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The LOFAR Two-metre Sky Survey: Deep Fields Data Release 2 I. The ELAIS-N1 field
Indexado
WoS WOS:001439267100011
Scopus SCOPUS_ID:86000621041
DOI 10.1051/0004-6361/202452930
Año 2025
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



We present the final 6 '' resolution data release of the ELAIS-N1 field from the LOw-Frequency ARray (LOFAR) Two-metre Sky Survey Deep Fields project (LoTSS Deep). The 144 MHz images are the most sensitive achieved to date at this frequency and were created from 290 TB of data obtained from 505 h on-source observations taken over 7.5 years. The data were processed following the strategies developed for previous LoTSS and LoTSS Deep data releases. The resulting images span 24.53 square degrees, and using a refined source detection approach, we identified 154 952 radio sources formed from 182 184 Gaussian components within this area. The maps reach a noise level of 10.7 mu Jy beam(-1) at 6 '' resolution, where approximately half of the noise is due to source confusion. In about 7.4% of the image, our limited dynamic range around bright sources results in a further > 5% increase in the noise. The images have a flux density scale accuracy of about 9%, and the standard deviation of offsets between our source positions and those from Pan-STARRS is 0.2 '' in RA and Dec for high significance detections. We searched individual epoch images for variable sources, identifying 39 objects with considerable variation. We also searched for circularly polarised sources, achieving three detections of previously known emitters (two stars and one pulsar) whilst constraining the typical polarisation fraction plus leakage to be less than 0.045%.

Revista



Revista ISSN
Astronomy & Astrophysics 0004-6361

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Shimwell, T. W. - ASTRON - Países Bajos
Leiden Univ - Países Bajos
Netherlands Foundation for Research in Astronomy - Países Bajos
Sterrewacht Leiden - Países Bajos
2 Hale, C. L. - UNIV OXFORD - Reino Unido
UNIV EDINBURGH - Reino Unido
University of Oxford - Reino Unido
University of Edinburgh, Institute for Astronomy - Reino Unido
3 Best, P. N. - UNIV EDINBURGH - Reino Unido
University of Edinburgh, Institute for Astronomy - Reino Unido
4 Botteon, A. - INAF Ist Radioastron - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia
5 Drabent, Alexander - Thuringer Landessternwarte - Alemania
Thuringer Landessternwarte Tautenburg - Alemania
6 Hardcastle, M. J. - Univ Hertfordshire - Reino Unido
University of Hertfordshire - Reino Unido
7 Jelic, V. - Rudjer Boskovic Inst - Croacia
Institut Ruđer Bošković - Croacia
8 de Jong, J. M. G. H. J. - Leiden Univ - Países Bajos
Sterrewacht Leiden - Países Bajos
9 Kondapally, R. - UNIV EDINBURGH - Reino Unido
University of Edinburgh, Institute for Astronomy - Reino Unido
10 Roettgering, H. J. A. - Leiden Univ - Países Bajos
10 Röttgering, H. J.A. - Sterrewacht Leiden - Países Bajos
11 Tasse, C. - Univ PSL - Francia
Rhodes Univ - República de Sudáfrica
GEPI - Galaxies, Etoiles, Physique, Instrumentation - Francia
Rhodes University - República de Sudáfrica
12 van Weeren, R. J. - Leiden Univ - Países Bajos
Sterrewacht Leiden - Países Bajos
13 Williams, W. L. - Jodrell Bank - Reino Unido
SKA Organisation, UK - Reino Unido
14 Bonafede, A. Mujer INAF Ist Radioastron - Italia
UNIV BOLOGNA - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia
Alma Mater Studiorum Università di Bologna - Italia
15 Bondi, M. - INAF Ist Radioastron - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia
16 Brüggen, M. - Universität Hamburg - Alemania
16 Brueggen, M. - UNIV HAMBURG - Alemania
Universität Hamburg - Alemania
17 Brunetti, G. - INAF Ist Radioastron - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia
18 Callingham, J. R. - ASTRON - Países Bajos
Leiden Univ - Países Bajos
Netherlands Foundation for Research in Astronomy - Países Bajos
Sterrewacht Leiden - Países Bajos
19 De Gasperin, F. - INAF Ist Radioastron - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia
20 Duncan, K. J. - UNIV EDINBURGH - Reino Unido
University of Edinburgh, Institute for Astronomy - Reino Unido
21 Horellou, C. - Chalmers Univ Technol - Suecia
Onsala Space Observatory - Suecia
22 Iyer, S. - Univ Amsterdam - Países Bajos
Anton Pannekoek Instituut voor Sterrenkunde - Países Bajos
23 de Ruiter, I. - Univ Amsterdam - Países Bajos
Anton Pannekoek Instituut voor Sterrenkunde - Países Bajos
24 Malek, K. Mujer Natl Ctr Nucl Res - Polonia
National Centre for Nuclear Research (NCBJ) - Polonia
25 Nair, D. G. - Universidad de Concepción - Chile
Max Planck Inst Radio Astron - Alemania
Max Planck Institute for Radio Astronomy - Alemania
26 Morabito, L. K. - Univ Durham - Reino Unido
Durham University - Reino Unido
27 Prandoni, I. - INAF Ist Radioastron - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna - Italia
28 Rowlinson, A. - ASTRON - Países Bajos
Univ Amsterdam - Países Bajos
Netherlands Foundation for Research in Astronomy - Países Bajos
Anton Pannekoek Instituut voor Sterrenkunde - Países Bajos
29 Sabater, J. Hombre
30 Le Brun, A. M. C. - ASTRON - Países Bajos
Univ Amsterdam - Países Bajos
Univ Groningen - Países Bajos
Netherlands Foundation for Research in Astronomy - Países Bajos
Anton Pannekoek Instituut voor Sterrenkunde - Países Bajos
Kapteyn Instituut - Países Bajos
31 Smith, D. J. B. - Univ Hertfordshire - Reino Unido
University of Hertfordshire - Reino Unido
32 Sweijen, F. - Univ Durham - Reino Unido
Durham University - Reino Unido

