4.7 Article

CFHTLenS: the Canada-France-Hawaii Telescope Lensing Survey - imaging data and catalogue products

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stt928

关键词

methods: data analysis; cosmology: observations

资金

  1. Deutsche Forschungsgemeinschaft [ER 327/3-1]
  2. Transregional Collaborative Research Centre [TR 33]
  3. CITA National Fellowship [Marie Curie IOF 252760]
  4. DFG [Hi 1495/2-1]
  5. Natural Sciences and Engineering Research Council of Canada (NSERC)
  6. Canadian Institute for Advanced Research (CIfAR)
  7. European Research Council under the EC [240185, 279396]
  8. Marie Curie IRG grant [230924]
  9. Netherlands Organisation for Scientific Research (NWO) [639.042.814]
  10. Royal Society University Research Fellowship
  11. CNRS/Institut National des Sciences de l'Univers (INSU)
  12. Programme National Galaxies et Cosmologie (PNCG)
  13. Spanish Science Ministry [AYA2009-13936 Consolider-Ingenio CSD2007-00060]
  14. Generalitat de Catalunya [2009SGR1398]
  15. European Commissions Marie Curie Initial Training Network CosmoComp [PITN-GA-2009-238356]
  16. NSFC [11103012, 10878003, 12ZZ134]
  17. SMEC [10CG46]
  18. STCSM grant [11290706600]
  19. Research council of Norway [177254/V30]
  20. DFG cluster of excellence 'Origin and Structure of the Universe'
  21. European Research Council [24067]
  22. NSF [AST-0444059-001, GO0-11147A]
  23. Netherlands Organization for Scientific Research (NWO)
  24. Beecroft Institute for Particle Astrophysics and Cosmology
  25. European Research Council (ERC) [240185] Funding Source: European Research Council (ERC)
  26. STFC [ST/J001422/1, ST/H002456/1] Funding Source: UKRI
  27. Science and Technology Facilities Council [ST/J001422/1, ST/H002456/1] Funding Source: researchfish

向作者/读者索取更多资源

We present data products from the Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS). CFHTLenS is based on the Wide component of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS). It encompasses 154 deg(2) of deep, optical, high-quality, sub-arcsecond imaging data in the five optical filters u*g(')r(')i(')z('). The scientific aims of the CFHTLenS team are weak gravitational lensing studies supported by photometric redshift estimates for the galaxies. This paper presents our data processing of the complete CFHTLenS data set. We were able to obtain a data set with very good image quality and high-quality astrometric and photometric calibration. Our external astrometric accuracy is between 60 and 70 mas with respect to Sloan Digital Sky Survey (SDSS) data, and the internal alignment in all filters is around 30 mas. Our average photometric calibration shows a dispersion of the order of 0.01-0.03 mag for g(')r(')i(')z(') and about 0.04 mag for u* with respect to SDSS sources down to i(SDSS) < 21. We demonstrate in accompanying papers that our data meet necessary requirements to fully exploit the survey for weak gravitational lensing analyses in connection with photometric redshift studies. In the spirit of the CFHTLS, all our data products are released to the astronomical community via the Canadian Astronomy Data Centre at ext-link-type=uri xlink:href=http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/community/CFHTLens/query.html xmlns:xlink=http://www.w3.org/1999/xlink>http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/community/CFHTLens/query.html. We give a description and how-to manuals of the public products which include image pixel data, source catalogues with photometric redshift estimates and all relevant quantities to perform weak lensing studies.

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