The main goal of the "Pi of the Sky" experiment is to detect optical counterparts of GRBs at the very beginning and during the gamma emission or even before it. The observation strategy is based on the continuous monitoring of the large part of the sky with high temporal resolution and the fast image processing algorithms, allowing for optical transient recognition in real time. The full system will consist of 2 sites separated by a distance of the order 100 km, each site consisting of 12 custom-designed survey CCD cameras. Pairs of cameras from two sites will work in coincidence and observe the same field of view to allow rejection of false signals coming from near-earth objects. The whole system will be capable of continuous observation of about 1.5 steradian of the sky, which roughly corresponds to the field monitored by the Swift satellite. The installation of the whole system will continue in 2011.
We are very grateful for the hospitality and support we received from the BOOTES group from IAA, Granada, and from the INTA management and staff.
Some pictures from the new site (click to enlarge):
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| Where we are (green arrow) | The North landscape |
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| The open dome and cameras | The cameras close up |