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

Author:

Segal Gary12,Parkinson David3ORCID,Norris Ray24ORCID,Hopkins Andrew M5,Andernach Heinz6ORCID,Alexander Emma L7ORCID,Carretti Ettore8ORCID,Koribalski Bärbel S24ORCID,Legodi Letjatji S9,Leslie Sarah10ORCID,Luo Yan11,Pierce Jonathon C S12ORCID,Tang Hongming13ORCID,Vardoulaki Eleni6,Vernstrom Tessa14ORCID

Affiliation:

1. School of Mathematics and Physics, University of Queensland , St Lucia, Brisbane, QLD 4072, Australia

2. CSIRO Space and Astronomy , PO Box 76, Epping, 1710, NSW, Australia

3. Korea Astronomy and Space Science Institute , Daejeon 34055, Korea

4. Western Sydney University , Locked Bag 1797, Penrith, NSW 2751, Australia

5. Australian Astronomical Optics, Macquarie University , 105 Delhi Rd, North Ryde, NSW 2113, Australia

6. Thüringer Landessternwarte , Sternwarte 5, D-07778 Tautenburg, Germany

7. Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester , Manchester M13 9PL, UK

8. INAF, Istituto di Radioastronomia , Via Gobetti 101, I-40129 Bologna, Italy

9. South African Radio Astronomy Observatory , 2 Fir Street, Black River Park, Observatory, Cape Town, 7925, South Africa

10. Leiden Observatory, Leiden University , PO Box 9513, NL-2300 RA Leiden, the Netherlands

11. School of Physics and Astronomy, Sun Yat-sen University , 2 Daxue Road, Zhuhai 519082, China

12. Centre for Astrophysics Research, University of Hertfordshire , College Lane, Hatfield AL10 9AB, UK

13. Department of Astronomy, Tsinghua University , Beijing 100084, China

14. ICRAR, The University of Western Australia , 35 Stirling Hwy, 6009 Crawley, Australia

Abstract

ABSTRACTThe 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.

Funder

Science and Technology Facilities Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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