Balloon-borne observations of NGC 4511 using the MISO telescope

Details Balloon-borne observations of NGC 4511 using the MISO telescope Balloon-borne observations of NGC 4511 using the MISO telescope

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...8018998p&link_type=abstract

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Balloon-Borne Instruments, Seyfert Galaxies, Spectrum Analysis, X Ray Telescopes, Emission Spectra, Gamma Rays, Stellar Spectra

Scientific paper

The Seyfert Galaxy NGC 4151 was observed from balloon altitudes using the MISO low energy gamma-ray telescope on May 23, 1977. The spectrum was measured over the range 0.04 to 20 MeV and a change in the spectral index was observed at about 2 MeV. The data at low energies are in good agreement with other hard X-ray data, but at higher energies the data are consistent with an exponential spectrum having an e-folding energy of 2.1 MeV.

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