English

Software Polarization Spectrometer "PolariS"

Instrumentation and Methods for Astrophysics 2014-12-04 v1

Abstract

We have developed a software-based polarization spectrometer, PolariS, to acquire full-Stokes spectra with a very high spectral resolution of 61 Hz. The primary aim of PolariS is to measure the magnetic fields in dense star-forming cores by detecting the Zeeman splitting of molecular emission lines. The spectrometer consists of a commercially available digital sampler and a Linux computer. The computer is equipped with a graphics processing unit (GPU) to process FFT and cross-correlation using the CUDA (Compute Unified Device Architecture) library developed by NVIDIA. Thanks to a high degree of precision in quantization of the analog-to-digital converter and arithmetic in the GPU, PolariS offers excellent performances in linearity, dynamic range, sensitivity, bandpass flatness and stability. The software has been released under the MIT License and is available to the public. In this paper, we report the design of PolariS and its performance verified through engineering tests and commissioning observations.

Keywords

Cite

@article{arxiv.1412.1256,
  title  = {Software Polarization Spectrometer "PolariS"},
  author = {Izumi Mizuno and Seiji Kameno and Amane Kano and Makoto Kuroo and Fumitaka Nakamura and Noriyuki Kawaguchi and Katsunori M. Shibata and Seisuke Kuji and Nario Kuno},
  journal= {arXiv preprint arXiv:1412.1256},
  year   = {2014}
}

Comments

18 pages, 14 figures, Accepted for Journal of Astronomical Instrumentation

R2 v1 2026-06-22T07:18:53.800Z