10 19 39.25 -25 49 21.9           SNIc 6 1
8 SN 2006C SN* 12 02 32.50 +41 02 40.2     17.5     SNII 12 1
9 SN 2008bf SN* 12 04 02.878 +20 14 42.29           SNIa 74 2
10 AT 2020aavt ev 14 13 57.82623692308 +31 33 20.7115200000           ~ 1 0
11 AT 2019rra SN* 16 38 39.370 +33 40 41.44           SNIIP 2 0
12 ATLAS 19ypi ev 17 04 45.836 +15 21 15.17           SN.Ia 1 0
13 SN 2011ft SN* 17 52 42.98 +29 04 10.6           SNIb 11 1
14 ATLAS 20kcx ev 19 42 26.15699895653 -15 52 44.1017791304           SN.II 1 0

To bookmark this query, right click on this link: simbad:objects in 2022AJ....164..195F and select 'bookmark this link' or equivalent in the popup menu