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento



Fuente
Comisión Nacional de Investigación Científica y Tecnológica
European Commission
Deutsche Forschungsgemeinschaft
European Research Council
DFG
Iran Nanotechnology Initiative Council
STFC
Science and Technology Facilities Council
INAF
UK STFC
Max-Planck-Gesellschaft
NWO
Science Foundation Ireland
BMBF, Germany
MPG, Germany
NWO, The Netherlands
UK Science and Technology Facilities Council (STFC)
Leverhulme Trust
Nederlandse Organisatie voor Wetenschappelijk Onderzoek
Bundesministerium für Bildung und Forschung
FONDECYT Postdoctorado
UK Research and Innovation
STFC through an Ernest Rutherford Fellowship
ERC consolidator grant
Istituto Nazionale di Astrofisica
Gauss Centre for Supercomputing
Universite d'Orleans, France
Science and Technology Facilities Council, UK
Observatoire de Paris, France
CNRS-INSU, France
MIWF-NRW, Germany
University of Hertfordshire
Oxford Hintze Centre for Astrophysical Surveys from the Hintze Family Charitable Foundation
Ministry of Science and Higher Education, Poland
Hintze Family Charitable Foundation
Institut National des Sciences de l'Univers
John von Neumann Institute for Computing
NWO Aspasia grant
Consorzio Interuniversitario per la Fisica Spaziale
Ministry of Science and Higher Education of the Russian Federation
SURF
CONICYT through FONDECYT POSTDOCTORADO
DBEI
ERC Starting Grant ClusterWeb
Department of Business, Enterprise and Innovation
Physics Department of Turin university at the C3S Supercomputing Centre, Italy
LOFAR
Jülich Supercomputing Centre, Forschungszentrum Jülich
European Union - Next Generation EU
Dipartimento di Fisica, Università degli Studi di Torino
Science Foundation Ireland (SFI), Department of Business, Enterprise and Innovation (DBEI), Ireland
MIWF-NRW
UKRI FLF
LOFAR-ERIC
John von Neumann Institute for Computing (NIC)
NWA CORTEX grant - Dutch Research Council (NWO)
NWA-ORC
Anton Pannekoek Institute for Astronomy

