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V-LoTSS: The circularly polarised LOFAR Two-metre Sky Survey
| Indexado |
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| DOI | 10.1051/0004-6361/202245567 | ||||
| Año | 2023 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
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 beam1 and resolution of 203 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.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Callingham, J. | - |
Sterrewacht Leiden - Países Bajos
Netherlands Foundation for Research in Astronomy - Países Bajos Leiden Univ - Países Bajos ASTRON - Países Bajos |
| 2 | Shimwell, T. W. | - |
Sterrewacht Leiden - Países Bajos
Netherlands Foundation for Research in Astronomy - Países Bajos Leiden Univ - Países Bajos ASTRON - Países Bajos |
| 3 | Vedantham, H. K. | Hombre |
Netherlands Foundation for Research in Astronomy - Países Bajos
Kapteyn Instituut - Países Bajos ASTRON - Países Bajos Univ Groningen - Países Bajos |
| 4 | Bassa, C. G. | - |
Netherlands Foundation for Research in Astronomy - Países Bajos
ASTRON - Países Bajos |
| 5 | O'Sullivan, Shane P. | Hombre |
Dublin City University - Irlanda
Dublin City Univ - Irlanda |
| 6 | Yiu, T. W.H. | - |
Netherlands Foundation for Research in Astronomy - Países Bajos
Kapteyn Instituut - Países Bajos ASTRON - Países Bajos Univ Groningen - Países Bajos |
| 7 | Bloot, S. | - |
Netherlands Foundation for Research in Astronomy - Países Bajos
Kapteyn Instituut - Países Bajos ASTRON - Países Bajos Univ Groningen - Países Bajos |
| 8 | Best, P. N. | - |
University of Edinburgh, Institute for Astronomy - Reino Unido
|
| 9 | Hardcastle, M. J. | Hombre |
University of Hertfordshire - Reino Unido
Univ Hertfordshire - Reino Unido |
| 10 | Haverkorn, M. | - |
Radboud Universiteit - Países Bajos
Radboud Univ Nijmegen - Países Bajos |
| 11 | Kavanagh, R. D. | - |
Netherlands Foundation for Research in Astronomy - Países Bajos
ASTRON - Países Bajos |
| 12 | Lamy, L. | - |
L'Observatoire de Paris - Francia
Laboratoire d'Astrophysique de Marseille - Francia Univ PSL - Francia Aix Marseille Univ - Francia |
| 13 | Pope, B. J.S. | - |
The University of Queensland - Australia
University of Southern Queensland - Australia UNIV QUEENSLAND - Australia Univ Southern Queensland - Australia |
| 14 | Masip Macia, Yunesky | Hombre |
Sterrewacht Leiden - Países Bajos
Leiden Univ - Países Bajos |
| 15 | Schwarz, D. J. | - |
Universität Bielefeld - Alemania
Univ Bielefeld - Alemania |
| 16 | Tasse, C. | - |
L'Observatoire de Paris - Francia
Rhodes University - República de Sudáfrica Univ PSL - Francia Rhodes Univ - República de Sudáfrica |
| 17 | van Weeren, R. J. | Hombre |
Sterrewacht Leiden - Países Bajos
Leiden Univ - Países Bajos |
| 18 | White, Glenn J. | Hombre |
The Open University - Reino Unido
RAL Space - Reino Unido Open Univ - Reino Unido STFC Rutherford Appleton Lab - Reino Unido |
| 19 | Zarka, P. | - |
L'Observatoire de Paris - Francia
Universite d'Orleans - Francia Univ PSL - Francia Univ Orleans - Francia |
| 20 | Bomans, D. | - |
Ruhr-Universität Bochum - Alemania
Ruhr Univ Bochum RUB - Alemania |
| 21 | Bonafede, A. | Mujer |
Alma Mater Studiorum Università di Bologna - Italia
Istituto Di Radioastronomia, Bologna - Italia UNIV BOLOGNA - Italia |
| 22 | Bonato, M. | Hombre |
Istituto Di Radioastronomia, Bologna - Italia
Ist Radioastron IRA - Italia |
| 23 | Botteon, A. | - |
Alma Mater Studiorum Università di Bologna - Italia
Istituto Di Radioastronomia, Bologna - Italia Ist Radioastron IRA - Italia |
| 24 | Bruggen, M. | - |
Universität Hamburg - Alemania
UNIV HAMBURG - Alemania |
| 25 | Chyzy, K. T. | - |
Uniwersytet Jagiellonski - Polonia
Jagiellonian Univ - Polonia |
| 26 | Drabent, Alexander | - |
Thuringer Landessternwarte Tautenburg - Alemania
