For the first time the birth of a black hole have been filmed. Cameras of the "Pi of the Sky" project recorded this remarkable event with 4 minutes sequence of 10 seconds long images. In almost 20 seconds the object became so bright that it could be visible with the naked eye. Then it begun fading and in 4 minutes it became 100 times fainter. At that time the observation was taken over by larger telescopes.
The "Pi of the Sky" observation combined with the Swift satellite gamma-ray data for the first time confirmed with 10s precision that optical emission starts simultaneously with the gamma-ray burst. Optical observations during the first seconds of the burst are crucial to understand the mechanism of releasing such huge energy.
This observation was the proof of the novel concept of the "Pi of the Sky" project. Usually, optical emission from GRB is observed by telescopes listening to alerts from satellite gamma ray detectors. Signal distribution and turning the telescope take some time and the very first minute of the outburst cannot be observed. The principle of the "Pi of the Sky" project is different. The apparatus monitors continuously large fraction of the sky taking 10s exposures and detects optical flashes independently, while the satellite information confirms the origin of the flash. Currently "Pi of the Sky" apparatus consists of two cameras installed in Las Campanas Observatory. They cover 20x20 degree of the sky. To increase the chance of observing a GRB 32 new cameras are under construction. They will cover 1/3 of the visible sky continuously. Original plan was to cover pi (~3.14) steradians of the sky, giving the name for the project. The name recalls also the title of John Barrow book "Pi in the sky" arguing that the phenomena we observe are governed by physical laws expressed in mathematical language.
The “Pi of the Sky” project was inspired by Bohdan Paczynski, great astrophysicist who past away last year. He contributed a lot to the understanding of GRBs and he always claimed that small telescopes have large potential for sky surveys.
The project is conducted by collaboration of Polish research institutes: Soltan Institute for Nuclear Studies (Warsaw), Center for Theoretical Physics PAS (Warsaw), Warsaw University, Warsaw University of Technology, Space Research Center PAS (Warsaw), University of Cardinal Stefan Wyszynski (Warsaw), Pedagogical University of Cracow.
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