4.6 Article

The LOFAR Two-metre Sky Survey V. Second data release

期刊

ASTRONOMY & ASTROPHYSICS
卷 659, 期 -, 页码 -

出版社

EDP SCIENCES S A
DOI: 10.1051/0004-6361/202142484

关键词

surveys; catalogs; radio continuum: general; techniques: image processing

资金

  1. CNRS-INSU, France
  2. Observatoire de Paris, France
  3. Universite d'Orleans, France
  4. BMBF, Germany
  5. MIWF-NRW, Germany
  6. MPG, Germany
  7. Science Foundation Ireland (SFI), Department of Business, Enterprise and Innovation (DBEI), Ireland
  8. NWO, The Netherlands
  9. Science and Technology Facilities Council, UK
  10. Ministry of Science and Higher Education, Poland
  11. Istituto Nazionale di Astrofisica (INAF), Italy
  12. SURF Cooperative [e-infra 180169]
  13. NWO [2019.056]
  14. Gauss Centre for Supercomputing e.V. through the John von Neumann Institute for Computing (NIC) [CHTB00]
  15. STFC [ST/P000096/1, ST/R000905/1, ST/V000624/1]
  16. Italian LOFAR IT
  17. EU [101017207]
  18. UK STFC [ST/R000972/1, ST/V000594/1]
  19. CAS-NWO programme for radio astronomy - Netherlands Organisation for Scientific Research (NWO) [629.001.024]
  20. VIDI research programme - Netherlands Organisation for Scientific Research (NWO) [639.042.729]
  21. BMBF Verbundforschung [05A20STA, 05A20PB1, 05A20PC3, 50OR1906]
  22. ERC Starting Grant ClusterWeb [804208]
  23. Deutsche Forschungsgemeinschaft under Germany's Excellence Strategy [EXC 2121, 390833306]
  24. European Union's Horizon 2020 research and innovation programme under the Marie Skodowska-Curie grant [892117]
  25. Leverhulme Trust through an Early Career Research Fellowship
  26. European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme [772663]
  27. UKRI Future Leaders Fellowship [MR/T042842/1]
  28. South African Research Chairs Initiative of the Department of Science and Technology
  29. National Research Foundation
  30. Emeritus Fellowship from the Leverhulme Trust
  31. STFC through a ScotDIST Intensive Data Science Scholarship
  32. ERC Stg 'DRANOEL' [714245]
  33. MIUR FARE grant SMS
  34. ERC-Stg grant 'DRANOEL'
  35. ERC Stg MAGCOW [714196]
  36. Polish National Science Center [2020/38/E/ST9/00395, 2018/30/E/ST9/00698, 2018/31/G/ST9/03388]
  37. Polish Ministry of Science and Higher Education [DIR/WK/2018/12]
  38. INAF under the SKA/CTA PRIN FORECaST
  39. INAF under PRIN MAIN STREAM SAuROS project
  40. Ministero degli Affari Esteri e della Cooperazione Internazionale - Direzione Generale per la Promozione del Sistema Paese Progetto di Grande Rilevanza [ZA18GR02]
  41. Alexander von Humboldt Foundation
  42. UK Science and Technology Facilities Council (STFC) [ST/R00109X/1, ST/R000794/1, ST/T000295/1]
  43. DFG [427771150]
  44. MSHE [DIR/WK/2016/2017/05-1, 59/E-383/SPUB/SP/2019.1]
  45. NAWA Bekker fellowship [PPN/BEK/2019/1/00431]
  46. ERC through the grant ERC-Stg 'DRANOEL' [714245]
  47. Croatian Science Foundation [IP-2018-01-2889]
  48. Science and Technology Facilities Council (STFC) [ST/R504737/1]
  49. National Science Centre, Poland [2017/26/E/ST9/00216]
  50. National Science Centre [UMO-2018/30/E/ST9/00082]
  51. Departments of Excellence 2018 - 2022 Grant - Italian Ministry of Education, University and Research (MIUR) [L. 232/2016]
  52. ERC Starting Grant MAGCOW [714196]
  53. ERC Starting Grant 'DRANOEL' [714245]
  54. Inter-University Institute for Data Intensive Astronomy (IDIA)
  55. University of Cape Town
  56. University of Pretoria
  57. University of the Western Cape
  58. South African Radio Astronomy Observatory
  59. South African Department of Science and Innovation's National Research Foundation under the ISARP RADIOSKY2020 Joint Research Scheme (DSI-NRF Grant) [113121]
  60. CSUR HIPPO Project (DSI-NRF Grant) [121291]
  61. China Scholarship Council
  62. David Dunlap family
  63. University of Toronto
  64. Natural Sciences and Engineering Research Council of Canada (NSERC) [RGPIN-2015-05948]
  65. Canada Research Chairs program
  66. European Research Council (ERC) [714245] Funding Source: European Research Council (ERC)

向作者/读者索取更多资源

This article presents the data release of LOFAR Two-metre Sky Survey, which covers 27% of the northern sky with 120-168 MHz images. The catalogue includes 4,396,228 radio sources, most of which have never been detected at radio wavelengths before. The images were derived from extensive and automated data processing, including correction for instrumental properties and ionospheric distortions. The release of Stokes I, Q, U, and V images, as well as calibrated uv-data, enables the thorough scientific exploitation of this unique dataset.
In this data release from the ongoing LOw-Frequency ARray (LOFAR) Two-metre Sky Survey we present 120-168 MHz images covering 27% of the northern sky. Our coverage is split into two regions centred at approximately 12h45m +44 degrees 30' and 1h00m +28 degrees 00' and spanning 4178 and 1457 square degrees respectively. The images were derived from 3451 h (7.6 PB) of LOFAR High Band Antenna data which were corrected for the direction-independent instrumental properties as well as direction-dependent ionospheric distortions during extensive, but fully automated, data processing. A catalogue of 4 396 228 radio sources is derived from our total intensity (Stokes I) maps, where the majority of these have never been detected at radio wavelengths before. At 6 '' resolution, our full bandwidth Stokes I continuum maps with a central frequency of 144 MHz have: a median rms sensitivity of 83 mu Jy beam(-1); a flux density scale accuracy of approximately 10%; an astrometric accuracy of 0.2 ''; and we estimate the point-source completeness to be 90% at a peak brightness of 0.8 mJy beam(-1). By creating three 16 MHz bandwidth images across the band we are able to measure the in-band spectral index of many sources, albeit with an error on the derived spectral index of > +/- 0.2 which is a consequence of our flux-density scale accuracy and small fractional bandwidth. Our circular polarisation (Stokes V) 20 '' resolution 120-168 MHz continuum images have a median rms sensitivity of 95 mu Jy beam(-1), and we estimate a Stokes Ito Stokes V leakage of 0.056%. Our linear polarisation (Stokes Q and Stokes U) image cubes consist of 480 x 97.6 kHz wide planes and have a median rms sensitivity per plane of 10.8 mu Jy beam(-1) at 4' and 2.2 mu Jy beam(-1) at 20 ''; we estimate the Stokes I to Stokes Q/U leakage to be approximately 0.2%. Here we characterise and publicly release our Stokes I, Q, U and V images in addition to the calibrated uv-data to facilitate the thorough scientific exploitation of this unique dataset.

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