Towards an automatic processing of CCD images with CPCS 2.0. (arXiv:2006.05160v1 [astro-ph.IM])

Towards an automatic processing of CCD images with CPCS 2.0. (arXiv:2006.05160v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Zielinski_P/0/1/0/all/0/1">Pawel Zielinski</a> (1), <a href="http://arxiv.org/find/astro-ph/1/au:+Wyrzykowski_L/0/1/0/all/0/1">Lukasz Wyrzykowski</a> (1), <a href="http://arxiv.org/find/astro-ph/1/au:+Mikolajczyk_P/0/1/0/all/0/1">Przemyslaw Mikolajczyk</a> (2), <a href="http://arxiv.org/find/astro-ph/1/au:+Rybicki_K/0/1/0/all/0/1">Krzysztof Rybicki</a> (1), <a href="http://arxiv.org/find/astro-ph/1/au:+Kolaczkowski_Z/0/1/0/all/0/1">Zbigniew Kolaczkowski</a> (2,3,4) (1. Astronomical Observatory, University of Warsaw, 2. Astronomical Institute, University of Wroclaw, 3. Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 4. deceased)

We present a new automatic tool for time-domain astronomy – the Cambridge
Photometric Calibration Server 2.0 – developed under OPTICON H2020 programme.
It has been designed to respond to the need of automated rapid photometric data
calibration and dissemination for transient events, primarily from Gaia space
mission. CPCS has been in operation since 2013 and has been used to calibrate
around 130 000 observations of hundreds of transients. We present the status of
this tool’s development and demonstrate improvements made in the second
version. The tests present the ability to combine CCD imaging data from
multiple telescopes and a whole variety of instruments. New tool provides
science-ready photometric data within minutes from observations in the
automatic manner.

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