Thuringer Landessternwarte - Alemania |
| 27 | Emig, K. L. | Mujer |
National Radio Astronomy Observatory - Estados Unidos
Natl Radio Astron Observ - Estados Unidos |
| 28 | Gloudemans, A. J. | - |
Sterrewacht Leiden - Países Bajos
Leiden Univ - Países Bajos |
| 29 | Guerkan, G. | - |
Thuringer Landessternwarte - Alemania
CSIRO Space & Astron - Australia Thuringer Landessternwarte Tautenburg - Alemania Commonwealth Scientific and Industrial Research Organization - Australia Commonwealth Scientific and Industrial Research Organisation - Australia |
| 29 | Gürkan, G. | - |
Thuringer Landessternwarte Tautenburg - Alemania
Commonwealth Scientific and Industrial Research Organization - Australia |
| 30 | Hajduk, Marcin | Hombre |
Uniwersytet Warminsko-Mazurski w Olsztynie - Polonia
Univ Warm & Mazury - Polonia |
| 31 | Hoang, D. N. | - |
Universität Hamburg - Alemania
UNIV HAMBURG - Alemania |
| 32 | Hoeft, M. | - |
Thuringer Landessternwarte Tautenburg - Alemania
Thuringer Landessternwarte - Alemania |
| 33 | Iacobelli, M. | Hombre |
Netherlands Foundation for Research in Astronomy - Países Bajos
ASTRON - Países Bajos |
| 34 | Kadler, M. | Hombre |
Julius-Maximilians-Universität Würzburg - Alemania
UNIV WURZBURG - Alemania |
| 35 | Kunert-Bajraszewska, M. | - |
Uniwersytet Mikołaja Kopernika w Toruniu - Polonia
NCU - Polonia |
| 36 | Mingo, B. | - |
The Open University - Reino Unido
Open Univ - Reino Unido |
| 37 | Morabito, L. K. | - |
Durham University - Reino Unido
Univ Durham - Reino Unido |
| 38 | Nair, Dhanya G. | - |
Universidad de Concepción - Chile
|
| 39 | PEREZ-TORRES, MIGUEL ANGEL | Hombre |
Instituto de Astrofísica de Andalucía - CSIC - España
Universidad de Zaragoza - España European University Cyprus - Chipre Inst Astrofis Andalucia IAA CSIC - España UNIV ZARAGOZA - España European Univ Cyprus - Chipre CSIC - Instituto de Astrofísica de Andalucía (IAA) - España |
| 40 | Ray, Paul S. | Hombre |
Dublin Institute for Advanced Studies - Irlanda
Dublin Inst Adv Studies - Irlanda Institiúid Ard-Lénn Bhaile Átha Cliath - Irlanda |
| 41 | Riseley, C. | - |
Alma Mater Studiorum Università di Bologna - Italia
UNIV BOLOGNA - Italia |
| 42 | Rowlinson, A. | - |
Netherlands Foundation for Research in Astronomy - Países Bajos
Anton Pannekoek Instituut voor Sterrenkunde - Países Bajos |
| 43 | Le Brun, A. M. C. | - |
Sterrewacht Leiden - Países Bajos
Leiden Univ - Países Bajos |
| 44 | Sweijen, F. | - |
Sterrewacht Leiden - Países Bajos
Netherlands Foundation for Research in Astronomy - Países Bajos Leiden Univ - Países Bajos ASTRON - Países Bajos |
| 45 | Timmerman, R. | - |
Sterrewacht Leiden - Países Bajos
Leiden Univ - Países Bajos |
| 46 | Vaccari, M. | Hombre |
Istituto Di Radioastronomia, Bologna - Italia
Inter-university Institute for Data Intensive Astronomy - República de Sudáfrica Ist Radioastron IRA - Italia |
| 47 | Zheng, J. | - |
Universität Bielefeld - Alemania
Univ Bielefeld - Alemania |
| Fuente |
|---|
| Comisión Nacional de Investigación Científica y Tecnológica |
| Ministerio de Ciencia e Innovación |
| University of Pretoria |
| European Research Council |
| ERC |
| Science and Technology Facilities Council |
| Narodowe Centrum Nauki |
| UK STFC |
| NWO |
| National Science Centre, Poland |
| Leverhulme Trust |
| European Research Council (ERC) |
| Nederlandse Organisatie voor Wetenschappelijk Onderzoek |
| Bundesministerium für Bildung und Forschung |
| Agencia Estatal de Investigación |
| FONDECYT Postdoctorado |
| UK Research and Innovation |
| University of the Western Cape |
| Horizon 2020 Framework Programme |
| South African Radio Astronomy Observatory |
| ERC under the European Union's Horizon 2020 research and innovation programme |
| Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) |
| MSHE |
| Center of Excellence Severo Ochoa |
