Search for X-rays from the region of the Aries-Perseus flasher

Details Search for X-rays from the region of the Aries-Perseus flasher Search for X-rays from the region of the Aries-Perseus flasher

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....94..429l&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 94, Aug. 1987, p. 429-430. Research supported by the Stichting Astronomisch Onderzoe

Astronomy and Astrophysics

Astronomy

4

Aries Constellation, Astronomical Spectroscopy, Radiant Flux Density, Spaceborne Astronomy, Visible Spectrum, X Ray Sources, Data Processing, Exosat Satellite, Point Sources

Scientific paper

The region containing the Perseus flasher (Katz et al., 1986) was observed for 5.4 hr with the EXOSAT observatory. Upper limits (2 σ levels of confidence) to a point source with a steady X-ray flux were 2×10-12erg cm-2s-1 (0.1 - 2 keV) and 6×10-12erg cm-2s-1 (1 - 20 keV). Upper limits (4 σ level of confidence) to X-ray flashes of ≡1 s duration were 4×10-9erg cm-2s-1 (0.1 - 2 keV) and 7×10-10erg cm-2s-1 (1 - 20 keV).

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