2023ApJ...945..106P


Query : 2023ApJ...945..106P

2023ApJ...945..106P - Astrophys. J., 945, 106 (2023/March-2)

A Deep-learning Anomaly-detection Method to Identify Gamma-Ray Bursts in the Ratemeters of the AGILE Anticoincidence System.

PARMIGGIANI N., BULGARELLI A., URSI A., MACALUSO A., DI PIANO A., FIORETTI V., ABOUDAN A., BARONCELLI L., ADDIS A., TAVANI M. and PITTORI C.

Abstract (from CDS):

Astro-rivelatore Gamma a Immagini Leggero (AGILE) is a space mission launched in 2007 to study X-ray and gamma-ray astronomy. The AGILE team developed real-time analysis pipelines to detect transient phenomena such as gamma-ray bursts (GRBs) and react to external science alerts received by other facilities. The AGILE anticoincidence system (ACS) comprises five panels surrounding the AGILE detectors to reject background-charged particles. It can also detect hard X-ray photons in the energy range 50-200 keV. The ACS data acquisition produces a time series for each panel. The time series are merged into a single multivariate time series (MTS). We present a new deep-learning model for the detection of GRBs in the ACS data using an anomaly detection technique. The model is implemented with a convolutional neural network autoencoder architecture trained in an unsupervised manner, using a data set of MTSs randomly extracted from the AGILE ACS data. The reconstruction error of the autoencoder is used as the anomaly score to classify the MTS. We calculated the associated p-value distribution, using more than 107 background-only MTSs, to define the statistical significance of the detections. We evaluate the trained model with a list of GRBs reported by the GRBWeb catalog. The results confirm the model's capabilities to detect GRBs in the ACS data. We will implement this method in the AGILE real-time analysis pipeline.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Time series analysis - Gamma-ray bursts - Gamma-ray astronomy - Gamma-ray detectors - Convolutional neural networks

