4.7 Article

RoboPol: a four-channel optical imaging polarimeter

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 485, Issue 2, Pages 2355-2366

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz557

Keywords

instrumentation: polarimeters; techniques: polarimetric

Funding

  1. 'RoboPol' project under the 'Aristeia' Action of the 'Operational Programme Education and Lifelong Learning'
  2. European Social Fund (ESF)
  3. Greek National Resources
  4. European Comission [PCIG10-GA-2011-304001 'JetPop', PIRSES-GA-2012-31578 'EuroCal']
  5. NASA [NNX11A043G]
  6. NSF [AST-1109911]
  7. Polish National Science Centre [2011/01/B/ST9/04618, 2017/25/B/ST9/02805]
  8. European Commission Seventh Framework Programme (FP7) through the Marie Curie Career Integration Grant [PCIG-GA-2011-293531 'SFOnset']
  9. National Science Foundation [AST-1611547]
  10. European Research Counsil under the European Union's Horizon 2020 research and innovation programme [771282]
  11. International Fulbright Science and Technology Award
  12. International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the University of Bonn
  13. International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the University of Cologne
  14. Academy of Finland [317383]

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We present the design and performance of RoboPol, a four-channel optical polarimeter operating at the Skinakas Observatory in Crete, Greece. RoboPol is capable of measuring both relative linear Stokes parameters q and u (and the total intensity I) in one sky exposure. Though primarily used to measure the polarization of point sources in the R band, the instrument features additional filters (B, V, and I), enabling multiwavelength imaging polarimetry over a large field of view (13.6' x 13.6'). We demonstrate the accuracy and stability of the instrument throughout its 5 yr of operation. Best performance is achieved within the central region of the field of view and in the R band. For such measurements the systematic uncertainty is below 0.1 per cent in fractional linear polarization, p (0.05 per cent maximum likelihood). Throughout all observing seasons the instrumental polarization varies within 0.1 per cent in p and within similar to 1 degrees in polarization angle.

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