Analysis and Simulation of the Pi of the Sky Detector Response

Authors

  • L. W. Piotrowski
  • A. F. Zarnecki

DOI:

https://doi.org/10.14311/1484

Keywords:

Gamma-ray Bursts (GRB), point spread function (PSF), wide-field camera.

Abstract

The Pi of the Sky project observes optical flashes of astronomical origin and other light sources variable on short timescales, down to tens of seconds. We search mainly for optical emissions of Gamma Ray Bursts, but also for variable stars, blazars, etc. Precise photometry with a very large field of view (20?×20?) requires a careful study and modelling of a point spread function (PSF), as presented in this paper.

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Author Biographies

L. W. Piotrowski

A. F. Zarnecki

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Published

2011-01-06

How to Cite

Piotrowski, L. W., & Zarnecki, A. F. (2011). Analysis and Simulation of the Pi of the Sky Detector Response. Acta Polytechnica, 51(6). https://doi.org/10.14311/1484

Issue

Section

Articles