Hard X-ray observation of NGC 4151 with the MIFRASO telescope

During a balloon flight on July 29, 1986 of the Mifraso telescope, a region of the sky containing the Seyfert galaxy NGC 4151 was studied over the photon energy range 15-300 keV. A 5.5 sigma excess, interpreted as originating from the direction of NGC 4151, was detected in the energy band 27-80 keV....

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Veröffentlicht in:The Astrophysical journal 1990-06, Vol.356 (2), p.467-471
Hauptverfasser: PEROTTI, F, BURATTI, R, DIPPER, N. A, LEWIS, R. A, MAGGIOLI, P, QUADRINI, E, BAZZANO, A, UBERTINI, P, BASSANI, L, STEPHEN, J. B, COURT, A. J, DEAN, A. J
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Sprache:eng
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Zusammenfassung:During a balloon flight on July 29, 1986 of the Mifraso telescope, a region of the sky containing the Seyfert galaxy NGC 4151 was studied over the photon energy range 15-300 keV. A 5.5 sigma excess, interpreted as originating from the direction of NGC 4151, was detected in the energy band 27-80 keV. The corresponding emission spectrum may be represented by a single power law with a photon spectral index of alpha = 1.5 + or - 0.6. The result is compared to previous hard X-ray observations of this source. Apart from this measurement, an observation of the Crab Nebula as an in-flight calibration source of the telescope is described. 33 refs.
ISSN:0004-637X
1538-4357
DOI:10.1086/168854