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  • Blinov, D.; Maharana, S.; Bouzelou, F.; Casadio, C.; Gjerløw, Eirik; Jormanainen, J.; Kiehlmann, S.; Kypriotakis, J.A.; Liodakis, I.; Mandarakas, N.; Markopoulioti, L.; Panopoulou, G.V.; Pelgrims, V.; Pouliasi, A.; Romanopoulos, S.; Skalidis, R.; Anche, R.M.; Angelakis, E.; Antoniadis, J.; Medhi, B.J.; Hovatta, T.; Kus, A.; Kylafis, N.; Mahabal, A.; Myserlis, I.; Paleologou, E.; Papadakis, I.; Pavlidou, V.; Papamastorakis, I.; Pearson, T.J.; Potter, S.B.; Ramaprakash, A.N.; Readhead, A.C.S.; Reig, P.; Słowikowska, A.; Tassis, K.; Zensus, J.A. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2023)
    Context. Optical polarimeters are typically calibrated using measurements of stars with known and stable polarization parameters. However, there is a lack of such stars available across the sky. Many of the currently ...