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| 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
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%.
| 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 |
| 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 |
| 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]. |