Polarimetric imaging mode of VLT/SPHERE/IRDIS - II. Characterization and correction of instrumental polarization effects,

R. G. van Holstein; J. H. Girard; J. de Boer; F. Snik; J. Milli; D. M. Stam; C. Ginski; D. Mouillet; Z. Wahhaj; H. M. Schmid; C. U. Keller; M. Langlois; K. Dohlen; A. Vigan; A. Pohl; M. Carbillet; D. Fantinel; D. Maurel; A. Origné; C. Petit; J. Ramos; F. Rigal; A. Sevin; A. Boccaletti; H. Le Coroller; C. Dominik; T. Henning; E. Lagadec; F. Ménard; M. Turatto; S. Udry; G. Chauvin; M. Feldt; J.-L. Beuzit

doi:10.1051/0004-6361/201834996

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Volume 633 (January 2020)

A&A, 633 (2020) A64

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Fig. 15.

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Normalized Stokes parameters of the measured stellar polarization of T Cha as function of HWP cycle after applying our correction method.

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