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2. Combined spectroscopy and intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel. Issue 1 (15th June 2022)

3. Intensity interferometry of P Cygni in the H α emission line: towards distance calibration of LBV supergiant stars. Issue 1 (27th February 2020)

4. Rotational variation of the linear polarization of the asteroid (3200) Phaethon as evidence for inhomogeneity in its surface properties★. (1st August 2018)