| Instituto de Astrofisica de Andalucia |
| University of Hertfordshire |
| UK Science and Technology Funding Council |
| German Science Foundation DFG |
| University of Cape Town |
| BMBF Verbundforschung |
| NWO Aspasia grant |
| CONICYT through FONDECYT POSTDOCTORADO |
| Inter-University Institute for Data Intensive Astronomy (IDIA) |
| UKRI Future Leaders Fellowship |
| Gauss Centre for Supercomputing e.V. through the John von Neumann Institute for Computing (NIC) |
| DSI-NRF |
| IDIA |
| CSUR |
| Inter-University Institute for Data Intensive Astronomy |
| EASY |
| EOSC |
| South African Department of Science and Innovation’s National Research Foundation |
| MIUR FARE |
| German Science Foundation DFG, via the Collaborative Research Center |
| South African Department of Science and Innovation's National Research Foundation under CSUR HIPPO Project (DSI-NRF Grant ) |
| EOSC Future - European Union's Horizon 2020 research and innovation programme |
| Spanish Ministerio de Ciencia e Innovacion (MCIN), the Agencia Estatal de Investigacion (AEI) through MCIN/AEI) |
| SURF Co-operative |
| UK Science and Technology Funding Council (STFC) |
| MIUR FARE grant "SMS" |
| South African Department of Science and Innovation's National Research Foundationunder the ISARP RADIOSKY2020 Joint Research Scheme (DSI-NRF Grant) |
| Spanish Ministerio de Ciencia e Innovacion (MCIN), the Agencia Estatal de Investigacion (AEI) through the "Center of Excellence Severo Ochoa" award |
| Agradecimiento |
|---|
| The LOFAR data in this manuscript were processed by the LOFAR Two-Metre Sky Survey (LoTSS) team. This team made use of the LOFAR direction-independent calibration pipeline ( https://github.com/lofar-astron/prefactor ), which was deployed by the LOFAR e-infragroup on the Dutch National Grid infrastructure with support of the SURF Co-operative through grants e-infra 160022 e-infra 160152 (Mechev et al. 2017). The LoTSS direction dependent calibration and imaging pipeline ( http://github.com/mhardcastle/ddf-pipeline/ ) was run on compute clusters at Leiden Observatory and the University of Hertfordshire, which are supported by a European Research Council (ERC) Advanced Grant [NEWCLUSTERS-321271] and the UK Science and Technology Funding Council (STFC) [ST/P000096/1]. The Jülich LOFAR Long Term Archive and the German LOFAR network are both coordinated and operated by the Jülich Supercomputing Centre (JSC), and computing resources on the supercomputer JUWELS at JSC were provided by the Gauss Centre for Supercomputing e.V. (grant CHTB00) through the John von Neumann Institute for Computing (NIC). J.R.C. thanks the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) for support via the Talent Programme Veni grant. H.K. and S.B. acknowledge funding from the NWO for the project e-MAPS (project number Vi.Vidi.203.093) under the NWO talent scheme VIDI. T.W.H.Y. acknowledges funding from EOSC Future (Grant Agreement no. 101017536) projects funded by the European Union’s Horizon 2020 research and innovation programme. P.N.B. is grateful for support from the UK STFC via grant ST/V000594/1. M.J.H. acknowledges support from the UK STFC [ST/V000624/1]. M.H. acknowledges funding from the ERC under the European Union’s Horizon 2020 research and innovation programme (grant agreement no. 772663). R.J.v.W. and R.T. acknowledge support from the ERC Starting Grant ClusterWeb 804208. G.J.W. gratefully acknowledges the support of an Emeritus Fellowship from The Leverhulme Trust. D.J.B. acknowledges funding from the German Science Foundation DFG, via the Collaborative Research Center SFB1491 “Cosmic Interacting Matters – From Source to Signal”. A. Bonafede, A. Botteon, D.N.H., and C.J.R. acknowledge support from ERC Stg DRA-NOEL n. 714245 and MIUR FARE grant “SMS”. A.D. acknowledges support