English

EMPOL: an EMCCD based optical imaging polarimeter

Instrumentation and Methods for Astrophysics 2020-12-17 v1

Abstract

An Andor 1K ×\times 1K EMCCD detector has been used to develop an optical imaging polarimeter for use at the Cassegrain focus of 1.2 m telescope of PRL. The optics is derived from an older single-element detector instrument and consists of a rotating half-wave plate as modulator and a Foster prism as an analyser. The field of view of the instrument is 3 ×\times 3 sq arcmin. We describe the instrument and the observational methodology in this document. Extensive observations have been carried out with this instrument covering a large variety of sources e.g. near-Earth asteroids, comets, Lynds dark nebulae, open clusters and AGN such as blazars. In the current communication, we discuss some results from the initial calibration runs while the other results will be presented elsewhere.

Keywords

Cite

@article{arxiv.2012.08768,
  title  = {EMPOL: an EMCCD based optical imaging polarimeter},
  author = {Shashikiran Ganesh and Archita Rai and Aravind K and Alka Singh and Prachi Vinod Prajapati and Ashish Mishra and Prashanth Kasarla and Deekshya Roy Sarkar and Pitamber Singh Patwal and Namita Uppal and Sunil Chandra and Satyanarain Mathur and Amish B Shah and Kiran S Baliyan and U C Joshi},
  journal= {arXiv preprint arXiv:2012.08768},
  year   = {2020}
}

Comments

7 pages, 6 figures, Submitted to SPIE Conference Astronomical Telescopes + Instrumentation 2020

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