Issue |
A&A
Volume 670, February 2023
|
|
---|---|---|
Article Number | A124 | |
Number of page(s) | 15 | |
Section | Catalogs and data | |
DOI | https://doi.org/10.1051/0004-6361/202245567 | |
Published online | 17 February 2023 |
V-LoTSS: The circularly polarised LOFAR Two-metre Sky Survey★
1
Leiden Observatory, Leiden University,
PO Box 9513,
2300 RA
Leiden, The Netherlands
2
ASTRON, Netherlands Institute for Radio Astronomy,
Oude Hoogeveensedijk 4,
7991 PD
Dwingeloo, The Netherlands
3
Kapteyn Astronomical Institute, University of Groningen,
PO Box 800,
9700 AV
Groningen, The Netherlands
4
School of Physical Sciences and Centre for Astrophysics & Relativity, Dublin City University,
Glasnevin
D09 W6Y4, Ireland
5
Institute for Astronomy, University of Edinburgh, Royal Observatory,
Blackford Hill,
Edinburgh
EH9 3HJ, UK
6
Centre for Astrophysics Research, Department of Physics, Astronomy and Mathematics, University of Hertfordshire,
College Lane,
Hatfield
AL10 9AB, UK
7
Department of Astrophysics/IMAPP, Radboud University,
PO Box 9010,
6500 GL
Nijmegen, The Netherlands
8
LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris,
5 Place Jules Janssen,
92195
Meudon, France
9
Aix-Marseille Université, CNRS, CNES, LAM,
Marseille, France,
38 Rue Frédéric Joliot Curie,
13013
Marseille, France
10
School of Mathematics and Physics, The University of Queensland,
St Lucia, QLD
4072, Australia
11
Centre for Astrophysics, University of Southern Queensland,
West Street,
Toowoomba, QLD
4350, Australia
12
Fakultät für Physik, Universität Bielefeld,
Postfach 100131,
33501
Bielefeld, Germany
13
GEPI & ORN, Observatoire de Paris, Université PSL, CNRS,
5 Place Jules Janssen,
92190
Meudon, France
14
Department of Physics & Electronics, Rhodes University,
PO Box 94,
Grahamstown
6140, South Africa
15
School for Physical Sciences, The Open University,
Milton Keynes
MK11 9DL, England, UK
16
Space Science and Technology Division, RALSpace, STFC Rutherford Appleton Laboratory,
Chilton, Didcot
OX11 0NX, England, UK
17
ORN, Observatoire de Paris, CNRS, PSL, Université d’Orléans,
Nançay, France
18
Ruhr University Bochum (RUB), Faculty of Physics and Astronomy, Astronomical Institute,
Universitätsstr. 150,
44801
Bochum, Germany
19
Dipartimento di Fisica e Astronomia (DIFA), Universitá di Bologna,
via Gobetti 93/2,
40129
Bologna, Italy
20
Istituto Nazionale di Astrofisica (INAF) – Istituto di Radioastronomia (IRA),
via Gobetti 101,
40129
Bologna, Italy
21
Hamburger Sternwarte, Universität Hamburg,
Gojenbergsweg 112,
21029,
Hamburg, Germany
22
Astronomical Observatory of the Jagiellonian University,
ul. Orla 171,
30-244
Kraków, Poland
23
Thüringer Landessternwarte,
Sternwarte 5,
D-07778
Tautenburg, Germany
24
National Radio Astronomy Observatory,
520 Edgemont Road,
Charlottesville, VA
22903, USA
25
CSIRO Space & Astronomy,
PO Box 1130,
Bentley, WA
6102, Australia
26
Space Radio-Diagnostics Research Centre, University of Warmia and Mazury,
ul.Oczapowskiego 2,
10-719
Olsztyn, Poland
27
Institut für Theoretische Physik und Astrophysik, Universität Würzburg,
Emil-Fischer-Straße 31,
97074
Würzburg, Germany
28
Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, NCU,
Grudziadzka 5,
87-100
Toruń, Poland
29
School of Physical Sciences, The Open University,
Walton Hall,
Milton Keynes
MK7 6AA, UK
30
Centre for Extragalactic Astronomy, Department of Physics, Durham University,
Durham
DH1 3LE, UK
31
Institute for Computational Cosmology, Department of Physics, University of Durham,
South Road,
Durham
DH1 3LE, UK
32
Astronomy Department, Universidad de Concepción,
Casilla 160-C,
Concepción, Chile
33
Instituto de Astrofísica de Andalucía (IAA-CSIC),
Glorieta de la Astronomía s/n,
18008
Granada, Spain
34
Facultad de Ciencias, Universidad de Zaragoza,
Pedro Cerbuna 12,
50009
Zaragoza, Spain
35
School of Sciences, European University Cyprus,
Diogenes street, Engomi,
1516
Nicosia, Cyprus
36
Astronomy and Astrophysics Section, Dublin Institute for Advanced Studies,
31 Fitzwilliam Place,
Dublin
D02 XF86, Ireland
37
Anton Pannekoek Institute for Astronomy, University of Amsterdam,
Science Park 904,
1098 XH
Amsterdam, The Netherlands
38
Inter-University Institute for Data Intensive Astronomy, Department of Astronomy, University of Cape Town,
7701
Rondebosch, Cape Town, South Africa
39
Inter-University Institute for Data Intensive Astronomy, Department of Physics and Astronomy, University of the Western Cape,
7535
Bellville, Cape Town, South Africa
Received:
28
November
2022
Accepted:
17
December
2022
We present the detection of 68 sources from the most sensitive radio survey in circular polarisation conducted to date. We used the second data release of the 144 MHz LOFAR Two-metre Sky Survey to produce circularly polarised maps with a median noise of 140 µJy beam−1 and resolution of 20″ for ≈27% of the northern sky (5634 deg2). The leakage of total intensity into circular polarisation is measured to be ≈0.06%, and our survey is complete at flux densities ≥1 mJy. A detection is considered reliable when the circularly polarised fraction exceeds 1%. We find the population of circularly polarised sources is composed of four distinct classes: stellar systems, pulsars, active galactic nuclei, and sources unidentified in the literature. The stellar systems can be further separated into chromospherically active stars, M dwarfs, and brown dwarfs. Based on the circularly polarised fraction and lack of an optical counterpart, we show it is possible to infer whether the unidentified sources are likely unknown pulsars or brown dwarfs. By the completion of this survey of the northern sky, we expect to detect 300±100 circularly polarised sources.
Key words: surveys / catalogs / radio continuum: general / polarization
V-LoTSS catalogue is only available at the CDS via anonymous ftp to cdsarc.cds.unistra.fr (130.79.128.5) or via https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/670/A124
© The Authors 2023
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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