by the BMBF Verbundforschung under the grant 05A20STA. K.L.E. is a Jan-sky Fellow of the National Radio Astronomy Observatory. M. Haj and K.C.H. acknowledge the MSHE for granting funds for the Polish contribution to the International LOFAR Telescope (MSHE decision no. DIR/WK/2016/2017/05-1) and for maintenance of the LOFAR PL-612 Baldy (MSHE decision no. 59/E-383/SPUB/SP/2019.1), and LOFAR PL-611 Lazy (MSHE decision no. 46/E-338/SPUB/SP/2019). M.K. acknowledges support from the German Science Foundation DFG, via the Research Unit FOR 5195 “Relativistic Jets in Active Galaxies”. M.K.B. acknowledges support from the National Science Centre, Poland under grant no. 2017/26/E/ST9/00216. B.M. acknowledges support from the UK STFC under grants ST/R00109X/1, ST/R000794/1, and ST/T000295/1. L.K.M. is grateful for support from the UKRI Future Leaders Fellowship (grant MR/T042842/1). D.G.N. acknowledges funding from Conicyt through Fondecyt Postdoctorado (project code 3220195). M.P.T. acknowledges financial support from the Spanish Ministerio de Ciencia e Innovación (MCIN), the Agencia Estatal de Investigación (AEI) through the “Center of Excellence Severo Ochoa” award to the Instituto de Astrofísica de Andalucía (SEV-2017-0709) and through grant PID2020-117404GB-C21 funded by MCIN/AEI/10.13039/501100011033. T.P.R. acknowledges support from the ERC Grant No. 743029 (EASY). A.R. acknowledges funding from the NWO Aspasia grant (number: 015.016.033). M.V. acknowledges financial support from the Inter-University Institute for Data Intensive Astronomy (IDIA), a partnership of the University of Cape Town, the University of Pretoria, the University of the Western Cape and the South African Radio Astronomy Observatory, and from the South African Department of Science and Innovation’s National Research Foundation under the ISARP RADIOSKY2020 Joint Research Scheme (DSI-NRF Grant Number 113121) and the CSUR HIPPO Project (DSI-NRF Grant Number 121291). This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France, and NASA’s Astrophysics Data System. This work has also made use of TOPCAT (Taylor 2005); the IP YTHON package (Pérez & Granger 2007); SciPy (Jones et al. 2001); MATPLOTLIB , a P YTHON library for publication quality graphics (Hunter 2007); A STROPY , a community-developed core P YTHON package for astronomy (Astropy Collaboration 2013); and N UM P Y (Van Der Walt et al. 2011). |
| acknowledges financial support from the Spanish Ministerio de Ciencia e Innovacion (MCIN), the Agencia Estatal de Investigacion (AEI) through the "Center of Excellence Severo Ochoa" award to the Instituto de Astrofisica de Andalucia (SEV-2017-0709) and through grant PID2020-117404GB-C21 funded by MCIN/AEI/10.13039/501100011033. T.P.R. acknowledges support from the ERC Grant No. 743029 (EASY). A.R. acknowledges funding from the NWO Aspasia grant (number: 015.016.033). M.V. acknowledges financial support from the Inter-University Institute for Data Intensive Astronomy (IDIA), a partnership of the University of Cape Town, the University of Pretoria, the University of the Western Cape and the South African Radio Astronomy Observatory, and from the South African Department of Science and Innovation's National Research Foundation under the ISARP RADIOSKY2020 Joint Research Scheme (DSI-NRF Grant Number 113121) and the CSUR HIPPO Project (DSI-NRF Grant Number 121291). This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France, and NASA's Astrophysics Data System. This work has also made use of TOPCAT (Taylor 2005); the IPYTHON package (Perez & Granger 2007); SciPy (Jones et al. 2001); MATPLOTLIB, a PYTHON library for publication quality graphics (Hunter 2007); ASTROPY, a community-developed core PYTHON package for astronomy (Astropy Collaboration 2013); and NUMPY (Van Der Walt et al. 2011). |
