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Optical flash background ratesFlash background rates are measured from August 18-September 5, 1985 using the Lowell 0.61-m telescope at CTIO and the 28-cm f/10 Schmidt-Cassegrain telescope at ESO. During 230.1 hours of observing 40 flash events were detected, and it was observed that the background events were dominated by meteors and satellites passing through the field-of-view. The measured flash rate is compared with that of Pedersen et al. (1984), and it is determined that the background flash rate that is applicable to the data of Pedersen et al. for February 8, 1984 is 0.023 events/hr. The morphology of that flash, which appears to be controlled by a gamma-ray burster, is examined.
Document ID
19870049715
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Schaefer, B. E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Pedersen, H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Gouiffes, C.
(European Southern Observatory Santiago, Chile)
Poulsen, J. M.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Pizzichini, G.
(CNR Istituto di Tecnologie e Studio delle Radiazioni Extraterrestri, Bologna, Italy)
Date Acquired
August 13, 2013
Publication Date
March 1, 1987
Publication Information
Publication: Astronomy and Astrophysics
Volume: 174
Issue: 1-2,
ISSN: 0004-6361
Subject Category
Astrophysics
Accession Number
87A36989
Distribution Limits
Public
Copyright
Other

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