4.6 Article

Planck 2015 results II. Low Frequency Instrument data processings

期刊

ASTRONOMY & ASTROPHYSICS
卷 594, 期 -, 页码 -

出版社

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201525818

关键词

space vehicles: instruments; methods: data analysis; cosmic background radiation

资金

  1. ESA
  2. CNES (France)
  3. CNRS/INSU-IN2P3-INP (France)
  4. ASI (Italy)
  5. CNR (Italy)
  6. INAF (Italy)
  7. NASA (USA)
  8. DoE (USA)
  9. STFC (UK)
  10. UKSA (UK)
  11. CSIC (Spain)
  12. MINECO (Spain)
  13. JA (Spain)
  14. RES (Spain)
  15. Tekes (Finland)
  16. AoF (Finland)
  17. CSC (Finland)
  18. DLR (Germany)
  19. MPG (Germany)
  20. CSA (Canada)
  21. DTU Space (Denmark)
  22. SER/SSO (Switzerland)
  23. RCN (Norway)
  24. SFI (Ireland)
  25. FCT/MCTES (Portugal)
  26. ERC (EU)
  27. PRACE (EU)
  28. Science and Technology Facilities Council [ST/L000768/1, ST/L000393/1, ST/K002821/1, ST/F010885/1] Funding Source: researchfish
  29. UK Space Agency [ST/N001095/1, ST/H001212/1] Funding Source: researchfish

向作者/读者索取更多资源

We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our results and methods have remained unchanged since the 2013 paper and we highlight the changes made for the 2015 release, describing the products (especially timelines) and the ways in which they were obtained. We demonstrate that the pipeline is self-consistent (principally based on simulations) and report all null tests. For the first time, we present LFI maps in Stokes Q and U polarization. We refer to other related papers where more detailed descriptions of the LFI data processing pipeline may be found if needed.

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