2023MNRAS.521.1429S


Query : 2023MNRAS.521.1429S

2023MNRAS.521.1429S - Mon. Not. R. Astron. Soc., 521, 1429-1447 (2023/May-1)

Identifying anomalous radio sources in the Evolutionary Map of the Universe Pilot Survey using a complexity-based approach.

SEGAL G., PARKINSON D., NORRIS R., HOPKINS A.M., ANDERNACH H., ALEXANDER E.L., CARRETTI E., KORIBALSKI B.S., LEGODI L.S., LESLIE S., LUO Y., PIERCE J.C.S., TANG H., VARDOULAKI E. and VERNSTROM T.

Abstract (from CDS):

The Evolutionary Map of the Universe (EMU) large-area radio continuum survey will detect tens of millions of radio galaxies, giving an opportunity for the detection of previously unknown classes of objects. To maximize the scientific value and make new discoveries, the analysis of these data will need to go beyond simple visual inspection. We propose the coarse-grained complexity, a simple scalar quantity relating to the minimum description length of an image that can be used to identify unusual structures. The complexity can be computed without reference to the broader sample or existing catalogue data, making the computation efficient on new surveys at very large scales (such as the full EMU survey). We apply our coarse-grained complexity measure to data from the EMU Pilot Survey to detect and confirm anomalous objects in this data set and produce an anomaly catalogue. Rather than work with existing catalogue data using a specific source detection algorithm, we perform a blind scan of the area, computing the complexity using a sliding square aperture. The effectiveness of the complexity measure for identifying anomalous objects is evaluated using crowd-sourced labels generated via the Zooniverse.org platform. We find that the complexity scan identifies unusual sources, such as odd radio circles, by partitioning on complexity. We achieve partitions where 5 per cent of the data is estimated to be 86 per cent complete, and 0.5 per cent is estimated to be 94 per cent pure, with respect to anomalies and use this to produce an anomaly catalogue.

Abstract Copyright: © 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): surveys - galaxies: statistics - radio continuum: galaxies

Simbad objects: 45

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Number of rows : 45
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 LEDA 64440 Sy2 20 18 01.2940411824 -55 39 31.590064800   15.5       ~ 91 0
2 PMN J2026-5522 rG 20 26 44.4 -55 22 27           ~ 2 0
3 DES J202714.57-551846.9 rG 20 27 14.6 -55 18 47           ~ 1 0
4 2MASS J20281812-4924090 rG 20 28 18.12120 -49 24 09.0972           ~ 1 0
5 DES J203408.30-525341.8 rG 20 34 08.3 -52 53 42           ~ 1 0
6 FRL 74 G 20 36.5 -57 38   16       ~ 2 0
7 ESO 143-35 rG 20 36 34.5476181336 -57 37 23.170273968   15.02   13.28   ~ 18 0
8 NGC 6935 EmG 20 38 20.1988150992 -52 06 37.891816812   12.77 12.10 11.57   ~ 72 0
9 LEDA 142042 rG 20 41 12.0515507160 -52 57 37.790045172   15.33   14.46   ~ 16 0
10 ESO 234-68 rG 20 45 52.24212 -51 06 27.1808   14.38   12.69   ~ 27 0
11 LEDA 479547 rG 20 48 37.6615016914 -49 11 15.283881715           ~ 4 0
12 NGC 6984 Sy2 20 57 53.9873335608 -51 52 15.058670700   13.19 12.65 12.22   ~ 58 0
13 ORC J2058-5736a Rad 20 58 42.80 -57 36 58.0           ~ 10 0
14 DES J205848.79-573612.0 rG 20 58 48.7926829417 -57 36 12.147116007           ~ 3 0
15 ORC J2058-5736b Rad 20 58 56.30 -57 36 55.0           ~ 9 0
16 2MASX J21163413-6301068 rG 21 16 34.13087 -63 01 06.8660           ~ 1 0
17 ESO 236-8 Sy2 21 24 26.3026315872 -49 16 48.793134900   14.27   13.31   ~ 18 0
18 NGC 7059 EmG 21 27 21.4652309472 -60 00 52.783268292   12.51 12.30 11.38 11.9 ~ 84 0
19 3FGL J2127.5-6001 X 21 27 29.3 -60 01 02           ~ 21 0
20 LEDA 163125 rG 21 28 41.1951697224 -60 21 57.277737864   17.18   15.77   ~ 5 0
21 LEDA 66845 G 21 29 19.0390803192 -50 53 03.863430384   16.28       ~ 7 0
22 ACO 3771 ClG 21 29 43.2 -50 48 34           ~ 50 0
23 LEDA 66975 G 21 34 06.6924167880 -53 34 18.829328484   15.97       ~ 14 0
24 PKS 2130-53 rG 21 34 16.0 -53 36 55           ~ 21 0
25 LEDA 66976 BiC 21 34 17.6989476984 -53 38 10.612032792   15.71       ~ 12 0
26 ACO 3785 ClG 21 34 28 -53 37.6           ~ 19 2
27 FRL 106 BiC 21 35 11.4802975560 -62 04 42.892940820   15.90       ~ 14 0
28 NGC 7090 EmG 21 36 28.865 -54 33 26.35 12.35 11.60 11.05 10.82 11.2 ~ 183 0
29 2MASS J21380846-5937185 rG 21 38 08.4677056172 -59 37 18.615850014         17.212 ~ 1 0
30 LEDA 189336 BiC 21 39 29.9576436744 -51 23 44.005456428   15.96       ~ 10 0
31 ACO 3796 ClG 21 39.5 -51 23           ~ 12 1
32 LEDA 355032 rG 21 43 11.9 -61 28 18   18.049   16.479   ~ 3 0
33 DES J214331.34-510541.1 rG 21 43 31.3 -51 05 41           ~ 1 0
34 LEDA 488728 rG 21 44 02.1 -48 18 57           ~ 2 0
35 NGC 7125 EmG 21 49 15.945 -60 42 47.42   12.70 12.37 11.77   ~ 70 0
36 PKS 2148-555 rG 21 51 29.91033 -55 20 12.7530   15.79 16.0     ~ 31 0
37 LEDA 373590 rG 21 55 12.6 -59 09 02           ~ 3 0
38 PKS J2200-5610 rG 22 00 24.11850 -56 10 41.6434   15.96 16.0     ~ 21 1
39 IC 5152 rG 22 02 41.521 -51 17 47.20   11.03 10.9 10.19   ~ 273 1
40 NGC 7205 Sy2 22 08 34.3216157064 -57 26 33.586141884   11.77   10.63 11.1 ~ 123 0
41 DES J221640.02-625241.6 rG 22 16 40.0 -62 52 42           ~ 1 0
42 2MASS J22193349-6001502 rG 22 19 33.4640729466 -60 01 50.032480955         17.278 ~ 1 0
43 PKS 2218-50 rG 22 21 06.0 -50 18 25   15.3       ~ 11 1
44 APMUKS (BJ) B221818.62-503153.8 G 22 21 26.64553 -50 16 45.3040           ~ 1 0
45 NAME Local Group GrG ~ ~           ~ 9325 0

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