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Maximum-entropy image processing in gamma-ray astronomy.
DOI: 10.1093/mnras/187.2.145 Bibcode: 1979MNRAS.187..145S

Strong, A. W.; Bennett, K.; Skilling, J.

In order to make the fullest use of the information contained in data from a spark-chamber telescope, an image processing approach, is required. It is shown how the maximum-entropy reconstruction technique can be applied in a modification appropriate to a situation of low statistical weight per resolution solid angle, as usually occurs with presen…

1979 Monthly Notices of the Royal Astronomical Society
COS-B 27
Gamma rays from the Cygnus region and the nature of CG 78+1.
DOI: 10.1093/mnras/188.4.863 Bibcode: 1979MNRAS.188..863P

Strong, A. W.; Wolfendale, A. W.; Protheroe, R. J.

Interpretation of the galactic gamma-ray flux above 100 MeV has been complicated by the presence of a component due to 'point' sources of gamma-rays and by the lack of measurements of the molecular hydrogen (except along the galactic equator) which forms a large fraction of the interstellar medium (ISM). Recent CO observations of the Cygnus X regi…

1979 Monthly Notices of the Royal Astronomical Society
COS-B 10
A geometrical analysis of the gamma-ray light curves of pulsars.
DOI: 10.1093/mnras/189.4.823 Bibcode: 1979MNRAS.189..823M

Massaro, E.; Buccheri, R.; Salvati, M.

In the light curves of the COS-B gamma-ray pulsars, some common features are clearly recognizable; two main peaks always occur, and the intervening phase lag has not the natural value of 0.5. An interpretation is proposed which only involves a simplified geometrical description of the emission pattern, viz. two opposite hollow cones with a first-o…

1979 Monthly Notices of the Royal Astronomical Society
COS-B 5