Result: Search for optical flashes accompanying gamma ray bursts Pi of the Sky collaboration

Title:
Search for optical flashes accompanying gamma ray bursts Pi of the Sky collaboration
Source:
Photonics applications in astronomy, communications, industry, and high-energy physics experiments II (Wilga, 21-25 May 2003)SPIE proceedings series. :283-289
Publisher Information:
Bellingham WA: SPIE, 2004.
Publication Year:
2004
Physical Description:
print, 8 ref
Original Material:
INIST-CNRS
Document Type:
Conference Conference Paper
File Description:
text
Language:
English
Author Affiliations:
Soltan Institute for Nuclear Studies, Warsaw, Poland
Institute of Experimental Physics, Warsaw University, Poland
Institute of Electronic Systems, Warsaw University of Technology, Poland
Center for Theoretical Physics PAS, Warsaw, Poland
Rights:
Copyright 2004 INIST-CNRS
CC BY 4.0
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
Notes:
Astronomy
Accession Number:
edscal.16294920
Database:
PASCAL Archive

Further Information

Perhaps the most powerful cosmic processes ever observed are gamma ray bursts (GRB). So far, phenomena responsible for GRB have not been unambiguously identified. In the present paper we propose an approach completely different from the classical one. It employs experimental techniques developed for particle physics. Presented project is pioneering research in the unexplored so far domain of cosmic phenomena on the time scale of seconds. Both the rate of signal in question and the rate of unexpected background are not known. Therefore we decided to divide the project into two phases: phase I -two CCD cameras, phase II - a system of cameras covering all sky. The phase I is well defined whereas detailed realization of phase II will depend strongly on results and experience gained in phase I.