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
This paper is based (in part) on data obtained with the LOFAR telescope (LOFAR-ERIC) under project code LC2_024, LC4_008, LT10_012 and LT14_003. LOFAR (van Haarlem et al. 2013) is the Low Frequency Array designed and constructed by ASTRON. It has observing, data processing, and data storage facilities in several countries, that are owned by various parties (each with their own funding sources), and that are collectively operated by the LOFAR European Research Infrastructure Consortium (LOFAR-ERIC) under a joint scientific policy. The LOFAR-ERIC resources have benefited from the following recent major funding sources: CNRS-INSU, Observatoire de Paris and Universite d'Orleans, France; BMBF, MIWF-NRW, MPG, Germany; Science Foundation Ireland (SFI), Department of Business, Enterprise and Innovation (DBEI), Ireland; NWO, The Netherlands; The Science and Technology Facilities Council, UK; Ministry of Science and Higher Education, Poland. This research made use of the Dutch national e-infrastructure with support of the SURF Cooperative (e-infra 180169) and NWO (grants 2019.056 & 2023.036). The Juelich LOFAR Long Term Archive and the German LOFAR network are both coordinated and operated by the Juelich 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). This research made use of the University of Hertfordshire high-performance computing facility and the LOFAR-UK computing facility located at the University of Hertfordshire and supported by STFC [ST/P000096/1], and of the Italian LOFAR IT computing infrastructure supported and operated by INAF, and by the Physics Department of Turin university (under an agreement with Consorzio Interuniversitario per la Fisica Spaziale) at the C3S Supercomputing Centre, Italy. CLH acknowledges support from the Leverhulme Trust through an Early Career Research Fellowship. CLH also acknowledges support from the Oxford Hintze Centre for Astrophysical Surveys which is funded through generous support from the Hintze Family Charitable Foundation. PNB and RK are grateful for support from the UK STFC via grants ST/V000594/1 and ST/Y000951/1. AB acknowledges financial support from the European Union - Next Generation EU. MJH and DJBS acknowledge support from the UK Science and Technology Facilities Council (STFC) via grants ST/V000624/1 and ST/Y001249/1. RJvW acknowledges support from the ERC Starting Grant ClusterWeb 804208. MB acknowledges funding by the DFG under Germany's Excellence Strategy - EXC 2121 "Quantum Universe" - 390833306. FdG acknowledges support from the ERC Consolidator Grant ULU 101086378. KJD acknowledges support from the STFC through an Ernest Rutherford Fellowship (grant number ST/W003120/1). SI acknowledges the ASPIRE programme at the Anton Pannekoek Institute for Astronomy. IdR and AR acknowledge support from the NWO Aspasia grant (number 015.016.033). IdR, AR, and JMGHJdJ acknowledge support from the NWA CORTEX grant (NWA.1160.18.316) of the research programme NWA-ORC which is (partly) financed by the Dutch Research Council (NWO). D.G.N. acknowledges funding from Conicyt through Fondecyt Postdoctorado (project code 3220195). LKM is grateful for support from a UKRI FLF [MR/T042842/1]. IP acknowledges support from INAF under the Large Grant 2022 funding scheme (project "MeerKAT and LOFAR Team up: a Unique Radio Window on Galaxy/AGN co-Evolution"). FS appreciates the support of STFC [ST/Y004159/1].
This paper is based (in part) on data obtained with the LOFAR telescope (LOFAR-ERIC) under project code LC2-024, LC4-008, LT10-012 and LT14-003. LOFAR (van Haarlem et al. 2013) is the Low Frequency Array designed and constructed by ASTRON. It has observing, data processing, and data storage facilities in several countries, that are owned by various parties (each with their own funding sources), and that are collectively operated by the LOFAR European Research Infrastructure Consortium (LOFAR-ERIC) under a joint scientific policy. The LOFAR-ERIC resources have benefited from the following recent major funding sources: CNRS-INSU, Observatoire de Paris and Universit\u00E9 d'Orl\u00E9ans, France; BMBF, MIWF-NRW, MPG, Germany; Science Foundation Ireland (SFI), Department of Business, Enterprise and Innovation (DBEI), Ireland; NWO, The Netherlands; The Science and Technology Facilities Council, UK; Ministry of Science and Higher Education, Poland. This research made use of the Dutch national e-infrastructure with support of the SURF Cooperative (e-infra 180169) and NWO (grants 2019.056 & 2023.036). The J\u00FClich LOFAR Long Term Archive and the German LOFAR network are both coordinated and operated by the J\u00FClich 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). This research made use of the University of Hertfordshire high-performance computing facility and the LOFARUK computing facility located at the University of Hertfordshire and supported by STFC [ST/P000096/1], and of the Italian LOFAR IT computing infrastructure supported and operated by INAF, and by the Physics Department of Turin university (under an agreement with Consorzio Interuniversitario per la Fisica Spaziale) at the C3S