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Search for optical bursts from the gamma ray burst source GBS 0526-66

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dc.contributor.author Seetha, S
dc.contributor.author Sreenivasaiah, K. V
dc.contributor.author Marar, T. M. K
dc.contributor.author Kasturirangan, K
dc.contributor.author Rao, U. R
dc.contributor.author Bhattacharyya, J. C
dc.date.accessioned 2008-12-30T14:02:52Z
dc.date.available 2008-12-30T14:02:52Z
dc.date.issued 1985-08
dc.identifier.citation In NASA. Goddard Space Flight Center 19th International Cosmic Ray Conference, Vol. 1, pp 23 - 26 en
dc.identifier.uri http://hdl.handle.net/2248/4219
dc.description.abstract Attempts were made to detect optical bursts from the gamma-ray burst source GBS 0526-66 during Dec. 31, 1984 to Jan. 2, 1985 and Feb. 23 to Feb. 24, 1985, using the one meter reflector of the Kavalur Observatory. Jan. 1, 1985 coincided with the zero phase of the predicted 164 day period of burst activity from the source (Rothschild and Lingenfelter, 1984). A new optical burst photon counting system with adjustable trigger threshold was used in parallel with a high speed photometer for the observations. The best time resolution was 1 ms and maximum count rate capability was 255,000 counts s(-1). Details of the instrumentation and observational results are presented. en
dc.language.iso en en
dc.publisher NASA/STI en
dc.relation.uri http://adsabs.harvard.edu/abs/1985ICRC....1...23S en
dc.subject Gamma Ray Bursts en
dc.subject Radiation Sources en
dc.subject Light Emission en
dc.subject Photometers en
dc.subject Radiation Counters en
dc.subject Telescopes en
dc.title Search for optical bursts from the gamma ray burst source GBS 0526-66 en
dc.type Article en


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