S. L. S. Shorlin

TL;DR: In this article, the mean longitudinal magnetic field and net linear polarization of Ap and Bp stars were measured using least squares deconvolution (LSD) profiles, which can be used to detect weak Stokes V, Q and U Zeeman signatures.

TL;DR: In this article, the Least Squares Deconvolution multi-line analysis was used to detect magnetic fields in the photospheres of 74 stars, including 22 normal B, A and F stars, four emission-line Ba nd As tars, 25 Am stars, 10 HgMn stars, two Boo stars and 11 magnetic Ap stars.

TL;DR: In this paper, the first high-quality measurements of stellar Zeeman spectral line linear polarization were obtained using the new MuSiCoS spectropolarimeter at the Pic du Midi Observatory, over 360 spectra were obtained, in circular or linear polarization, of 14 magnetic Ap/Bp stars and six calibration objects.

TL;DR: In this paper, spectropolarimetric observations of RS CVn system HR 1099 (V711 Tau) were obtained from 1998 February to 2002 January with the spectropholarimeter MuSiCoS at the Telescope Bernard Lyot (Observatoire du Pic du Midi, France).

TL;DR: In this paper, spectropolarimetric observations of the RS CVn system HR 1099 (V711 Tau) secured from 1998 February to 2002 January with the spectropholarimeter MuSiCoS at the Telescope Bernard Lyot (Observatoire du Pic du Midi, France).