Supercomputing Centre, Italy. CLH acknowledges support from the Leverhulme Trust through an Early Career Research Fellowship. CLH also acknowledges support from the Oxford Hintze Centre for Astrophysical Surveys which is funded through generous support from the Hintze Family Charitable Foundation. PNB and RK are grateful for support from the UK STFC via grants ST/V000594/1 and ST/Y000951/1. AB acknowledges financial support from the European Union - Next Generation EU. MJH and DJBS acknowledge support from the UK Science and Technology Facilities Council (STFC) via grants ST/V000624/1 and ST/Y001249/1. RJvW acknowledges support from the ERC Starting Grant ClusterWeb 804208. MB acknowledges funding by the DFG under Germany's Excellence Strategy - EXC 2121 \"Quantum Universe\" - 390833306. FdG acknowledges support from the ERC Consolidator Grant ULU 101086378. KJD acknowledges support from the STFC through an Ernest Rutherford Fellowship (grant number ST/W003120/1). SI acknowledges the ASPIRE programme at the Anton Pannekoek Institute for Astronomy. IdR and AR acknowledge support from the NWO Aspasia grant (number 015.016.033). IdR, AR, and JMGHJdJ acknowledge support from the NWA CORTEX grant (NWA.1160.18.316) of the research programme NWA-ORC which is (partly) financed by the Dutch Research Council (NWO). D.G.N. acknowledges funding from Conicyt through Fondecyt Postdoctorado (project code 3220195). LKM is grateful for support from a UKRI FLF [MR/T042842/1]. IP acknowledges support from INAF under the Large Grant 2022 funding scheme (project \"MeerKAT and LOFAR Team up: a Unique Radio Window on Galaxy/AGN co-Evolution\"). FS appreciates the support of STFC [ST/Y004159/1].
This paper is based (in part) on data obtained with the LOFAR telescope (LOFAR-ERIC) under project code LC2-024, LC4-008, LT10-012 and LT14-003. LOFAR (van Haarlem et al. 2013) is the Low Frequency Array designed and constructed by ASTRON. It has observing, data processing, and data storage facilities in several countries, that are owned by various parties (each with their own funding sources), and that are collectively operated by the LOFAR European Research Infrastructure Consortium (LOFAR-ERIC) under a joint scientific policy. The LOFAR-ERIC resources have benefited from the following recent major funding sources: CNRS-INSU, Observatoire de Paris and Universit\u00E9 d'Orl\u00E9ans, France; BMBF, MIWF-NRW, MPG, Germany; Science Foundation Ireland (SFI), Department of Business, Enterprise and Innovation (DBEI), Ireland; NWO, The Netherlands; The Science and Technology Facilities Council, UK; Ministry of Science and Higher Education, Poland. This research made use of the Dutch national e-infrastructure with support of the SURF Cooperative (e-infra 180169) and NWO (grants 2019.056 & 2023.036). The J\u00FClich LOFAR Long Term Archive and the German LOFAR network are both coordinated and operated by the J\u00FClich 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). This research made use of the University of Hertfordshire high-performance computing facility and the LOFARUK computing facility located at the University of Hertfordshire and supported by STFC [ST/P000096/1], and of the Italian LOFAR IT computing infrastructure supported and operated by INAF, and by the Physics Department of Turin university (under an agreement with Consorzio Interuniversitario per la Fisica Spaziale) at the C3S Supercomputing Centre, Italy. CLH acknowledges support from the Leverhulme Trust through an Early Career Research Fellowship. CLH also acknowledges support from the Oxford Hintze Centre for Astrophysical Surveys which is funded through generous support from the Hintze Family Charitable Foundation. PNB and RK are grateful for support from the UK STFC via grants ST/V000594/1 and ST/Y000951/1. AB acknowledges financial support from the European Union - Next Generation EU. MJH and DJBS acknowledge support from the UK Science and Technology Facilities Council (STFC) via grants ST/V000624/1 and ST/Y001249/1. RJvW acknowledges support from the ERC Starting Grant ClusterWeb 804208. MB acknowledges funding by the DFG under Germany's Excellence Strategy - EXC 2121 \"Quantum Universe\" - 390833306. FdG acknowledges support from the ERC Consolidator Grant ULU 101086378. KJD acknowledges support from the STFC through an Ernest Rutherford Fellowship (grant number ST/W003120/1). SI acknowledges the ASPIRE programme at the Anton Pannekoek Institute for Astronomy. IdR and AR acknowledge support from the NWO Aspasia grant (number 015.016.033). IdR, AR, and JMGHJdJ acknowledge support from the NWA CORTEX grant (NWA.1160.18.316) of the research programme NWA-ORC which is (partly) financed by the Dutch Research Council (NWO). D.G.N. acknowledges funding from Conicyt through Fondecyt Postdoctorado (project code 3220195). LKM is grateful for support from a UKRI FLF [MR/T042842/1]. IP acknowledges support from INAF under the Large Grant 2022 funding scheme (project \"MeerKAT and LOFAR Team up: a Unique Radio Window on Galaxy/AGN co-Evolution\"). FS appreciates the support of STFC [ST/Y004159/1].

Muestra la fuente de financiamiento declarada en la publicación.