Design of a full-Stokes polarimeter for VLT/X-shooter

Authors
  • F. Snik
  • G. van Harten
  • R. Navarro
  • P. Groot
Publication date 2012
Host editors
  • I.S. McLean
  • S.K. Ramsay
  • H. Takami
Book title Ground-based and Airborne Instrumentation for Astronomy IV
Book subtitle 1-6 July 2012, Amsterdam, Netherlands
ISBN
  • 9780819491473
Series Proceedings of SPIE
Event Ground-based and Airborne Instrumentation for Astronomy IV
Article number 844625
Volume | Issue number 2
Number of pages 15
Publisher Bellingham, WA: SPIE
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
X-shooter is one of the most popular instruments at the VLT, offering instantaneous spectroscopy from 300 to 2500 nm. We present the design of a single polarimetric unit at the polarization-free Cassegrain focus that serves all three spectrograph arms of X-shooter. It consists of a calcite Savart plate as a polarizing beam-splitter and a rotatable crystal retarder stack as a "polychromatic modulator". Since even “superachromatic" wave plates have a wavelength range that is too limited for X-shooter, this novel modulator is designed to offer close-to-optimal polarimetric efficiencies for all Stokes parameters at all wavelengths. We analyze the modulator design in terms of its polarimetric performance, its temperature sensitivity, and its polarized fringes. Furthermore, we present the optical design of the polarimetric unit. The X-shooter polarimeter will furnish a myriad of science cases: from measuring stellar magnetic fields (e.g., Ap stars, white dwarfs, massive stars) to determining asymmetric structures around young stars and in supernova explosions.
Document type Conference contribution
Language English
Published at https://doi.org/10.1117/12.926163
Other links http://adsabs.harvard.edu/abs/2012SPIE.8446E..25S
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