Simbad objects: 72

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Number of rows : 72
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 GRB 180720B gB 00 02 06.99 -02 55 07.8           ~ 215 0
2 GRB 200131A gB 00 12 22.65 +51 07 00.2           ~ 23 0
3 GRB 180806A gB 00 46 12.91 +24 20 14.2           ~ 17 0
4 GRB 150510A gB 01 05 +04.8           ~ 23 0
5 GRB 101014A gB 01 47.8 -51 04           ~ 31 0
6 GRB 120129A gB 02 02 +59.3           ~ 20 0
7 GRB 140416A gB 02 22 +43.9           ~ 17 0
8 GRB 110825A gB 02 59.6 +15 24           ~ 33 0
9 GRB 190114C gB 03 38 01.18 -26 56 47.8           ~ 343 0
10 GRB 131028A gB 03 48 +72.2           ~ 14 0
11 GRB 171010A gB 04 26 19.41 -10 27 47.9           SNIc-BL 109 0
12 GRB 201020B gB 05 01 52.03 +77 04 05.9           ~ 34 0
13 GRB 160131A gB 05 12 40.31 -07 02 59.4           ~ 86 0
14 Fermi bn120711115 gB 06 18 42.839 -70 59 56.78           ~ 125 0
15 GRB 100511A gB 07 17.2 -04 39           ~ 28 0
16 Fermi bn120426090 gB 07 26 -65.6           ~ 17 0
17 GRB 100719D gB 07 33 +05.4           ~ 20 0
18 GRB 150523A gB 07 41 08.67 -45 25 13.6           ~ 24 0
19 Fermi bn141022087 gB 07 58 -75.2           ~ 5 0
20 GRB 190727B gB 08 25 59.90 -13 16 18.9           ~ 18 0
21 GRB 101123A gB 08 45.0 +06 31           ~ 27 0
22 GRB 160530B gB 08 54 +43.5           ~ 14 0
23 GRB 130408A gB 08 57 37.30 -32 21 38.9           ~ 98 0
24 GRB 171119A gB 09 02 -47.0           ~ 10 0
25 Fermi bn170808936 gB 09 43 +02.2           ~ 15 0
26 GRB 150424A gB 10 09 13.35 -26 37 51.2           ~ 94 0
27 GRB 111211A gB 10 12 21.700 +11 12 30.00           ~ 36 0
28 GRB 191221B gB 10 19 19.17 -38 09 27.5           ~ 66 0
29 GRB 131108A gB 10 26 00.480 +09 39 44.05           ~ 96 0
30 GRB 171011B gB 10 35.5 +01 39           ~ 7 0
31 GRB 141207A gB 10 40 +03.9           ~ 28 0
32 GRB 120911B gB 11 28 35 -37 41.8           ~ 11 0
33 GRB 140821A gB 11 39 +13.5           ~ 6 0
34 Fermi bn160113398 gB 12 29 02.4 +11 31 48           ~ 15 0
35 GRB 170115B gB 12 36 -46.9           ~ 25 0
36 GRB 100724A gB 12 58 10.38 -11 06 09.3           ~ 198 0
37 Fermi bn130320560 gB 13 02 -71.3           ~ 8 0
38 GRB 130606B gB 14 34 07.04 -22 06 08.2           ~ 47 0
39 GRB 110715A gB 15 50 44.090 -46 14 06.53           ~ 120 0
40 GRB 170607B gB 16 27 -39.2           ~ 10 0
41 GRB 200829A gB 16 44 49.42 +72 19 45.3           ~ 55 0
42 GRB 190103A gB 16 45.6 +17 23           ~ 7 0
43 GRB 140508A gB 17 01 51.95 +46 46 49.5           ~ 76 0
44 GRB 161010A gB 18 20 51.23 -28 47 06.5           ~ 10 0
45 GRB 141104A gB 18 37 57.0 -12 42 07           ~ 9 0
46 GRB 171227A gB 18 43 -35.0           ~ 27 0
47 GRB 110625A gB 19 06 55.85 +06 45 19.2           ~ 69 0
48 GRB 120707A gB 19 24 -34.4           ~ 21 0
49 GRB 150403A gB 20 46 01.17 -62 42 40.1           ~ 116 0
50 GRB 130821A gB 20 56 38.440 -12 02 36.53           ~ 25 0
51 GRB 101023A gB 21 11 51.26 -65 23 17.7           ~ 71 0
52 GRB 141028A gB 21 30 24.46 -00 13 55.6           ~ 109 0
53 Fermi bn150330828 gB 21 57 +50.0           ~ 22 0
54 GRB 180914B gB 22 09 25.56 +25 03 47.3           ~ 47 0
55 GRB 170127C gB 22 37 -63.9           ~ 39 0
56 GRB 190731A gB 22 38 52.76 -76 34 37.9           ~ 18 0
57 GRB 190706C gB 23 26.7 +24 45           ~ 7 0
58 GRB 170311B gB 23 43 48 +33 24.0           ~ 7 0
59 Fermi bn161218356 gB 23 54 -16.9           ~ 21 0
60 GRB 190501A gB ~ ~           ~ 14 0
61 GRB 160106A gB ~ ~           ~ 10 0
62 GRB 170626B gB ~ ~           ~ 5 0
63 GRB 200919C gB ~ ~           ~ 7 0
64 GRB 190329A gB ~ ~           ~ 6 0
65 GRB 190611B gB ~ ~           ~ 9 0
66 GRB 170522B gB ~ ~           ~ 5 0
67 GRB 190928A gB ~ ~           ~ 16 0
68 GRB 200903E gB ~ ~           ~ 6 0
69 GRB 181121A gB ~ ~           ~ 7 0
70 GRB 140509B gB ~ ~           ~ 3 0
71 GRB 181227A gB ~ ~           ~ 5 0
72 GRB 121118B gB ~ ~           ~ 7 0

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