Commissioning of the Dual-Beam Imaging Polarimeter for the UH 88-inch telescope
arXiv:0708.1335 · doi:10.1086/522379
Abstract
In this paper we present the design, calibration method, and initial results of the Dual-Beam Imaging Polarimeter (DBIP). This new instrument is designed to measure the optical polarization properties of point sources, in particular Main Belt asteroids. This instrument interfaces between the Tek 2048x2048 camera and the University of Hawaii's 88-inch telescope, and is available for facility use. Using DBIP we are able to measure linear polarization with a 1-sigma Poisson signal noise of 0.03% per measurement and a systematic error of order 0.06% +/- 0.02%. Additionally, we discuss measurements of the polarization of the asteroid 16 Psyche which were taken as part of the instrument commissioning. We confirm Psyche's negative polarization of -1.037% +/- 0.006% but find no significant modulation of the signal with rotation above the 0.05% polarization level.
Accepted to PASP
Cited by in corpus (5)
- Alignment of quasar polarizations with large-scale structures
- Linear spectropolarimetry of polarimetric standard stars with VLT/FORS2
- Polarization of asteroid (387) Aquitania: the newest member of a class of large inversion angle asteroids
- The IRCAL Polarimeter: Design, Calibration, and Data Reduction for an Adaptive Optics Imaging Polarimeter
- Dual-Beam Optical Linear Polarimetry from Southern Skies. Characterisation of CasPol for high precision polarimetry