The X and γ diffuse background
- 1 April 1975
- journal article
- Published by Springer Nature in La Rivista del Nuovo Cimento
- Vol. 5 (2) , 255-311
- https://doi.org/10.1007/bf02747042
Abstract
No abstract availableKeywords
This publication has 138 references indexed in Scilit:
- The Spectrum of Diffuse Cosmic X-Rays Observed by OSO-3 Between 7 and 100 KEVThe Astrophysical Journal, 1974
- Dependence of the energy per ion pair on the photon energy below 6 keV in various gasesNuclear Instruments and Methods, 1973
- Accelerator evaluation of a spark-chamber experiment for gamma-ray astronomyNuclear Instruments and Methods, 1973
- High-Energy Cosmic Gamma-Ray Observations from the OSO-3 SatelliteThe Astrophysical Journal, 1972
- Comment on Inverse Compton Models for the Isotropic X-Ray Back-Ground and Possible Thermal Emission from a Hot Intergalactic GasThe Astrophysical Journal, 1972
- Response functions for sodium iodide scintillation detectorsNuclear Instruments and Methods, 1972
- A balloon borne instrument for the study of cosmic x-raysNuclear Instruments and Methods, 1971
- A rocket payload using focusing X-ray optics for the observation of soft cosmic X-raysNuclear Instruments and Methods, 1971
- The Diffuse Cosmic X-Ray Background from 20 TO 220 keVThe Astrophysical Journal, 1970
- Intensity of the Soft X-ray Background Flux : Reply to Bowyer and FieldNature, 1970