2024MNRAS.531.2474S


Query : 2024MNRAS.531.2474S

2024MNRAS.531.2474S - Mon. Not. R. Astron. Soc., 531, 2474-2492 (2024/June-3)

NEural Engine for Discovering Luminous Events (NEEDLE): identifying rare transient candidates in real time from host galaxy images.

SHENG X., NICHOLL M., SMITH K.W., YOUNG D.R., WILLIAMS R.D., STEVANCE H.F., SMARTT S.J., SRIVASTAV S. and MOORE T.

Abstract (from CDS):

Known for their efficiency in analysing large data sets, machine learning-based classifiers have been widely used in wide-field sky survey pipelines. The upcoming Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will generate millions of real-time alerts every night, enabling the discovery of large samples of rare events. Identifying such objects soon after explosion will be essential to study their evolution. Using ∼5400 transients from the Zwicky Transient Facility (ZTF) Bright Transient Survey as training and test data, we develop NEEDLE (NEural Engine for Discovering Luminous Events), a novel hybrid (convolutional neural network + dense neural network) classifier to select for two rare classes with strong environmental preferences: superluminous supernovae (SLSNe) preferring dwarf galaxies, and tidal disruption events (TDEs) occurring in the centres of nucleated galaxies. The input data includes (i) cutouts of the detection and reference images, (ii) photometric information contained directly in the alert packets, and (iii) host galaxy magnitudes from Pan-STARRS (Panoramic Survey Telescope and Rapid Response System). Despite having only a few tens of examples of the rare classes, our average (best) completeness on an unseen test set reaches 73 per cent (86 per cent) for SLSNe and 80 per cent (87 per cent) for TDEs. While very encouraging for completeness, this may still result in relatively low purity for the rare transients, given the large class imbalance in real surveys. However, the goal of NEEDLE is to find good candidates for spectroscopic classification, rather than to select pure photometric samples. Our system will be deployed as an annotator on the UK alert broker, Lasair, to provide predictions of real-time alerts from ZTF and LSST to the community.

Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): methods: data analysis - surveys - transients: supernovae - transients: tidal disruption events

Simbad objects: 46

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Number of rows : 46
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 PSST 23jmv ev 00 22 36.290 -24 27 44.53           SLSN-I 2 0
2 SN 2022aawb SN* 01 44 52.380 +23 00 43.85           SNI 4 0
3 PSST 23jlr ev 02 23 18.740 -21 03 16.99           SLSN-I 2 0
4 SN 2020aatc SN* 02 48 16.40 -10 15 07.4           SNIa 5 0
5 SN 2021ek SN* 03 23 49.914 -10 02 41.18           SLSN-I 7 0
6 ATLAS 23qwt ev 04 25 50.100 -09 09 28.08           SLSN-I 2 0
7 ATLAS 23aqg ev 06 12 59.132 +68 48 45.35           SLSN-I 3 0
8 ATLAS 23upj ev 06 13 40.222 +69 43 38.89           SLSN-I 2 0
9 ATLAS 23csk ev 07 06 54.650 +37 58 35.54           SLSN-I 3 0
10 ATLAS 22bjqu ev 07 12 41.810 +07 18 59.95           SLSN-I 3 0
11 AT 2023xen ev 07 52 12.679 +37 21 34.15           ~ 1 0
12 AT 2023tmq ev 09 19 05.890 +13 26 52.80           ~ 1 0
13 ATLAS 22bnjj ev 09 24 01.916 -13 31 29.00           SLSN-I 1 0
14 SN 2020afah SN* 10 20 18.320 +53 19 21.40           ~ 5 0
15 ATLAS 22kxk ev 10 50 27.864 -06 17 48.15           SLSN-I 4 0
16 SN 2023aase SN* 11 32 22.070 -03 19 20.50           SLSN-I 2 0
17 ATLAS 23xoa ev 11 39 08.684 -11 14 57.90           SLSN-I 2 0
18 PSST 22diw ev 12 57 59.611 +41 04 42.06           SLSN-I 4 0
19 ATLAS 23jmp ev 12 58 59.485 +69 33 51.20           SLSN-I 1 0
20 SN 2021hpc SN* 13 33 01.069 +43 10 33.80           SLSN-I 4 0
21 AT 2023mhs ev 13 43 15.681 +19 15 00.90           ~ 3 0
22 SDSS J140941.88+552928.0 AGN 14 09 41.8833027816 +55 29 28.058874792           ~ 55 0
23 AT 2021ahpl ev 15 15 57.940 -19 17 31.96           SLSN-I 4 0
24 AT 2020pj ev 15 31 34.960 +33 05 41.47           ~ 17 0
25 SN 2022ljr SN? 15 43 02.080 +18 04 35.98           SLSN-I 5 0
26 SN 2023qvl ev 15 50 08.295 +53 39 37.04           SLSN-I 2 0
27 AT 2019mha ev 16 16 27.799 +56 25 56.29           ~ 19 0
28 SN 2018geo SN* 16 18 13.840 +39 07 25.74           SNIa 8 0
29 PSST 23dbu ev 16 18 21.539 +01 31 43.37           SLSN-I 2 0
30 ATLAS 22vfs ev 16 21 03.732 +14 50 54.75           SLSN-I 5 0
31 ATLAS 22rdp ev 17 36 38.683 +61 33 18.66           SLSN-I 4 0
32 AT 2023wdb ev 18 25 20.915 +30 11 21.46           TDE 1 0
33 AT 2023cvb ev 19 14 25.680 +41 40 09.28           ~ 6 0
34 PSST 22ger ev 19 20 10.670 +50 23 42.36           SLSN-I 3 0
35 AT 2023rvb ev 19 21 12.547 -22 38 39.61           ~ 2 0
36 PSST 22kdy ev 20 29 10.460 -06 46 17.08           SLSN-I 5 0
37 SN 2018ffs SN* 20 54 37.147 +22 04 51.81           SLSN-I 12 0
38 AT 2023mfm ev 21 37 27.961 -04 20 43.16           ~ 1 0
39 ATLAS 22xpx ev 21 48 58.161 -26 22 36.88           SLSN-I 3 0
40 PSST 23lke ev 22 19 56.013 +25 54 56.12           SLSN-I 2 0
41 ATLAS 23wjo ev 22 43 08.735 -23 47 30.87           SLSN-I 3 0
42 PSST 22nhu ev 23 03 54.175 +15 46 19.75           SLSN-I 2 0
43 ATLAS 23wsa ev 23 07 47.653 +43 51 03.63           SLSN-I 2 0
44 SN 2022ojm ev 23 37 46.031 +40 05 07.99           SLSN-I 3 0
45 AT 2023kvy ev 23 39 47.964 +08 09 53.62           ~ 3 0
46 ATLAS 20bbuz ev 23 57 24.783 +25 03 48.68           SN-IIn 1 0

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