# RoboPol: A four-channel optical imaging polarimeter

**Authors:** A. N. Ramaprakash, C. V. Rajarshi, H. K. Das, P. Khodade, D. Modi, G., Panopoulou, S. Maharana, D. Blinov, E. Angelakis, C. Casadio, L. Fuhrmann, T., Hovatta, S. Kiehlmann, O. G. King, N. Kylafis, A. Kougentakis, A. Kus, A., Mahabal, A. Marecki, I. Myserlis, G. Paterakis, E. Paleologou, I. Liodakis,, I. Papadakis, I. Papamastorakis, V. Pavlidou, E. Pazderski, T. J. Pearson, A., C. S. Readhead, P. Reig, A. Slowikowska, K. Tassis, J. A. Zensus

arXiv: 1902.08367 · 2019-03-06

## TL;DR

RoboPol is a four-channel optical polarimeter designed for multi-wavelength imaging polarimetry, capable of measuring linear polarization of point sources with high accuracy and stability over five years of operation.

## Contribution

The paper introduces RoboPol's design, performance, and stability, highlighting its ability to measure polarization in multiple bands simultaneously with minimal systematic errors.

## Key findings

- Achieves systematic uncertainty below 0.1% in fractional polarization
- Maintains instrumental polarization variation within 0.1% in p and 1° in angle
- Operates effectively over five years with consistent performance

## Abstract

We present the design and performance of RoboPol, a four-channel optical polarimeter operating at the Skinakas Observatory in Crete, Greece. RoboPol is capable of measuring both relative linear Stokes parameters $q$ and $u$ (and the total intensity $I$) in one sky exposure. Though primarily used to measure the polarization of point sources in the R-band, the instrument features additional filters (B, V and I), enabling multi-wavelength imaging polarimetry over a large field of view (13.6' $\times$ 13.6'). We demonstrate the accuracy and stability of the instrument throughout its five years of operation. Best performance is achieved within the central region of the field of view and in the R band. For such measurements the systematic uncertainty is below 0.1% in fractional linear polarization, $p$ (0.05% maximum likelihood). Throughout all observing seasons the instrumental polarization varies within 0.1% in $p$ and within 1$^\circ$ in polarization angle.

## Full text

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## Figures

17 figures with captions in the complete paper: https://tomesphere.com/paper/1902.08367/full.md

## References

54 references — full list in the complete paper: https://tomesphere.com/paper/1902.08367/full.md

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Source: https://tomesphere.com/paper/1902.08367