Bursts from Space: MeerKAT – the first citizen science project dedicated to commensal radio transients

Author:

Andersson Alex1ORCID,Lintott Chris1ORCID,Fender Rob12ORCID,Bright Joe1ORCID,Carotenuto Francesco1ORCID,Driessen Laura345ORCID,Espinasse Mathilde6ORCID,Gasealahwe Kelebogile27ORCID,Heywood Ian189ORCID,van der Horst Alexander J1011ORCID,Motta Sara12ORCID,Rhodes Lauren1ORCID,Tremou Evangelia13ORCID,Williams David R A4ORCID,Woudt Patrick2ORCID,Zhang Xian1415ORCID,Bloemen Steven16ORCID,Groot Paul2716ORCID,Vreeswijk Paul16,Giarratana Stefano1718ORCID,Saikia Payaswini19ORCID,Andersson Jonas20,Ruiz Arroyo Lizzeth20,Baert Loïc20,Baumann Matthew20,Domainko Wilfried20,Eschweiler Thorsten20,Forsythe Tim20,Gaudenzi Sauro20,Ann Grenier Rachel20,Iannone Davide20,Lahoz Karla20,Melville Kyle J20,De Sousa Nascimento Marianne20,Navarro Leticia20,Parthasarathi Sai20,Piilonen 20,Rahman Najma20,Smith Jeffrey20,Stewart B20,Temoke Newton20,Tworek Chloe20,Whittle Isabelle20

Affiliation:

1. Astrophysics, Department of Physics, University of Oxford , Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK

2. Department of Astronomy, University of Cape Town , Private Bag X3, Rondebosch 7701, South Africa

3. CSIRO, Space and Astronomy , PO Box 1130, Bentley, WA 6102, Australia

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

5. Sydney Institute for Astronomy, School of Physics, The University of Sydney , Camperdown, NSW 2006, Australia

6. AIM/CEA Paris-Saclay, Universite Paris Diderot , CNRS, F-91191 Gif-sur-Yvette, France

7. South African Astronomical Observatory , PO Box 9, Observatory 7935, South Africa

8. Department of Physics and Electronics, Rhodes University , PO Box 94, Makhanda 6140, South Africa

9. South African Radio Astronomy Observatory , 2 Fir Street, Observatory 7925, South Africa

10. Department of Physics, The George Washington University , 725 21st Street NW, Washington, DC 20052, USA

11. Astronomy, Physics and Statistics Institute of Sciences (APSIS) , 725 21st Street NW, Washington, DC 20052, USA

12. Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Brera , via E. Bianchi 46, I-23807 Merate (LC), Italy

13. National Radio Astronomy Observatory , Socorro, NM 87801, USA

14. Shanghai Astronomical Observatory, Chinese Academy of Sciences , 80 Nandan Road, Shanghai 200030, China

15. School of Astronomy and Space Science, University of Chinese Academy of Sciences , 19A Yuquanlu, Beijing 100049, China

16. Department of Astrophysics/IMAPP, Radboud University , PO 9010, NL-6500 GL Nijmegen, the Netherlands

17. Dipartimento di Fisica e Astronomia, Università degli Studi di Bologna , Via Gobetti 93/2, I-40129 Bologna, Italy

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

19. Center for Astro, Particle and Planetary Physics, New York University Abu Dhabi , PO Box 129188, Abu Dhabi, UAE

20. Citizen Scientist, Zooniverse c/o University of Oxford , Keble Road, Oxford OX1 3RH, UK

Abstract

ABSTRACT The newest generation of radio telescopes is able to survey large areas with high sensitivity and cadence, producing data volumes that require new methods to better understand the transient sky. Here, we describe the results from the first citizen science project dedicated to commensal radio transients, using data from the MeerKAT telescope with weekly cadence. Bursts from Space: MeerKAT was launched late in 2021 and received ∼89 000 classifications from over 1000 volunteers in 3 months. Our volunteers discovered 142 new variable sources which, along with the known transients in our fields, allowed us to estimate that at least 2.1 per cent of radio sources are varying at 1.28 GHz at the sampled cadence and sensitivity, in line with previous work. We provide the full catalogue of these sources, the largest of candidate radio variables to date. Transient sources found with archival counterparts include a pulsar (B1845-01) and an OH maser star (OH 30.1–0.7), in addition to the recovery of known stellar flares and X-ray binary jets in our observations. Data from the MeerLICHT optical telescope, along with estimates of long time-scale variability induced by scintillation, imply that the majority of the new variables are active galactic nuclei. This tells us that citizen scientists can discover phenomena varying on time-scales from weeks to several years. The success both in terms of volunteer engagement and scientific merit warrants the continued development of the project, while we use the classifications from volunteers to develop machine learning techniques for finding transients.

Funder

Science and Technology Facilities Council

Alfred P. Sloan Foundation

European Research Council

NRF

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Temporal and Spectral Properties of the Persistent Radio Source Associated with FRB 20190520B with the VLA;The Astrophysical Journal;2023-12-01

2. FRB 20121102A: images of the bursts and the varying radio counterpart;Monthly Notices of the Royal Astronomical Society;2023-08-18

3. A new pulsar candidate in 47 Tucanae discovered with MeerKAT imaging;Monthly Notices of the Royal Astronomical Society: Letters;2023-07-04

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