PASIPHAE will measure the polarization induced by the ISM on starlight in order to map the magnetic field in 3 dimensions.

3-dimensional ISM properties and their effect on searches for B-modes

Searching for inflationary B modes: can dust emission properties be extrapolated from 350 GHz to 150 GHz? - MNRAS, 451, L90 (2015)   K. Tassis & V. Pavlidou

Maps of the number of HI clouds along the line of sight at high galactic latitude - submitted to AAS journals (2020)   G. V. Panopoulou & D. Lenz

ISM polarization far from the Galactic plane

Local Measurements of the Mean Interstellar Polarization at High Galactic Latitudes - A&A, 616, A52 (2018)   R. Skalidis, G. V. Panopoulou, K. Tassis, V. Pavlidou, D. Blinov, I. Komis, I. Liodakis

Tomography of the magnetic field

Demonstration of magnetic field tomography with starlight polarization towards a diffuse sightline of the ISM - ApJ, 872, 56 (2019)   Georgia V. Panopoulou, Konstantinos Tassis, Raphael Skalidis, Dmitriy Blinov, Ioannis Liodakis, Vasiliki Pavlidou, Stephen B. Potter, Anamparambu N. Ramaprakash, Anthony C. S. Readhead, Ingunn K. Wehus

PASIPHAE: A high-Galactic-latitude, high-accuracy optopolarimetric survey - arXiv:1810.05652
   Konstantinos Tassis, Anamparambu N. Ramaprakash, Anthony C. S. Readhead, Stephen B. Potter, Ingunn K. Wehus, Georgia V. Panopoulou, Dmitry Blinov, Hans Kristian Eriksen, Brandon Hensley, Ata Karakci, John A. Kypriotakis, Siddharth Maharana, Evangelia Ntormousi, Vasiliki Pavlidou, Timothy J. Pearson, Raphael Skalidis

Side projects

Search for AGN counterparts of unidentified Fermi-LAT sources with optical polarimetry: Demonstration of the technique - A&A, 623, A61 (2019)
   N. Mandarakas, D. Blinov, I. Liodakis, K. Kouroumpatzakis, A. Zezas, G. V. Panopoulou, I. Myserlis, E. Angelakis, T. Hovatta, S. Kiehlmann, K. Kokolakis, E. Paleologou, A. Pouliasi, R. Skalidis, V. Pavlidou

Probing the unidentified Fermi blazar-like population using optical polarization and machine learning - arXiv:1904.04278
   I. Liodakis and D. Blinov

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